Wednesday, January 10, 2024

Beta Pictoris Cat's Tail: Nearby Planetary System Intrigues Astronomers

Beta Pictoris Cat's Tail: Nearby Planetary System Intrigues Astronomers

This is an animation portraying the creation of the cat’s tail, as hypothesized by a team of astronomers. This structure, which is seen in the southwest portion of Beta Pic’s secondary debris disk, is estimated to span 10 billion miles.

Scientists hypothesize that the cat’s tail is the result of a dust production event—like a collision—that occurred a mere one hundred years ago. Initially, the dust created follows the same orbital direction as its source, and then starts to spread out. The star’s light pushes the smallest, fluffiest dust particles away from the star faster, while bigger grains do not move as much, creating a trail of dust.

From an edge-on perspective, the sharp incline of the cat’s tail is an optical illusion. Our perspective along with the curvature of the tail creates the observed angle, while in fact, the tendril of dust is only departing from the disk at a five-degree incline.

Discover even more: https://webbtelescope.pub/3RXt9Nx 


Video Credits:

Animation

NASA, ESA, CSA, STScI, R. Crawford (STScI).

Science

C. Stark (NASA-GSFC), M. Perrin (STScI), I. Rebollido (Astrobiology Center).

Duration: 30 seconds

Release Date: Jan. 10, 2024


#NASA #ESA #Astronomy #Space #Science #Stars #Star #BetaPictoris #PlanetarySystem #Dust #Debris #Pictoris #Constellation #JamesWebb #SpaceTelescope #JWST #Cosmos #Universe #UnfoldTheUniverse #Europe #CSA #Canada #GSFC #STScI #UnitedStates #STEM #Education #Animation #HD #Video

Webb Discovers Dusty Cat’s Tail in Nearby Beta Pictoris Planetary System

Webb Discovers Dusty Cat’s Tail in Nearby Beta Pictoris Planetary System


Beta Pictoris, a young planetary system located just 63 light-years away, continues to intrigue scientists even after decades of in-depth study. It possesses the first dust disc imaged around another star—a disc of debris produced by collisions between asteroids, comets, and planetesimals. Observations from the NASA/European Space Agency Hubble Space Telescope revealed a second debris disc in this system [1], inclined with respect to the first. Now, a team of astronomers using the NASA/European Space Agency/Canadian Space Agency James Webb Space Telescope to image the Beta Pictoris (Beta Pic) system has discovered a new, previously unseen structure.

The Webb telescope uses a coronagraph—an instrument designed to block out the direct light from a star so that surrounding objects which would otherwise be hidden in the star's glare can be observed.

The team, led by Isabel Rebollido of the Astrobiology Center in Spain, and now an European Space Agency Research Fellow, used Webb’s NIRCam (Near-Infrared Camera) and MIRI (Mid-Infrared Instrument) to investigate the composition of Beta Pic’s previously detected main and secondary debris discs. The results exceeded their expectations, revealing a sharply inclined branch of dust, shaped like a cat’s tail, that extends from the southwest portion of the secondary debris disc.

“Beta Pictoris is the debris disc that has it all: It has a really bright, close star that we can study very well,” said Rebollido. “While there have been previous observations from the ground in this wavelength range, they did not have the sensitivity and the spatial resolution that we now have with Webb, so they didn’t detect this feature.”

A Star’s Portrait Improved with Webb

Even with Webb, peering at Beta Pic in the right wavelength range—in this case, the mid-infrared—was crucial to detect the cat’s tail, as it only appeared in the MIRI data. Webb’s mid-infrared data also revealed differences in temperature between Beta Pic’s two discs, which likely is due to differences in composition.

“We didn’t expect Webb to reveal that there are two different types of material around Beta Pic, but MIRI clearly showed us that the material of the secondary disc and cat’s tail is hotter than the main disc,” said Christopher Stark, a co-author of the study at NASA’s Goddard Space Flight Center in Greenbelt, Maryland. “The dust that forms that disc and tail must be very dark, so we don’t easily see it at visible or near-infrared wavelengths—but in the mid-infrared, it’s glowing.”

