Have you ever dreamed of walking on the Moon or exploring the mysteries of space? NASA’s Artemis mission is a program that will make those dreams a reality. The Artemis program aims to land humans on the Moon, establish a long-term presence on and around the Moon, and eventually send astronauts to Mars. But the mission is not just about exploration and discovery. Artemis will also demonstrate new technologies and inspire the next generation of space explorers.

Now you probably be wondering,

What is NASA’s Artemis mission?

Artemis is the name of NASA’s program that seeks to achieve multiple objectives. The program aims to land humans on the Moon, establish a long-term human presence on and around the Moon, and eventually send astronauts to Mars. To achieve these goals, Artemis will rely on innovative technologies to explore more of the lunar surface than ever before, and NASA will collaborate with commercial and international partners.

The Artemis program has set forth several objectives that it aims to achieve. One of its key objectives is to demonstrate new technologies, capabilities, and business approaches needed for future exploration, including Mars. In addition, Artemis seeks to study the Moon to gain insights into the origin and history of Earth, the Moon, and our solar system.

Furthermore, the program aims to establish American leadership and a strategic presence on the Moon, expanding U.S. global economic impact. It also seeks to broaden commercial and international partnerships, which will be crucial for the program’s success. Finally, Artemis aims to inspire a new generation and encourage careers in STEM, positioning the next generation to lead future space exploration missions.

Here is,

Some amazing facts about Artemis Mission!

  1. Artemis is named after the twin sister of Apollo and the goddess of the Moon in Greek mythology.
  2. NASA chose the name to symbolize its efforts to return astronauts, science payloads, and technology demonstrations to the lunar surface.
  3. The tip of the A in the Artemis logo points beyond the Moon to signify that the Moon is not the end goal but rather a preparation for future exploration beyond it.
  4. The crescent in the logo represents missions from the perspective of the audience, with the focus on going from Earth to the Moon and returning with knowledge and development.
  5. The crescent also resembles Artemis’ bow, which represents the source of energy and effort sent toward the Moon.
  6. The Moon is the primary destination for the Artemis program and a stepping stone toward Mars.
  7. The trajectory in the logo moves from left to right through the crossbar of the A, highlighting the differences in the return to the Moon compared to the Apollo missions.
  8. The red color of the trajectory represents the course to Mars.
  9. The A in the logo represents an arrowhead from Artemis’ quiver and symbolizes the launch of missions.

Let’s start with the,

Artemis 1!

After four delays, Artemis 1 was launched on November 16 at 1:47 am EST (6:47 am GMT). Artemis I is NASA’s first flight test of their deep space exploration system, including the Orion spacecraft, Space Launch System (SLS) rocket, and ground systems at Kennedy Space Center in Cape Canaveral, Florida. This uncrewed mission is the first in a series of increasingly complex missions that are establishing a foundation for human deep space exploration and demonstrating NASA’s commitment and capability to extend human existence to the Moon and beyond.

Now, here is the,

Map of Artemis 1!

Map of Artemis 1

Artemis 1 was a test flight of the Space Launch System (SLS) rocket and the Orion spacecraft, designed to demonstrate their ability to travel to the Moon and beyond. The mission began on November 30, 2021, with the launch of the SLS rocket from NASA’s Kennedy Space Center in Florida. The spacecraft traveled a total distance of approximately 450,000 kilometers to the Moon, where it entered a lunar orbit at an altitude of 400 kilometers above the lunar surface. This was followed by a trans-lunar injection burn that sent the spacecraft approximately 64,373 kilometers beyond the Moon and into deep space.

During the mission, the spacecraft carried out a series of tests and maneuvers, including a flyby of the Moon, a test of the Orion spacecraft’s heat shield, and a demonstration of its communication and navigation systems. On December 11, 2021, after a mission lasting 25.5 days, the module landed in the Pacific Ocean close to California. The mission was a significant milestone in NASA’s Artemis program, which aims to return humans to the Moon and establish a sustainable presence there by the end of the decade.

It’s worth noting that the Space Launch System is the most powerful rocket ever built, generating 8.8 million pounds of thrust on liftoff. This makes it 1.3 million pounds more powerful than the Saturn V rocket used in the Apollo missions, and capable of carrying larger payloads and traveling further into space.

Continuing with the mission briefing,

What is the current status of the Artemis 1 mission?

NASA’s Artemis I mission, an uncrewed flight test, successfully demonstrated the agency’s deep space rocket, spacecraft, and ground systems readiness for future missions to the Moon. Engineers have extensively reviewed data since the mission’s completion to confirm the initial observations, including the performance of the Space Launch System (SLS) rocket and Orion spacecraft. The SLS rocket flew precisely as designed, meeting or exceeding performance expectations, while the Exploration Ground Systems program is repairing damaged components and making upgrades in preparation for future Artemis missions.

The Orion spacecraft successfully performed every aspect of its journey beyond the Moon, including generating more power than expected and consuming less power than predicted. NASA is examining two observations from the flight in more detail: variations across the appearance of Orion’s heat shield and an issue where latching current limiters switched open without commanding several times throughout the mission. Despite these issues, NASA is making progress towards the Artemis II mission, with the heat shield set to be attached to the crew module in May and the mobile launcher undergoing testing this summer. The agency is determined to ensure crew safety is a top priority for future missions.

Now let’s dig in to find out,

Artemis 2!

Artemis II marks a significant milestone in NASA’s quest for deep space exploration, as it will be the first manned mission of the Orion spacecraft, Space Launch System rocket, and ground systems at Kennedy Space Center. With four astronauts aboard, the mission will test the spacecraft’s systems in the actual environment of deep space and confirm their operational readiness for future missions. The Artemis II flight test will be crucial in paving the way for the historic Artemis III mission, which aims to land the first woman and next man on the Moon.

Here is,

Map of Artemis 2!

Map of Artemis 2

Artemis 2 is the second planned mission of NASA’s Artemis program and is currently scheduled for launch in 2024. The mission will be crewed by four astronauts and will be the first time humans have traveled beyond low Earth orbit since the Apollo 17 mission in 1972. The mission will be launched into space by the Space Launch System (SLS) rocket, and the crew will fly the Orion spacecraft to a distance of 7402 kilometers beyond the Moon’s far side. This will be followed by a lunar flyby, allowing the crew to observe and study the lunar surface from a closer distance.

The spacecraft will then return to Earth, and the mission is expected to take between eight to ten days to complete. During the mission, the crew will collect valuable flight test data that will help NASA refine its plans for future crewed missions to the Moon and beyond. It’s worth noting that Artemis 2 is a crucial step towards NASA’s goal of returning humans to the Moon and establishing a sustainable presence there by the end of the decade. By testing the Orion spacecraft and the SLS rocket in a crewed mission beyond low Earth orbit, NASA will be one step closer to achieving this goal.

Now here are some more details on this mission,

What is the current status of the Artemis 2 mission?

NASA’s Artemis II, the first crewed Artemis mission that will send four astronauts around the Moon and return them home, has achieved a significant milestone in its development. All five major Space Launch System (SLS) rocket’s core stage structures have been fully integrated by teams at NASA’s Michoud Assembly Facility in New Orleans. The engine section, which is located at the bottom of the 212-foot-tall core stage, was joined to the rest of the rocket stage on March 17. The next step will be to integrate the four RS-25 engines into the engine section to complete the stage.