To explain the hotter temperature, the team deduced that the dust may be highly porous “organic refractory material,” similar to the matter found on the surfaces of comets and asteroids in our solar system. For example, a preliminary analysis of material sampled from asteroid Bennu by NASA’s OSIRIS-Rex mission found it to be very dark and carbon-rich, much like what MIRI detected at Beta Pic.

The Tail’s Puzzling Beginning Warrants Future Research

However, a major lingering question remains: What could explain the shape of the cat’s tail, a uniquely curved feature unlike what is seen in discs around other stars?

Rebollido and the team modelled various scenarios in an attempt to emulate the cat’s tail and unravel its origins. Though further research and testing is required, the team presents a strong hypothesis that the cat’s tail is the result of a dust production event that occurred a mere one hundred years ago.

“Something happens—like a collision—and a lot of dust is produced,” shared Marshall Perrin, a co-author of the study at the Space Telescope Science Institute in Baltimore, Maryland. “At first, the dust goes in the same orbital direction as its source, but then it also starts to spread out. The light from the star pushes the smallest, fluffiest dust particles away from the star faster, while the bigger grains do not move as much, creating a long tendril of dust.”

“The cat’s tail feature is highly unusual, and reproducing the curvature with a dynamical model was difficult,” explained Stark. “Our model requires dust that can be pushed out of the system extremely rapidly, which again suggests it’s made of organic refractory material.”

The team’s preferred model explains the sharp angle of the tail away from the disc as a simple optical illusion. Our perspective combined with the curved shape of the tail creates the observed angle of the tail, while in fact, the arc of material is only departing from the disc at a five-degree incline. Taking into consideration the tail’s brightness, the team estimates the amount of dust within the cat’s tail to be equivalent to a large main belt asteroid spread out across 16 billion kilometers.

A recent dust production event within Beta Pic’s debris discs could also explain an asymmetry previously spotted by the Atacama Large Millimeter/submillimeter Array in 2014: a clump of carbon monoxide (CO) located near the cat’s tail. Since the star’s radiation should break down CO within roughly one hundred years, this still-present concentration of gas could be lingering evidence of the same event.

“Our research suggests that Beta Pic may be even more active and chaotic than we had previously thought,” said Stark. “Webb continues to surprise us, even when looking at the most well-studied objects. We have a completely new window into these planetary systems.”

These results were presented in a press conference at the 243rd meeting of the American Astronomical Society in New Orleans, Louisiana.

The observations were taken as part of Guaranteed Time Observation program 1411.

Webb is the largest, most powerful telescope ever launched into space. Under an international collaboration agreement, ESA provided the telescope’s launch service, using the Ariane 5 launch vehicle. Working with partners, ESA was responsible for the development and qualification of Ariane 5 adaptations for the Webb mission and for the procurement of the launch service by Arianespace. ESA also provided the workhorse spectrograph NIRSpec and 50% of the mid-infrared instrument MIRI, which was designed and built by a consortium of nationally funded European Institutes (The MIRI European Consortium) in partnership with JPL and the University of Arizona.

Webb is an international partnership between NASA, ESA and the Canadian Space Agency (CSA).


Image Credit: NASA, ESA, CSA, STScI, C. Stark and K. Lawson (NASA GSFC), J. Kammerer (ESO), and M. Perrin (STScI).

Release Date: Jan. 10, 2024


#NASA #ESA #Astronomy #Space #Science #Stars #Star #BetaPictoris #PlanetarySystem #Dust #Debris #Pictoris #Constellation #JamesWebb #SpaceTelescope #JWST #Cosmos #Universe #UnfoldTheUniverse #Europe #CSA #Canada #GSFC #STScI #UnitedStates #STEM #Education

Supernovae Give Rise to Black Holes or Neutron Stars | ESO

Supernovae Give Rise to Black Holes or Neutron Stars | ESO


ESOcast 269 Light: Astronomers have found a direct link between the explosive deaths of massive stars and the formation of the most compact and enigmatic objects in the Universe—black holes and neutron stars. This video summarizes the discovery. With the help of the European Southern Observatory’s Very Large Telescope (ESO’s VLT) and ESO’s New Technology Telescope (NTT), two teams were able to observe the aftermath of a supernova explosion in a nearby galaxy, finding evidence for the mysterious compact object it left behind.