The engine section is the most complex and intricate part of the rocket stage, housing the engines and including vital systems for mounting, controlling, and delivering fuel from the propellant tanks to the engines. The RS-25 engines and the two solid rocket boosters, which together generate 8.8 million pounds of thrust at takeoff, also attach to it. The core stage for Artemis II is built, outfitted, and assembled at Michoud. Through Artemis missions, NASA aims to land the first woman and the first person of color on the surface of the Moon, paving the way for a long-term lunar presence and serving as a stepping stone for astronauts on the way to Mars.

 

Published by: Sky Headlines

The space race has always been a source of excitement and awe, with every new development pushing the limits of human knowledge and technology. NASA’s CAPSTONE Mission is no exception, representing a new era of innovation and exploration. This spacecraft is set to make history by testing cutting-edge systems and technologies in space, paving the way for future lunar missions and human exploration of the moon. CAPSTONE will change our understanding of the universe and space exploration with its mission objectives and goals.

Come along as we delve into the specifics of this astounding mission and the future it could unlock. So,

What is NASA’s CAPSTONE?

The CAPSTONE, or Cislunar Autonomous Positioning System Technology Operations and Navigation Experiment, is one of NASA’s first spacecraft to fly in a near-rectilinear halo orbit (NRHO). This innovative spacecraft, developed by Advanced Space and propelled by Stellar Exploration, is a 12U CubeSat type. So, it will take on the role of a trailblazer by demonstrating cutting-edge technologies and operations in space. With a total cost of around $30 million.

NASA's CAPSTONE
Credits: Illustration by NASA/Daniel Rutter

CAPSTONE’s primary mission is set to last six months. But it has the potential to continue operating for an additional year or more in an extended mission. Scheduled to launch on June 28th, 2022, aboard an Electron/Photon HyperCurie rocket from Rocket Lab’s Mahia Launch Complex in New Zealand, CAPSTONE has entered the Near-Rectilinear Halo Orbit (NRHO) around the moon on November 14th, 2022.

You should also know,

What is the purpose of the CAPSTONE satellite?

CAPSTONE’s mission objectives are extensive and include many significant accomplishments for future lunar missions. One of its key objectives is to verify the characteristics of a cis-lunar near rectilinear halo orbit. Also, it will help determine its usefulness for future spacecraft. The main goal of CAPSTONE’s mission is to test out new systems and technologies in space as part of a technology demonstration. In addition to its role as a trailblazer, CAPSTONE will also serve as a vital component of NASA’s larger Lunar Gateway program. Moreover, it aims to establish a permanent human presence on the moon.

Artemis Moon Program!
Image Credits: Illustration by NASA/Daniel Rutter

Anyhow,

One of CAPSTONE’s main goals is to test a new navigation system that will allow it to measure its position relative to NASA’s Lunar Reconnaissance Orbiter (LRO) without relying on ground stations. This system will help pave the way for future lunar missions by enabling spacecraft to navigate autonomously and more efficiently in space. With its arrival in lunar orbit on November 14, 2022, CAPSTONE is about to finish its six-month mission to orbit the moon, collect data, and test new technologies that will help us learn more about and explore our neighbor in the sky.

Now you might be thinking,

Did CAPSTONE reach the Moon?

The CAPSTONE mission operations team verified that the CAPSTONE spacecraft entered the Moon’s orbit on November 13, 2022. At 7:39 p.m. EST, the CubeSat executed its first orbit insertion maneuver by firing its thrusters to place the spacecraft into orbit. CAPSTONE is currently in an NRHO or near-rectilinear halo orbit. This NRHO is the same orbit that will support the Artemis missions of NASA. CAPSTONE is the first spacecraft to fly an NRHO and the first CubeSat to function on the Moon.

NASA's pathfinding moon CubeSat
Image Credits: Illustration by NASA/Daniel Rutter

Moreover, Let’s find out,

What is the current status of NASA’s Capstone?

The CAPSTONE spacecraft is currently operating successfully in a Near Rectilinear Halo Orbit (NRHO) around the Moon, fulfilling its mission objectives. The spacecraft has completed approximately 12.5 orbits since its arrival on November 13th and has operated successfully through two lunar eclipses. So this presented challenges for its thermal and power systems. The spacecraft has also executed two maintenance maneuvers to keep it in its desired orbit.

The CAPSTONE team has completed interface testing with the Lunar Reconnaissance Orbiter ground systems and is preparing for further experiments. It includes crosslink experiments with LRO and technology demonstrations using the Cislunar Autonomous Positioning System (CAPS). The spacecraft still has approximately 56% of its fuel remaining. Hence, it provides a significant margin to operate in the NRHO for the planned mission duration and beyond. The CAPSTONE mission team has satisfied its fourth mission objective of disseminating lessons learned from the mission by publishing several papers related to mission operations and program development. The team plans to publish additional papers in the future detailing their upcoming plans in the NRHO.

 

Published by: Sky Headlines

NASA and a private company called Axiom Space showed off new spacesuits that will be used by astronauts when they go to the Moon. These suits are Axiom Extravehicular Mobility Units or AxEMUs. They’re better than Apollo and ISS suits. The new suits were only partially shown so the design would not be copied. An extra layer of fabric only for display is covering the new Axiom Space xEMU spacesuits.

The primary reason for using this cover layer is to hide the specific details and design of the spacesuit since they are proprietary, meaning they are owned by Axiom Space and not meant to be revealed to the public or competitors. The press release also explains that the spacesuit will be white, as it needs to reflect heat and protect astronauts from the extremely high temperatures on the Moon.

What is the difference between this suit and the new AxEMU spacesuit?

Compared to the Apollo suits, the new xEMU spacesuits are one-piece suits with a “hatch” on the back, which is a back entry design that allows astronauts to step into the suit from behind. The suit has a hard torso that provides the core structure, arms and legs, and various mobility joints. The arms and legs can be changed out for custom fitting, which provides a better fit for the individual astronaut.

Additionally, the AxEMU spacesuit has a portable life support system on the back that provides life support systems for heat and cooling, air to breathe, and even food and water. The helmet bubble is mounted to the hard upper torso, and on top is the visor assembly that includes lights to allow astronauts to see in shadowed areas or during the lunar night. The new gloves and boots are designed to be more flexible and durable, allowing astronauts to work longer hours on the lunar surface.

xEMU spacesuits
Axiom Space engineer Jim Stein wears the prototype of the new AxEMU. Via NASA TV

However, we got to see that they are more functional and flexible than older suits,

How to get inside the xEMU spacesuits?

The suit is a one-piece suit with a hard torso that provides the core structure of the suit and arms and legs with various mobility joints. It can change out the legs and arms for fitting. To get into the suit, the astronaut would first approach the suit from the back, where there is a hatch or opening. They would then open the hatch and step into the suit one leg at a time. And pull  it up to their waist. They would then slip their arms into the arm openings, which have a variety of mobility joints to allow for flexibility.

spacesuits for moon exploration
Credit: Axiom Space

Once the arms are in, the astronaut would put on the helmet. The helmet is then attached to the hard upper torso of the xEMU spacesuits. The visor assembly is located on top of the helmet bubble. The visor assembly includes lights that help astronauts see in shadowed areas or during the lunar night. The backpack is located on the rear of the spacesuit. The backpack contains life support systems that provide cooling and heat, air to breathe, and even food and water to the astronaut. Once the backpack is attached, the astronaut is ready to go outside and perform a spacewalk or extravehicular activity (EVA).

Now, you might be wondering,

Who demonstrates the suit by putting the suit on?