When massive stars reach the end of their lives, they collapse under their own gravity so rapidly that a violent explosion known as a supernova ensues. Astronomers believe that, after all the excitement of the explosion, what is left is the ultra-dense core, or compact remnant, of the star. Depending on how massive the star is, the compact remnant will be either a neutron star—an object so dense that a teaspoon of its material would weigh around a trillion kilograms here on Earth—or a black hole—an object that nothing, not even light, can escape from.   

Astronomers have found many clues hinting at this chain of events in the past, such as finding a neutron star within the Crab Nebula, the gas cloud left behind when a star exploded nearly a thousand years ago. However, they had never before seen this process happen in real time, meaning that direct evidence of a supernova leaving behind a compact remnant has remained elusive. “In our work, we establish such a direct link,” says Ping Chen, a researcher at the Weizmann Institute of Science, Israel, and lead author of a study published today in Nature and presented at the 243rd American Astronomical Society meeting in New Orleans, USA.

The researchers’ lucky break came in May 2022, when South African amateur astronomer Berto Monard discovered the supernova SN 2022jli in the spiral arm of the nearby galaxy NGC 157, located 75 million light-years away. Two separate teams turned their attention to the aftermath of this explosion and found it to have a unique behavior.

After the explosion, the brightness of most supernovae simply fades away with time; astronomers see a smooth, gradual decline in the explosion’s ‘light curve’. But SN 2022jli’s behavior is very peculiar: as the overall brightness declines, it doesn’t do so smoothly, but instead oscillates up and down every 12 days or so. “In SN 2022jli’s data we see a repeating sequence of brightening and fading,” says Thomas Moore, a doctoral student at Queen’s University Belfast, Northern Ireland, who led a study of the supernova published late last year in the Astrophysical Journal. “This is the first time that repeated periodic oscillations, over many cycles, have been detected in a supernova light curve,” Moore noted in his paper. 

The Moore and Chen teams believe that the presence of more than one star in the SN 2022jli system could explain this behavior. In fact, it is not unusual for massive stars to be in orbit with a companion star in what is known as a binary system, and the star that caused SN 2022jli was no exception. What is remarkable about this system, however, is that the companion star appears to have survived the violent death of its partner and the two objects, the compact remnant and the companion, likely kept orbiting each other.

The data collected by the Moore team, including observations with ESO’s NTT in Chile’s Atacama Desert, did not allow them to pin down exactly how the interaction between the two objects caused the highs and lows in the light curve. Nevertheless, the Chen team had additional observations. They found the same regular fluctuations in the system’s visible brightness that the Moore team had detected, and they also spotted periodic movements of hydrogen gas and bursts of gamma rays in the system. Their observations were made possible thanks to a fleet of instruments on the ground and in space, including X-shooter on ESO's VLT, also located in Chile.

Putting all the clues together, the two teams generally agree that when the companion star interacted with the material thrown out during the supernova explosion, its hydrogen-rich atmosphere became puffier than usual. Then, as the compact object left behind after the explosion zipped through the companion’s atmosphere on its orbit, it would steal hydrogen gas, forming a hot disc of matter around itself. This periodic stealing of matter, or accretion, released lots of energy that was picked up as regular changes of brightness in the observations.

Even though the teams could not observe light coming from the compact object itself, they concluded that this energetic stealing can only be due to an unseen neutron star, or possibly a black hole, attracting matter from the companion star’s puffy atmosphere. “Our research is like solving a puzzle by gathering all possible evidence,” Chen says. “All these pieces lining up lead to the truth.” 

With the presence of a black hole or neutron star confirmed, there is still plenty to unravel about this enigmatic system, including the exact nature of the compact object or what end could await this binary system. Next-generation telescopes such as ESO’s Extremely Large Telescope, scheduled to begin operation later this decade, will help with this, allowing astronomers to reveal unprecedented details of this unique system.


Credit: European Southern Observatory (ESO)

Directed by: Angelos Tsaousis and Martin Wallner

Editing: Angelos Tsaousis

Written by: Tom Howarth and Pamela Freeman

Footage and photos: ESO / Luis Calçada, Martin Kornmesser, Angelos Tsaousis, Alexandre Santerne, Hubble

Scientific consultant: Paola Amico, Mariya Lyubenova

Duration: 1 minute, 29 seconds

Release Date: Jan. 10, 2024


#NASA #ESO #Astronomy #Space #Science #BlackHoles #Stars #NeutronStars #Galaxy #NGC157 #Supernovae #Supernova #SN2022jli #Constellation #VLT #Cosmos #Universe #Astrophysics #Chile #Europe #STEM #Education #HD #Video

Red Sprites Observed near Coast of Turkey | Earth Science

Red Sprites Observed near Coast of Turkey | Earth Science

Photographer Tsouras Panagiotis: "Shown above are red sprites and the rising Moon as captured from Levadia, Greece on November 4, 2023. These high altitude, mysterious sprites are produced by intense thunderstorm cells. They last but a second or two and are generated at altitudes ranging from about 25-55 mi (40-89 km) above the Earth's surface, typically during the mature and decaying stages of large thunderstorm complexes. Under the most favorable conditions they may be observed every few minutes. Note that the storm responsible for this event was near coast of Turkey, more than 200-miles (322 km) east of my location in central Greece. Though they've been seen by the unaided eye, in most cases they're imaged by sensitive cameras."

Technical Details: Sony A7sii camera; 1/25 seconds exposure time; f1.4; ISO 1200.

Sometimes lightning occurs out near space. One such lightning type is red sprite lightning. It has only been photographed and studied on Earth over the past 25 years. The origins of all types of lightning remain topics for research, and scientists are still trying to figure out why red sprite lightning occurs at all. 

Research has shown that following a powerful positive cloud-to-ground lightning strike, red sprites may start as 100-meter balls of ionized air that shoot down from about 80-km high at 10 percent the speed of light. They are quickly followed by a group of upward streaking ionized balls. 


Red Sprites: These mysterious bursts of light in the upper atmosphere momentarily resemble gigantic jellyfish. One unusual feature of sprites is that they are relatively cold. They operate more like long fluorescent light tubes than hot compact light bulbs. In general, red sprites take only a fraction of a second to occur and are best seen when powerful thunderstorms are visible from the side.


Image & Caption Credit: Tsouras Panagiotis  

Caption Acknowledgement: National Aeronautics and Space Administration (NASA)

Location: Levadia, Greece Coordinates: 38.441441, 22.981376

Release Date: Jan. 9, 2024


#NASA #Science #Moon #Planet #Earth #Atmosphere #Weather #Meteorology #Storm #Lightning #RedSprites #Levadia #Greece #Turkey #Türkiye #Photography #TsourasPanagiotis #Photographer #CitizenScience #STEM #Education #EPoD

Tuesday, January 09, 2024

Thor's Helmet: Nebula NGC 2359 in Canis Major

Thor's Helmet: Nebula NGC 2359 in Canis Major


Thor not only has his own day (Thursday), but a helmet in the heavens. Popularly called Thor's Helmet, NGC 2359 is a hat-shaped cosmic cloud with wing-like appendages. Heroically sized even for a Norse god, Thor's Helmet is about 30 light-years across. In fact, the cosmic head-covering is more like an interstellar bubble, blown with a fast wind from the bright, massive star near the bubble's center. Known as a Wolf-Rayet star, the central star is an extremely hot giant thought to be in a brief, pre-supernova stage of evolution. NGC 2359 is located about 15,000 light-years away toward the constellation of the Great Overdog. 