Axiom Space engineer Jim Stein wore a prototype of the new suit and demonstrated it by walking around, doing squats, lunges, kneeling, and more. As well as displaying how much flexibility the arms of the new suit provided.

NASA’s Extravehicular Activity and Human Surface Mobility Program office are based at the Johnson Space Center (JSC). The program office conducted ten years of research on spacesuits for lunar activities, including moonwalks. He shared research findings with Axiom, the designers of the xEMU spacesuits. Axiom used this information to develop the new AxEMU spacesuit. The next astronauts landing on the Moon will wear this new spacesuit.

advanced AxEMU spacesuits
A view of the back of the new AxEMU suit. To the right is Russell Ralston, deputy program manager for Extravehicular Activity at Axiom Space. Via NASA TV.

Let’s find out,

What are the experts’ remarks on this?

Lara Kearney is the program manager. She explains that developing a spacesuit for the Artemis missions was challenging due to the Moon’s harsh environment. In particular, the south pole’s temperature requirements presented a significant challenge. The team aimed to make the new suit more mobile than the Apollo suits to improve astronaut movement. However, they also leveraged their past knowledge and experience to guide Axiom Space in developing the new spacesuit.

NASA’s Johnson Space Center Director Vanessa Wyche says NASA has not created a new astronaut spacesuit in the last 40 years. The last time NASA created new spacesuits was for the Space Shuttle program. Therefore, the collaboration with Axiom Space has created a new spacesuit, the AxEMU, which Wyche describes as being more functional. She adds that NASA will collaborate with Axiom Space to make the new spacesuit safe for astronauts.

 

Published by: Sky Headlines

The universe is full of mysteries, and one of the biggest is whether or not an asteroid could hit Earth in a way that would be very terrible. It’s hard to imagine the severity of the damage and lives that could be lost in such a tragedy. But what if there were some way to stop a catastrophe of this scale? So this is where DART comes in. The DART mission is a fascinating and challenging task that could alter the path of human events by revealing new ways to safeguard Earth from asteroids.

But firstly we should know that,

What is this Dart?

DART, short for Double Asteroid Redirection Test, is a planetary defense mission led by NASA and the Laboratory of Applied Physics of Johns Hopkins University. The mission’s primary objective is to test the effectiveness of a technique called a kinetic impactor. Hence, it involves redirecting the path of an asteroid by colliding with a spacecraft into it at high speed.

The spacecraft, also called the DART impactor, was launched on November 23, 2021, on a SpaceX Falcon 9 rocket from Vandenberg, SLC-4E. The DART impactor weighs 610 kg. It carries a CubeSat called LICIACube, which was deployed six months and four days into the mission. The target of the DART mission is the Didymos system. It is a binary asteroid system consisting of two objects – the primary asteroid Didymos and its smaller moonlet called Dimorphos. The DART impactor is expected to collide with Dimorphos on September 26, 2022, at a distance of 56.7 km from the Didymos system.

Here arises the question,

What is the purpose of DART?

The Double Asteroid Redirection Test (DART) mission aims to test if intentionally crashing a spacecraft into an asteroid is an effective way to change its pathway to respond to a potential asteroid impact threat. DART’s target is the binary asteroid system Didymos, composed of two asteroids – Didymos and Dimorphos. The DART spacecraft impacted Dimorphos. It is a smaller moonlet asteroid orbiting Didymos, nearly head-on, shortening the time it takes Dimorphos to orbit Didymos by 33 minutes. The scientists designed the impact carefully to bring Dimorphos’s orbit slightly closer to Didymos. But the system is not on a path to collide with Earth and poses no actual threat. The DART demonstration tests technology and capability to respond to a future asteroid impact threat, should one ever be discovered.

Furthermore, you need to find out,

What are the main objectives of DART’s mission?

The Double Asteroid Redirection Test (DART) mission has several key objectives, which include testing our ability to achieve a kinetic impact on an asteroid and observing its response. The primary objective of the mission is to demonstrate a kinetic impact with the smaller moonlet asteroid Dimorphos. It orbits the larger asteroid Didymos in a binary system. Another key objective is to change the binary orbital period of Dimorphos by using DART’s kinetic impact. So, an investigation team will measure it using telescopes on Earth. It observes how much the impact has changed the asteroid’s motion in space.

Additionally, the DART mission aims to engage the international planetary science community and foster worldwide cooperation to address the global issue of planetary defense. The use of ground-based telescope observations before and after the impact will allow for precise measurements of Dimorphos’ period change. Moreover, the mission seeks to measure the effects of the impact and resulting ejecta on Dimorphos. As it provides valuable insights into the behavior of asteroids and their response to impacts. By achieving these objectives, the DART mission will help advance our understanding of planetary defense and our ability to mitigate potential asteroid impact threats.

Now, come to the discussion that,

Was the NASA DART mission successful or not?

NASA has recently confirmed that the Double Asteroid Redirection Test (DART) mission has successfully changed the orbit of an asteroid. It marked the first time humans have intentionally altered the motion of a celestial object. Hence, by colliding with the smaller moonlet asteroid, Dimorphos, DART impacted its target asteroid, Didymos, in successfully demonstrating asteroid deflection technology. The impact reduced the time it takes for Dimorphos to orbit Didymos by 32 minutes, down from the previous 11 hours and 55 minutes. This margin of error is around plus or minus 2 minutes. NASA had set a minimum goal of a 73-second orbit period change. The DART mission surpassed it by over 25 times. Astronomers on Earth have been using telescopes to measure the change in orbit since the impact occurred on September 26, 2022.

Moreover, let’s find out,

What are experts’ views on this mission?

The DART coordination lead from the Johns Hopkins Applied Physics Laboratory (APL) in Laurel. Maryland “Nancy Chabot,” says: “DART has given us some fascinating data about both asteroid properties and the effectiveness of a kinetic impactor as a planetary defense technology,” Moreover, she explains: “The DART team is continuing to work on this rich dataset to fully understand this first planetary defense test of asteroid deflection.”

Bill Nelson, NASA’s Administrator, says: “All of us have a responsibility to protect our home planet. After all, it’s the only one we have”. Moreover, he explains: “This mission shows that NASA is trying to be ready for whatever the universe throws at us. NASA has proven we are serious as a defender of the planet. This is a watershed moment for planetary defense and all of humanity.  Demonstrating commitment from NASA’s exceptional team and partners from around the world.”

The Director of NASA’s Planetary Science Division at NASA Headquarters in Washington is Lori Glaze. She says: “This result is one important step toward understanding the full effect of DART’s impact with its target asteroid”.  While, she added: “As new data come in each day, astronomers will be able to better assess. They will assess whether, and how, a mission like DART could be used in the future. It will help protect Earth from a collision with an asteroid if we ever discover one headed our way.”

So, here comes the point,

What are researchers looking forward to for this mission?

The investigation team is currently focused on gathering more data with ground-based observatories and radar facilities to improve the precision of the period measurement of Dimorphos. While this is ongoing, attention has shifted towards measuring the efficiency of momentum transfer from DART’s impact with the asteroid. This involves analyzing the ejecta. As it is the debris launched into space by the impact, to better understand how it affected DART’s push against Dimorphos. To do this, the team needs more information on the physical properties of the asteroid. It includes the characteristics of its surface and its strength.