This remarkably sharp image is a mixed cocktail of data from narrowband filters, capturing not only natural looking stars but details of the nebula's filamentary structures. The star in the center of Thor's Helmet is expected to explode in a spectacular supernova sometime within the next few thousand years.


Image Credit & Copyright: Ritesh Biswas

Ritesh's website: 

https://www.astrobin.com/users/Astrovert_Tez/

Release Date: Jan. 9, 2024


#NASA #Astronomy #Space #Science #Stars #Nebula #ThorsHelmetNebula #NGC2359 #WolfRayetStar #CanisMajor #Constellation #MilkyWayGalaxy #Cosmos #Universe #Telescope #Astrophotographer #CitizenScience #STEM #Education #APoD

Recientemente: El primer lanzamiento robótico de Artemis a la Luna | NASA

Recientemente: El primer lanzamiento robótico de Artemis a la Luna | NASA

Recientemente en la NASA, la versión en español de las cápsulas This Week at NASA, te informa semanalmente de lo que está sucediendo en la NASA. 

Ciencia de la NASA: https://ciencia.nasa.gov

Para obtener más información sobre la ciencia de la NASA, suscríbete al boletín semanal: https://www.nasa.gov/suscribete


Credit: National Aeronautics and Space Administration (NASA)

Duration: 2 minutes

Release Date: Jan. 9, 2024


#NASA #Space #Astronomy #Science #NASAenespañol #español #ArtemisProgram #Moon #SouthPole #MonsMouton #WaterIce #Astrobotic #PeregrineLunarLander #Robotics #SpaceTechnology #SpaceExploration #Jupiter #Io #SolarSystem #ULA #VulcanRocket #CLPS #UnitedStates #STEM #Education #HD #Video

How NASA’s X-59 Supersonic Aircraft May Change the Future of High-Speed Flight

How NASA’s X-59 Supersonic Aircraft May Change the Future of High-Speed Flight

NASA’s X-59 quiet supersonic research aircraft is the product of decades of aeronautics and supersonic flight research. The X-59 is designed to be able to fly supersonic, or faster than the speed of sound, without producing a loud sonic boom, which occurs when aircraft fly at such speeds. Instead, the X-59 is designed to reduce that boom to a quieter sonic “thump.” 

The X-59 is the centerpiece of NASA’s Quesst mission that seeks to understand the public’s response to quieter supersonic flight and provide data to regulators to consider removing the current ban on commercial supersonic flight over land, opening the future to reduced flight times around the country and the world.

The X-59's goal is to help change existing national and international aviation rules that ban commercial supersonic flight over land.

Learn more here:

https://www.nasa.gov/flightlog

X-59 Free Maker Bundle (STEM Education):

https://www.nasa.gov/sites/default/files/atoms/files/x-59-maker-bundle-v8.pdf

Hablas español? Visita: https://ciencia.nasa.gov/el-x-59-se-asemeja-una-aeronave-real para aprender mas sobre la mision Quesst


Video Credit: National Aeronautics and Space Administration (NASA)

Duration: 2 minutes

Release Date: Jan. 9, 2024


#NASA #Aerospace #SupersonicFlight #SupersonicAircraft #X59 #Sonicboom #QuietAviation #Aviation #QuesstMission #CommercialAviation #Science #Physics #Engineering #AerospaceResearch #AeronauticalResearch #FlightTests #LockheedMartin #NASAArmstrong #AFRC #EdwardsAFB #California #UnitedStates #STEM #Education #HD #Video

Artemis: Onward to the Moon | NASA

Artemis: Onward to the Moon | NASA

With Artemis missions, NASA will land the first woman and first person of color on the Moon, using innovative technologies to explore more of the lunar surface than ever before. We will collaborate with commercial and international partners and establish the first long-term presence on the Moon. Then, we will use what we learn on and around the Moon to take the next giant leap: sending the first astronauts to Mars.

NASA’s Artemis II Crew: 

Commander Reid Wiseman, Pilot Victor Glover, and Mission Specialist Christina Koch from NASA, and Mission Specialist Jeremy Hansen from the Canadian Space Agency.

Artemis II will be NASA’s first crewed flight test of the Space Launch System (SLS) rocket and Orion spacecraft around the Moon to verify today’s capabilities for humans to explore deep space and pave the way for long-term exploration and science on the lunar surface.

Learn more about the Artemis II Mission:

https://www.nasa.gov/artemis-ii


Credit: National Aeronautics and Space Administration (NASA)

Video Producer: Sonnet Apple

Duration: 1 minute, 25 seconds

Release Date: Jan. 9, 2024


#NASA #CSA #Space #Moon #ArtemisProgram #ArtemisII #OrionSpacecraft #DeepSpace #Astronauts #VictorGlover #ChristinaKoch #JeremyHansen #ReidWiseman #MoonToMars #Science #SpaceExploration #HumanSpaceflight #UnitedStates #Canada #ForAllHumanity #STEM #Education #Animation #HD #Video

US-India Partnership: NISAR—Tracking Earth’s Changes from Space | NASA/ISRO

US-India Partnership: NISARTracking Earth’s Changes from Space | NASA/ISRO

NASA and the Indian Space Research Organisation (ISRO) have teamed up to create a powerful new space mission that will track our changing Earth in fine detail. The satellite, called NISAR, will use an advanced radar system to deepen our understanding of deforestation, shrinking glaciers and sea ice loss, natural hazards, climate change, and other global vital signs.

Short for NASA-ISRO Synthetic Aperture Radar, NISAR features two radar instruments: one from ISRO, and one built at NASA’s Jet Propulsion Laboratory (JPL) in Southern California. Peering through cloud cover and vegetation, the satellite will bounce radar signals off nearly all the planet’s land and ice twice every 12 days, monitoring motions of the surface down to fractions of an inch along with changes in other characteristics. 

NISAR is undergoing final integration and testing at ISRO’s satellite facility in Bengaluru, India, and will launch from ISRO’s Satish Dhawan Space Centre in Sriharikota, India. Launch is expected in early 2024; the specific date will be announced by ISRO.

NISAR’s payload will be the most advanced radar system ever launched as part of a NASA science mission, and it will feature the largest-ever radar antenna of its kind: a drum-shaped, wire mesh reflector nearly 40 feet (12 meters) in diameter that will extend from a 30-foot (9-meter) boom.

The mission’s science instruments consist of L- and S-band radar, so named to indicate the wavelengths of their signals. ISRO built the S-band radar, which it shipped to JPL in March 2021. Engineers spent much of the last two years integrating the instrument with the JPL-built L-band system, then conducting tests to verify they work well together.

Once in operation, NISAR will be able to collect measurements day and night, in all weather conditions, and its trove of data will help researchers better understand a broad range of Earth science topics, including landslides, groundwater loss, and the carbon cycle.

More About the Mission

NISAR is the first-ever collaboration between NASA and ISRO on an Earth-observing mission. JPL, which is managed for NASA by Caltech in Pasadena, leads the U.S. component of the project and is providing the mission’s L-band SAR. NASA is also providing the radar reflector antenna, the deployable boom, a high-rate communication subsystem for science data, GPS receivers, a solid-state recorder, and payload data subsystem. ISRO is providing the spacecraft bus, the S-band SAR, the launch vehicle, and associated launch services and satellite mission operations.