Investigaters are investigating these issues currently. As the astronomers continuing to study imagery of Dimorphos from DART’s terminal approach and the Light Italian CubeSat for Imaging of Asteroids (LICIACube). In approximately four years, scientists has planned the European Space Agency’s Hera project  to conduct detailed surveys of both Dimorphos and Didymos. They focus on the crater left by DART’s collision and precise measurement of Dimorphos’ mass. This future mission will provide valuable insights into the effects of DART’s impact on the asteroid. And then it is aid in the development of future planetary defense strategies.

 

Published by: Sky Headlines

On January 28, 1986, a catastrophic event occurred that shocked the world and forever changed the future of space exploration. At 11:39:13 EST (16:39:13 UTC), the Space Shuttle Challenger, with its crew of seven aboard, broke apart just 73 seconds into its flight, losing all crew members. The Challenger disaster occurred off the coast of Florida, in the Atlantic Ocean, and was caused by the failure of an O-ring seal in the right Solid Rocket Booster (SRB), due to cold weather and wind shears. The impact of this tragedy was profound, leading to the cancellation of the Teacher in Space Project and subsequent civilian shuttle spaceflights, as well as the grounding of the entire Shuttle fleet for the implementation of new safety measures.

Let’s find out,

Construction and Features:

Challenger disaster
Credit: NASA

NASA’s second Space Shuttle orbiter, Challenger (OV-099), was a Structural Test Item (STA-099). The decision to build STA-099 was made due to the low production rate of the Orbiters, which made it necessary to have a prototype vehicle that could be converted into a flight vehicle later on. The purpose of the STA-099 was to undergo structural testing to validate computational models and to show compliance with the required 1.4 factor of safety. The testing was performed to a safety factor of 1.2 times the design limit loads to prevent damage during structural testing.

NASA initially planned to convert the prototype orbiter, Enterprise (OV-101), which was used for flight testing, as the second operational orbiter. But, design changes made during the construction of the first orbiter, Columbia (OV-102), would have required considerable rework. Although STA-099’s qualification testing averted damage, NASA found that reconstructing STA-099 as OV-099 would be less expensive than refitting Enterprise.

Challenger had some design modifications as compared to its predecessor, Columbia. Most of the tiles on the payload bay doors, top wing surface, and rear fuselage surface were replaced with DuPont white Nomex felt insulation, resulting in a Thermal Protection System with fewer tiles. This change allowed Challenger to carry a more payload of 2,500 lb (1,100 kg) than Columbia. Challenger was the first orbiter to carry a head-up display system.  Scientists used the system during the descent phase of a mission. The head-up display supplied crucial information to the crew during the landing.

Moreover, it comes about

Flights and Modifications:

Challenger made its first flight on April 4, 1983, and quickly became the primary orbiter in NASA’s Space Shuttle fleet, flying more missions per year than Columbia. In fact, between 1983 and 1984, Challenger flew on 85% of all Space Shuttle missions. Challenger, Discovery, and other Space Shuttles were in heavy use during the early 1980s. It flew three missions a year from 1983 to 1985. Challenger and Discovery underwent modifications at Kennedy Space Center. The modifications allowed them to carry the Centaur-G upper stage in their payload bays. Challenger’s next mission, had STS-51-L been successful, was to deploy the Ulysses probe with the Centaur. The Ulysses probe would have studied the polar regions of the Sun.

Challenger achieved many milestones during its spaceflight career. The milestones included being the first for many groups, such as the first American woman, African-American, and Canadian in space. Challenger also completed three Spacelab missions and performed the Space Shuttle’s first night launch and landing. However, Challenger is most remembered for the tragic loss of the orbiter and its seven-member crew. The loss occurred on January 28, 1986, during mission STS-51-L.  The debris of the vessel was collected and stored in decommissioned missile silos at Cape Canaveral Air Force Station. Occasionally, different pieces of debris from the orbiter wash up on the Florida coast and are transported to the silos for storage. It’s worth noting that Challenger was the only Space Shuttle that never wore the NASA “meatball” logo, due to its early loss.

Here is to discuss,

What was the disaster Of Challenger?

Space Shuttle Challenger
Credit: NASA

Tragically, Challenger met its demise during its tenth mission, STS-51-L, on January 28, 1986. The Space Shuttle was destroyed just 73 seconds into the flight, at an altitude of approximately 46,000 feet. The cause of the Challenger disaster was later determined to be an O-ring seal failure on the right solid rocket booster (SRB). The O-rings failed to seal properly due to various factors, including cold weather. A plume of flame was able to escape from the SRB due to the failed O-ring seal.

The escaping flame caused the structural failure of the external fuel tank (ET) and the SRB. The structural failure of the ET and SRB caused the vehicle to break apart. The break-up of the vehicle occurred under the stress of aerodynamic loads. The loss of the seven crew members on board was a tragic outcome of the disaster. The Challenger disaster was a significant setback for the Space Shuttle program. They grounded the Space Shuttle fleet for nearly three years as a result of the tragedy.

When it comes about,

The views of Janet Petro

Janet Petro, who is the Kennedy Space Center Director, says: “Challenger and her crew live on in the hearts and memories of both NASA and the nation,” Moreover, she added: “Today, as we turn our sights again toward the Moon and Mars, we see that the same love of exploration that drove the Challenger crew is still inspiring the astronauts of today’s Artemis Generation, calling them to build on the legacy of knowledge and discovery for the benefit of all humanity.”

Lastly,

When did the world see Challenger’s sad loss?

January 28, 1986, the world saw the Challenger’s sad loss. President Ronald Reagan appointed a special commission to investigate the cause of the disaster. The commission was tasked with developing corrective measures. Former secretary of state William Rogers led the commission. The commission included notable figures such as former astronaut Neil Armstrong and former test pilot Chuck Yeager.

The investigation found an “O-ring” seal failed in one of the two solid-fuel rockets. The O-ring was to be elastic and pliable. The O-ring did not respond as expected due to the cold temperature at launch time. The failure of the O-ring caused a breach in the seal. Hot gases escaped through the breach and damaged critical parts of the space shuttle. The damage caused by the hot gases led to the catastrophic failure of the Challenger.

As a result of the investigation, NASA suspended all manned spaceflights for more than two years while it redesigned and improved various features of the space shuttle. The commission’s recommendations led to changes in NASA’s safety protocols and a renewed focus on safety in the space program. The lessons learned from the Challenger disaster continue to inform NASA’s approach to space exploration today.

To sum it up:

Bill Nelson, NASA’s Administrator, says: “While it has been nearly 37 years since seven daring and brave explorers lost their lives aboard Challenger, this tragedy will forever be seared in our country’s collective memory. For millions around the globe, myself included, Jan. 28, 1986, still feels like yesterday,” Moreover, he says: “This discovery allows us to pause once again, to uplift the legacies of the seven pioneers we lost, and to reflect on how this tragedy changed us. At NASA, the core value of safety is – and must forever remain – our top priority, especially as our missions explore more of the cosmos than ever before.”

 

Published by: Sky Headlines

The James Webb Space Telescope has made one of its first images of WR 124, a Wolf-Rayet star 15,000 light-years away in the constellation Sagittarius. The star is one of the brightest, most massive, and briefly observable stars known.

Now come to the point that,

Webb’s instruments reveal the detailed structure of WR 124’s nebula!

The Mid-Infrared Instrument (MIRI) on Webb reveals that Wolf-Rayet stars are effective dust emitters. In longer mid-infrared wavelengths, cooler cosmic dust illuminates, revealing the structure of WR 124’s nebula. Webb’s Near-Infrared Camera (NIRCam) balances the brightness of the star core of WR 124 with the intricate details in the fainter gas surrounding it.

Here is a term to know,

What is WR 124?

The material-ejected ring nebula M1-67  surrounds WR 124 a Wolf–Rayet star in the constellation Sagitta. At a radial velocity of around 200 kilometers per second, it is one of the fastest runaway stars in the Milky Way. Paul W discovered it in 1938. Merrill and classified as a Wolf–Rayet star with a high velocity. WR 124 is 30 times the Sun’s mass and has already shed 10 Suns’ worth of material. As the blasted gas recedes from the star and cools, cosmic dust develops and emits infrared light that Webb can detect.

So, here arises the question,

What is the importance of observing the rare Wolf-Rayet phase?

Before going supernova, massive stars go through a short Wolf-Rayet phase. Webb’s detailed observations of this rare phase are helpful to astronomers because they show how this phase works. Wolf-Rayet stars are now shedding their outer layers, resulting in their characteristic gas and dust halos.

But,

How does WR 124 help in understanding the early history of the universe?

Astronomers use stars like WR 124 as analogs to comprehend better a crucial period in the universe’s early history. These dying stars initially seeded the newborn cosmos with heavy elements formed in their cores, elements that are now widespread across the universe, including on Earth.

Furthermore,

Contribution to the universe’s “dust budget”!

Astronomers are interested in the genesis of cosmic dust that can survive a supernova explosion and contribute to the universe’s overall “dust budget” for a variety of reasons. Dust plays an essential function in the universe as it provides shelter for budding stars, aids in the formation of planets, and provides a platform for molecules, including the building blocks of life on Earth, to form and clump together. Despite dust’s crucial roles, there is more dust in the universe than can be explained by astronomers’ existing dust-formation hypotheses. The universe has an excess of dust in its budget.

We will be looking forward for,

Future possibilities for studying cosmic dust!

Before Webb, dust-loving astronomers required more specific data to investigate concerns of dust creation in environments such as WR 124 and whether the dust grains were large enough to survive the supernova and become a significant contributor to the total dust budget. Webb offers new opportunities for researching cosmic dust. It is best viewed at infrared light wavelengths.

Revealed Wolf Rayet star nebula
Credits: NASA, ESA, CSA, STScI, Webb ERO Production Team

Lastly,

Summary:

NASA’s James Webb Space Telescope has looked at WR 124, a Wolf-Rayet star that is 15,000 light-years away and is in the constellation Sagittarius. Webb’s instruments have given us a clear picture of how the star’s nebula is put together. This shows that Wolf-Rayet stars are good at making dust. Before going supernova, WR 124 goes through a short phase called Wolf-Rayet, which is interesting for astronomers to study. Astronomers can also use stars like WR 124 to learn about a critical time in the universe’s early history. Cosmic dust is essential to the universe, and Webb gives us new ways to study it. Infrared wavelengths of light show the best cosmic dust, which Webb can also see.

 

Published by: Sky Headlines

Space experts are warning that an asteroid named 2023 DW, could collide with Earth on Valentine’s Day in 2046. The 50-meter-wide asteroid was discovered by the European Space Agency on February 26, 2023. It is expected to take over two decades to reach Earth, possibly even three.

The asteroid has been added to the “risk list,” which documents objects in space that could potentially impact Earth. According to NASA’s Center for Near Earth Objects, the asteroid poses no unusual level of danger. And the chance of collision is currently extremely unlikely. However, 2023 DW is the only object on the list with a ranking higher than zero on the Torino Scale, which rates space objects’ risk of colliding with Earth.

Valentine's Day 2046
Captured by Nasa’s Lucy spacecraft. Photograph: NASA/Goddard/ZUMA Press Wire Service/REX/Shutterstock

However, we need to know,

What do scientists say about this event?

Italian astronomer Piero Sicoli has predicted a 1 in 400 chance of 2023 DW hitting Earth and has even developed a map indicating where the asteroid could potentially strike. Despite this, the planetary defense coordination office at NASA states that the risk of collision with Earth is currently very small.

Davide Farnocchia is a navigation engineer at the JPL in Pasadena, California. He says: “This object is not particularly concerning,”

If the asteroid collided with Earth, it could cause catastrophic damage. With a diameter of 50 meters, the impact could be equivalent to a nuclear explosion. It resulted in widespread destruction and loss of life.

While the risk of collision is currently very low, scientists are constantly monitoring the asteroid’s trajectory and making updates to their predictions as new data becomes available.  Technology cannot rule out the possibility of a collision with Earth completely.

NASA said on its official Asteroid Watch account on Twitter: “We’ve been tracking a new asteroid named 2023 DW. It has a very small chance of impacting Earth in 2046″.  Moreover, NASA added: “Often when new objects are first discovered, it takes several weeks of data to reduce the uncertainties and adequately predict their orbits years into the future.”

If you are wondering,

Is this the first time an asteroid is going to collide with Earth?

It’s important to note that the Solar System is indeed filled with millions of asteroids. Many of them come close to Earth regularly. Astronomers have been tracking near-Earth objects for decades, and are discovering new ones all the time.

Earlier this year, in January, astronomers observed one of the closest approaches by a known near-Earth object ever recorded. This object, called 2023 BU, was only the size of a box truck, but it came very close to Earth – closer than the distance between the Earth and the Moon. Astronomers only discovered it a week before its closest approach, highlighting the need for continued vigilance in tracking these objects.

In short, the specific asteroid 2023 DW that astronomers have predicted to impact Earth on Valentine’s Day 2046 is getting a lot of attention. It’s certainly not the first time an asteroid has come close to our planet.  Hence, it likely won’t be the last. Scientists and astronomers are constantly monitoring the skies for potential threats and working on developing technologies to mitigate the risk of an impact.

Hence, the question arises:

What are the efforts of scientists to Deflect Hazardous Asteroids?

In the meantime, researchers and space agencies are working on developing methods to deflect potentially hazardous asteroids away from Earth’s orbit. The consequences of a collision with an asteroid could be catastrophic, and we must continue to invest in this technology to protect our planet from future threats.

As Valentine’s Day 2046 approaches, the world will be watching closely as scientists track the trajectory of asteroid 2023 DW. The risk of collision is currently low. So, we must remain vigilant and prepared for any potential threats to our planet.

Here is a point to clear;

What is the role of DART’s mission?

While an asteroid’s impact may seem unlikely, scientists and professionals are creating tools and techniques to reduce the risk. The DART mission’s success implies we can prepare for near-Earth objects like asteroids with proper planning and preparation.

The Planetary Defense Coordination Office will decide if and when to take action if 2023 DW, the asteroid projected to crash Earth on Valentine’s Day 2046. The recently tested Double Asteroid Redirection Test (DART) impactor could be used to change an asteroid’s trajectory.

NASA’s DART mission successfully collided a spacecraft into an asteroid to adjust its trajectory, showing that scientists and professionals can prepare for potentially dangerous space rocks. Scientists have prepared for years to encounter an asteroid.

NASA announced DART’s success in October 2021. The DART mission changed its direction by crashing a spacecraft into a tiny asteroid, showing that such technologies may divert a dangerous asteroid.

Mr. Farnocchia said: “That’s the very reason why we flew that mission,”.He says, “and that mission was a spectacular success.”

So now let’s wrap this up:

Summary:

NASA experts are warning of a potential hazard to Earth in 2046. As a 50-meter-wide asteroid named 2023, DW might collide with the planet on Valentine’s Day. While scientists are now considering the chance of collision extremely low. As astronomers have added asteroid to the “risk list” of objects in space that has the potential to impact Earth. This is the only object on the list with a Torino Scale ranking over zero. The effects of a collision with an asteroid could be devastating. Researchers and space agencies are working on creating means to deflect potentially harmful asteroids away from Earth’s orbit. Experts are now counting on NASA’s asteroid-punishing DART probe to deflect the asteroid.

 

Published by: Sky Headlines

The Moon has always been a source of fascination for humanity, inspiring myths and legends across different cultures. Howeverour understanding of the Moon has grown in the last century in the last century thanks to space agencies’ efforts worldwide. India has also stepped forward to uncover the mysteries and disclose the myths about the moon. The Indian Space Research Organization (ISRO) launched a series of missions called Chandrayaan to the Moon to learn more about its composition, structure, and history. Chandrayaan-1 launched in 2008 and discovered water on the Moon. ISRO launched Chandrayaan-2, a moon landing project, in 2019. Despite the lander’s crash, the orbiter continues to collect data. ISRO has prepared its next attempt Chandrayaan-3 to land a spacecraft on the moon for flight. ISRO will launch the spacecraft in June 2023.

All these projects highlight India’s expanding capacity for space research and its dedication to expanding humanity’s knowledge of space and expanding humanity’s place in it.

Now, we will discuss the Chandrayaan missions launched from India, which have significantly advanced our understanding of the nearest celestial neighbors.

Let’s start with,

Chandrayaan-1: The First Indian Lunar Space Probe

On October 22, 2008, India’s national space agency, the Indian Space Research Organization (ISRO), officially started its Chandrayaan Missions with Chandrayaan-1, India’s first lunar space probe. The scientists designed the mission to conduct remote sensing studies of the Moon from lunar orbit. It collected data on the lunar surface’s mineralogy and elemental composition. Built at only Rs. 386 crores ($76 million), within three years, it was a low-cost spacecraft. Chandrayaan-1 carried a suite of scientific instruments from India, the United States, and the European Space Agency (ESA), making it a truly international effort.

Chandrayaan Missions: Chandrayaan 1
Image Credit: ISRO

Now, you may need to know,

What were the mission objectives and instrumentation?

Chandrayaan-1 had several objectives, including mapping the Moon in infrared, visible, and X-ray light and prospecting for various elements, minerals, and ice. Some of the particular instruments on board the spacecraft included:

  • To create a three-dimensional atlas of the lunar surface, which would help study the distribution of elements and minerals.
  • Determining the extent and depth of water-ice deposits on the lunar surface is essential for future human settlements.
  • Studying the moon’s mineral composition and geology would help us understand its formation and evolution.
  • To study the moon’s atmosphere, particularly the presence of helium-3, a rare isotope that could be used as a fuel in nuclear fusion.
  • To test new technologies for future space missions. Such as a new imaging spectrometer and a miniaturized synthetic aperture radar.

On the whole,

Is Chandrayaan-1 a success or failure?

The mission started on Oct. 22, 2008, and ended on Aug. 28, 2009. The scientists planned to leave the spacecraft in space for about two years.  But, sadly couldn’t keep exploring due to technical issues. During its operational lifetime of approximately ten months, Chandrayaan-1 made several significant discoveries, including detecting water on the Moon’s surface and mapping various elements and minerals on the lunar surface. However, the mission ended abruptly in 2009 when radio contact was lost with the spacecraft.

ISRO says that this spacecraft has almost all its objectives accomplished by then. So instead of any emergency crash, it is better to dismantle it. Chandrayaan-1 did not crash. But the Indian Space Research Organization (ISRO)  intentionally ended its mission. The spacecraft was in a polar orbit around the Moon. It had completed more than 3,400 orbits and collected a wealth of scientific data. However, communication with the spacecraft was lost and attempts to re-establish contact failed. Intovoid any potential damage or interference with future lunar missions, ISRO intentionally crashed the spacecraft into the lunar surface. The exact location of the impact is unknown. But scientists believe that it is in the Moon’s south pole region.

Later on, ISRO succeeded in building up another spacecraft,

Chandrayaan-2: India’s Ambitious Lunar Lander Mission

One of the Chandrayaan Missions, Chandrayaan-2, also known as 44441, was a landmark Indian lunar mission launched by the Indian Space Research Organization (ISRO) on July 22, 2019. The Geosynchronous Satellite Launch Vehicle Mark III (GSLV-MkIII) carried out the mission. It aimed to explore the uncharted lunar south pole region. With a total mass of 3850 kg and a nominal power of 1000 W, the Chandrayaan-2 mission lasted almost a month, from its launch date until its unfortunate end on August 20, 2019. The mission was a significant milestone in India’s space exploration program and had several key objectives, including mapping the lunar surface, studying the composition of the Moon’s atmosphere, and searching for evidence of water on the lunar surface.

Chandrayaan Missions: Chandrayaan 2
Image Credit: ISRO

Let’s take a closer look on,

What were the mission objectives and instrumentation?

Chandrayaan-2 had several objectives, including conducting high-resolution remote sensing of the lunar surface, studying the Moon’s water ice deposits, and characterizing the Moon’s tenuous atmosphere. Some of the special instruments on board the spacecraft included:

  • The mission aimed to study the lunar surface’s topography, mineralogy, and geology to understand its origin and evolution.
  • Chandrayaan-2 aimed to detect and map the distribution of water ice on the Moon’s surface, which could be a potential resource for future space exploration.
  • The mission aimed to study the Moon’s tenuous atmosphere and understand its composition and dynamics.
  • Chandrayaan-2 also aimed to demonstrate India’s capabilities in soft landing on the lunar surface and rover mobility on the Moon.

Are you wondering,

How did Chandrayaan-2 fail?

The Chandrayaan-2 mission, unfortunately, met an untimely end when communication was lost during the lander descent at an altitude of about 2.1 km. Despite crashing on the lunar surface at 70.881 S, 22.784 E, the lander appeared to remain in one piece. But all communications and operations were impossible. The rover, which was supposed to be deployed shortly after landing, needed help to complete its mission. 

Although the lander and rover portions of the mission were planned for only 14-15 days, the orbiter continues to operate and gather valuable data about the Moon. Despite the challenges faced during the mission, Chandrayaan-2 was a significant achievement for India’s space exploration program. It contributed to our understanding of the Moon’s composition and the potential for future human exploration. The lessons learned from this mission will undoubtedly inform future lunar missions and continue to advance the field of planetary science.

Last but not least, 

Chandrayaan-3: India’s Next Lunar Mission:

After the success of Chandrayaan-1 and the ambitious Chandrayaan-2 mission failure, India’s space agency, the Indian Space Research Organization (ISRO), is not stopping its Chandrayaan Missions. Chandrayaan-3, also known as Chandrayaan3, is the upcoming lunar mission of the Indian Space Research Organization (ISRO). Scientists have designed it to pick up where the Chandrayaan-2 mission left off. The primary objective of this mission is to further explore and study the Moon’s surface, with a specific focus on the south polar region. 

The mission will be launched using the Geosynchronous Satellite Launch Vehicle Mark III (GSLV-MkIII) from the Satish Dhawan Space Centre in Sriharikota, India. With a mass of 1752 kg and a nominal power of 738 W, Chandrayaan-3 is expected to be launched in June 2023. The scientists originally planned to launch the mission in 2020. But has been delayed due to technical issues and the COVID-19 pandemic. Here’s what we know so far about Chandrayaan-3.

Chandrayaan Missions: Chandrayaan 3
Image Credit: ISRO

Now let us take a closer look on,

What is the mission design?

Chandrayaan 3 is a lunar mission scheduled to launch in 2023 from Sriharikota, India, using a GSLV Mark 3 heavy-lift launch vehicle. After entering an elliptic parking orbit, the propulsion module will bring the lander/rover into a 100 km circular polar lunar orbit. Then it will separate from it. The lander will then touch down with the rover in the Moon’s south polar region, near 69.37 S, 32.35 E. 

The touchdown velocity will be less than 2 m/s vertical and 0.5 m/s horizontal to ensure a safe landing. The propulsion module/communications relay satellite will remain in lunar orbit to enable communications with Earth, with Chandrayaan 2 serving as a backup relay. The lander and rover are designed to operate for one lunar daylight period, which is about 14 Earth days. This mission will enable further exploration of the lunar surface and allow for studying the Moon’s geology and resources.

Moreover, 

What scientific instruments are onboard Chandrayaan 3?

Chandrayaan-3, the third lunar mission by the Indian Space Research Organization (ISRO), will consist of a propulsion module, a lander, and a rover. The propulsion module generates 758 W power and carries the lander and rover to the moon. The lander has various sensors to ensure a safe touchdown, and the rover is equipped with navigation cameras and a solar panel that generates 50 W power. 

The lander will carry four scientific instruments: Chandra’s Surface Thermophysical Experiment (ChaSTE), the Instrument for Lunar Seismic Activity (ILSA), the Radio Anatomy of Moon Bound Hypersensitive ionosphere and Atmosphere (RAMBHA), and a passive laser retroreflector array provided by NASA. The rover will carry two instruments to study the local surface elemental composition. These include an Alpha Particle X-ray Spectrometer (APXS) and Laser Induced Breakdown Spectroscope (LIBS).

The propulsion module/orbiter will carry the Spectropolarimetry of the Habitable Planet Earth (SHAPE) experiment to study Earth from lunar orbit. It will launch in June 2023, using the GSLV-MkIII launch vehicle from Sriharikota, India.

Lastly,

What are the objectives of Chandrayaan-3?

The objectives of this Chandrayaan Mission are similar to that of its predecessor, Chandrayaan-2. The mission aims to conduct a soft landing on the lunar surface and deploy a rover to explore the surface in greater detail. The primary scientific goals of the mission are:

  • To study the composition of the lunar surface: Chandrayaan-3 will carry scientific instruments to study the lunar surface’s mineralogy, elemental composition, and water content. This data will help scientists understand the Moon’s formation and evolution better.
  • To study the lunar environment: The mission will also study the lunar environment. It includes the Moon’s tenuous atmosphere, magnetic field, and radiation environment. This data will help scientists understand the challenges faced by future human missions to the Moon.
  • To explore the South Pole-Aitken Basin: The landing site for Chandrayaan-3 is expected to be near the Moon’s South Pole-Aitken Basin. This basin is particularly interesting to scientists because it is the largest and oldest impact basin on the Moon. Studying the basin’s composition and structure could shed light on the early history of the Moon and the solar system.

What are India’s expectations with Chandrayaan Missions?

India is not anywhere close to stopping the progress of uncovering the mysteries of the moon. Regardless of the Chandrayaan-2 failure, India heads up to discover more of the moon’s surface and neighboring celestial stars. India is now looking at its masterpiece with fixed eyes to accomplish the objectives of Chandrayaan-2.

Published by: Sky Headlines

The universe is vast and complex, and our ability to grasp it is limited by the instruments we have at our disposal. That’s where remarkable space-based observatories like the Spitzer Space Telescope come in – with its advanced infrared capabilities. This telescope allowed us to see the universe in a whole new light. That unlocks secrets that were previously hidden from us. In this blog, we will travel through time to learn about the Spitzer Space Telescope, its accomplishments, and the fantastic discoveries it has aided in.

But firstly we should know that,

What is the Spitzer Space Telescope?

This spacecraft was launched on August 25, 2003, at 5:35 AM. It aimed to study the cosmos in a completely different light. Orbiting at a height of 568 km and moving at a speed of 0.4741 km/s, Spitzer was a revolutionary piece of technology that gave us a new perspective on space. At $720 million, this project marked a significant investment for space travel in the future.

NASA launched the Spitzer Space Telescope as part of the Great Observatories Program, which included other space-based observatories like the Hubble Space Telescope, Compton Gamma-Ray Observatory, and the Chandra X-Ray Observatory. While those telescopes focused on visible light, gamma rays, and X-rays, respectively. The Spitzer was designed to detect infrared radiation, which is primarily heat radiation. This allowed it to observe objects in the universe that were too cool or obscured by dust to be seen with optical telescopes.

Spitzer Space Telescope
Credits: NASA/JPL-Caltech

Moreover,

What was the use of the Spitzer Space Telescope?

The Spitzer Space Telescope was an essential tool when studying the cosmos in infrared light. Its primary function was to detect infrared radiation, mainly heat. Spitzer’s sensitive detectors have helped astronomers learn more about distant and hidden regions of the cosmos. Such as dusty stellar nurseries, the centers of galaxies, and newly forming planetary systems.

Using Spitzer’s infrared vision, astronomers have studied inaccessible phenomena. Such as failed stars (brown dwarfs), extrasolar planets, gigantic molecular clouds, and organic chemicals that could be the key to life on other worlds. As a whole, the Spitzer Space Telescope is crucial in solving cosmic puzzles.

Here is the important thing to note;

Is the Spitzer telescope still in space?

Yes, the Spitzer telescope is still in space but no longer operational. The Spitzer telescope lasted in the cold phase for about 16 years. The Spitzer Space Telescope, which NASA launched in 2003, was the most sensitive infrared space telescope ever built at the time of its launch. During its 16 years of existence, it fundamentally altered our understanding of the cosmos.

The associate administrator of NASA’s Science Mission Directorate in Washington is “Thomas Zurbuchen”. He says: “Spitzer has taught us about entirely new aspects of the cosmos and taken us many steps further in understanding how the universe works. It addresses questions about our origins and whether or not are we alone”.  Moreover, he said: “This Great Observatory has also identified some important and new questions and tantalizing objects for further study, mapping a path for future investigations to follow. Its immense impact on science certainly will last well beyond the end of its mission.”

However,

What makes the Spitzer Space Telescope unique?

The Spitzer Space Telescope was unique for various reasons. One of the most remarkable features of Spitzer was its ability to detect infrared radiation. It allowed it to study cosmic regions hidden from optical telescopes. The Spitzer telescope also had a large mirror that measured 33 inches (85 cm) in diameter, which made it the largest infrared telescope ever launched into space.

Furthermore, Spitzer was the final mission in NASA’s Great Observatories Program – a family of four space-based observatories, each observing the Universe in a different kind of light. The program also includes the visible-light Hubble Space Telescope (HST), Compton Gamma-Ray Observatory (CGRO), and Chandra X-Ray Observatory (CXO). Spitzer was also unique because of its cryogenic telescope assembly, which contained the telescope and Spitzer’s three scientific instruments.

Here is to understand,

What can the Spitzer telescope see that others Cannot?

The Spitzer Space Telescope was capable of seeing cosmic regions that are hidden from optical telescopes. It could detect infrared radiation, which allowed it to study cooler objects in space, such as failed stars (brown dwarfs), extrasolar planets, giant molecular clouds, and organic molecules that may hold the secret to life on other planets. Spitzer also studied the centers of galaxies and newly forming planetary systems, which are difficult to observe with optical telescopes.

Spitzer’s ability to see the Universe in a different kind of light than optical telescopes allows astronomers to study the Universe in previously impossible ways. Overall, Spitzer’s unique capabilities made it an essential tool for understanding the Universe.

What are the Discoveries of the Spitzer space telescope?

The spitzer space telescope has helped in knowing the universe better than ever. Some of its major discoveries are:

  • Spitzer detects heat radiation and infrared light. Scientists used Spitzer data to create the first exoplanet “weather map” in May 2009. This exoplanet weather map showed temperature changes on HD 189733b, a massive gas planet. The scientists also found roaring winds in the planet’s atmosphere.
  • Infrared light usually penetrates gas and dust clouds better than visible light. Hence, Spitzer has shown star-birthing zones. Spitzer captured young stars emerging from the Rho Ophiuchi dark cloud. Astronomers call this cloud “Rho Oph.” The nebula is 410 light-years from Earth, near Scorpius and Ophiuchus.
  • Spitzer found COSMOS-AzTEC3 in 2011. This set of galaxies’ light reached Earth after 12 billion years. Scientists believe proto-clusters like this one evolved into modern galaxy clusters. COSMOS-AzTEC3 was the furthest proto-cluster ever found. It helps researchers understand how galaxies started and evolved.
  • Spitzer was the first telescope capable of directly identifying chemicals in the atmospheres of exoplanets back in 2007. Chemical compounds in two gas exoplanets were identified using spectroscopy. These gas-based “hot Jupiters,” HD 209458b and HD 189733b, orbit closer to their suns than our solar system’s gas planets. Directly studying exoplanet atmospheres could lead to the discovery of life on rocky worlds. This artist’s rendering depicts a heated Jupiter.
  • Supermassive black holes reside in most galaxies. Spitzer found two of the most distant supermassive black holes, revealing galaxy formation history. Quasars are black holes with discs. Spitzer found two quasars that emerged less than 1 billion years after the cosmos. Their light took 13 billion years to reach Earth.

 

Let’s conclude this discussion:

Scientists initially designed the Spitzer Space Telescope for a short mission. But it exceeded expectations and continued to operate for over a decade. In January 2020, NASA announced that it was retiring the Spitzer Space Telescope due to its aging hardware and limited remaining capabilities. However, the Spitzer Space Telescope legacy will live on through countless discoveries. As it helped make the new avenues of research it opened up. The Spitzer mission will live on through its science.

 

Published by: Sky Headlines

A massive simulated survey has been developed by scientists, which provides insight into what can be anticipated from the future observations of the Nancy Grace Roman Space Telescope. Even though this virtual version is only a bit of the actual survey that will take place, it comprises an enormous number of 33 million galaxies and 200,000 foreground stars in our galaxy.

So to clarify the point,

How utilizing the simulation can help the scientists?

By utilizing the simulation, scientists can strategize the most effective observing techniques, experiment with various methods to extract useful information from the vast amount of data gathered by the mission, and investigate the potential benefits of conducting simultaneous observations with other telescopes.

An assistant professor of physics at Duke University in Durham, North Carolina “Michael Troxel” says: “The volume of data Roman will return is unprecedented for a space telescope”. Moreover, he said: “Our simulation is a testing ground we can use to make sure we will get the most out of the mission’s observations.”

Here is to know;

What role do the Rubin and Roman simulations employ?

The researchers used a mock universe, initially created to aid scientific planning for the Vera C. Rubin Observatory located in Chile, which will commence entire operations in 2024. The Rubin and Roman simulations employ the same source. So, astronomers can make a comparison between them to determine what they can gain by combining the telescopes’ observations. Once they are both actively surveying the cosmos. Troxel has led the paper detailing the findings. And scientists have approved it for publication in The Monthly Notices of the Royal Astronomical Society.

Simulated Survey of Grace Telescope Insights from NASA
Credits: NASA’s Goddard Space Flight Center and M. Troxel

Term to know,

What is Cosmic Construction?

The High Latitude Wide Area Survey of the Roman Space Telescope will include imaging and spectroscopy, with the former being the primary subject of the latest simulation. Spectroscopy gauges the intensity of light emitted by celestial objects at varying wavelengths. In contrast, Roman’s imaging will expose the exact locations and forms of countless faint galaxies utilized for charting dark matter. Although invisible, astronomers can deduce its existence by observing its influence on ordinary matter. Scientists will employ both techniques over an immense stretch of the universe.

The presence of mass bends the structure of space-time, with larger masses producing a more significant impact.  Scientists called this phenomenon as gravitational lensing. Whereby light emanating from a remote source is distorted when it passes through intervening objects. When the things causing the lensing are massive or clusters of galaxies, it can alter or appear as background sources as multiple images.

Simulated Survey of Grace Telescope
Credits: Caltech-IPAC/R. Hurt

Let’s come to the point,

What is weak lensing?

Objects with less mass can generate more subtle effects, known as weak lensing. The Roman Space Telescope will be capable of using weak lensing to detect how dark matter clusters affect the appearance of remote galaxies. By observing these lensing effects, researchers can expand our understanding of dark matter by filling in the gaps in our knowledge.

A physics professor at Ohio State University in Columbus and a co-author of the paper is “Chris Hirata”. He says: “Theories of cosmic structure formation make predictions for how the seed fluctuations in the early universe grow into the distribution of matter that can be seen through gravitational lensing”. Moreover, he says: “But the predictions are statistical in nature. So we test them by observing vast regions of the cosmos. Scientists will optimize Roman, with its wide field of view,  to efficiently survey the sky. It will complement observatories such as the James Webb Space Telescope that are designed for deeper investigation of individual objects.”

Ground and Space

The simulated survey of the Roman Space Telescope encompasses an expanse of 20 square degrees in the sky, which is roughly equivalent to the size of 95 full moons. When the scientists conduct the actual survey, it will be a hundred times larger, revealing over a billion galaxies. Meanwhile, the Vera C. Rubin Observatory will survey an even broader section, spanning 18,000 square degrees, almost half of the entire sky. However, it will possess lower resolution as it must penetrate Earth’s turbulent atmosphere.

Pairing the Roman and Rubin simulations presents an opportunity for researchers to attempt the detection of identical objects in both sets of images, a previously unattainable feat. This is significant because ground-based observations frequently lack the resolution to distinguish multiple closely situated sources as distinct entities. At times, they may merge, adversely affecting weak lensing measurements. Scientists can now determine the difficulties and advantages of “deblending” such objects by comparing Rubin’s images with Roman images.

 

 

Here arises the question,

How will Roman’s extensive perspective of the cosmos enable astronomers?

Roman’s extensive perspective of the cosmos will enable astronomers to achieve much more than the survey’s original objectives. Such as studying the evolution and structure of the universe, charting dark matter, and differentiating between leading theories that seek to explain the accelerating expansion of the universe. With the new synthetic Roman data at their disposal, researchers can preview additional scientific breakthroughs. It will stem from acquiring a highly detailed view of such a vast region of the universe.

The senior project scientist for the Roman mission at NASA’s Goddard Space Flight Center in Greenbelt  Maryland is  “Julie McEnery”. She says: “With Roman’s gigantic field of view, we anticipate many different scientific opportunities. But we will also have to learn to expect the unexpected,”. Moreover, she says: “The mission will help answer critical questions in cosmology while potentially revealing brand new mysteries for us to solve.”

 

Published by: Sky Headlines