To learn more about NISAR, visit: https://nisar.jpl.nasa.gov/


Credit: NASA/JPL-Caltech/ISRO

Duration: 3 minutes

Release Date: Jan. 9, 2024


#NASA #ISRO #Space #Planet #Earth #Science #NISAR #Satellite #Spacecraft #SyntheticApertureRadar #SAR #EarthObservation #Land #Ice #Climate #ClimateChange #GlobalHeating #SpaceTechnology #Engineering #India #BhāratGaṇarājya #JPL #Caltech #UnitedStates #STEM #Education #HD #Video

New Planet Mars Images | NASA Mars Curiosity & Perseverance Rovers

New Planet Mars Images | NASA Mars Curiosity & Perseverance Rovers



Mars 2020 - sol 1021


Mars 2020 - sol 1022


Mars 2020 - sol 1010


MSL - sol 4056


MSL - sol 4054


Mars 2020 - sol 1020


Mars 2020 - sol 1024


MSL - sol 4056


Celebrating 11+ Years on Mars (2012-2023)
Mission Name: Mars Science Laboratory (MSL)
Rover Name: Curiosity
Main Job: To determine if Mars was ever habitable to microbial life. 
Launch: Nov. 6, 2011
Landing Date: Aug. 5, 2012, Gale Crater, Mars

Celebrating 2+ Years on Mars
Mission Name: Mars 2020
Rover Name: Perseverance
Main Job: Seek signs of ancient life and collect samples of rock and regolith (broken rock and soil) for return to Earth.
Mars Helicopter (Ingenuity)
Launch: July 30, 2020    
Landing: Feb. 18, 2021, Jezero Crater, Mars

For more information on NASA's Mars missions, visit: mars.nasa.gov

Image Credits: NASA/JPL-Caltech/ASU/MSSS
Processing: Kevin M. Gill
Image Release Dates: Dec. 30, 2023-Jan. 8, 2024

#NASA #Space #Astronomy #Science #Mars #RedPlanet #Planet #Astrobiology #Geology #CuriosityRover #MSL #MountSharp #GaleCrater #PerseveranceRover #Mars2020 #JezeroCrater #Robotics #SpaceTechnology #SpaceEngineering #JPL #Caltech #UnitedStates #CitizenScience #KevinGill #STEM #Education

Layered Bedrock on Mars | NASA's Mars Reconnaissance Orbiter

Layered Bedrock on Mars | NASA's Mars Reconnaissance Orbiter

Layered sediments are the key to the puzzle of Martian history. They tell us about the conditions that existed when the sediments were deposited, and how they changed over time. This image shows an eroded mesa made up of rhythmically layered bedrock that seems to indicate cyclic deposition. The layers are accentuated by recent dark sand deposits that have accumulated on the benches of the brighter sediments. The plateau is topped by a younger set of layers that appear to be finer and less blocky than the older layers below, suggesting a different depositional environment. Similar layered sediments are found in nearby craters in southwestern Arabia Terra.

The University of Arizona, Tucson, operates the High Resolution Imaging Science Experiment (HiRISE) instrument, that was built by Ball Aerospace & Technologies Corp., Boulder, Colorado. 

NASA's Jet Propulsion Laboratory, a division of Caltech in Pasadena, California, manages the Mars Reconnaissance Orbiter Project for NASA's Science Mission Directorate, Washington.

“For 17 years, MRO has been revealing Mars to us as no one had seen it before,” said the mission’s project scientist, Rich Zurek of JPL.


Video Credit: NASA/JPL-Caltech/University of Arizona

Narration: Tre Gibbs

Duration: 1 minute

Release Date: Nov. 17, 2021


#NASA #Space #Astronomy #Mars #Planet #RedPlanet #Science #Geology #Landscape #Terrain #Geoscience #Bedrock #SedimentLayers #Mesa #MRO #Orbiter #Spacecraft #HiRISE #Camera #JPL #Caltech #UniversityOfArizona #BallAerospace #STEM #Education #HD #Video

United Launch Alliance Vulcan Rocket Flight Test Highlights

United Launch Alliance Vulcan Rocket Flight Test Highlights

"United Launch Alliance (ULA) marked the beginning of a new era of space capabilities with the successful launch of its next generation Vulcan rocket on Jan. 8, 2024, at 2:18 a.m. EST from Space Launch Complex-41 at Cape Canaveral Space Force Station. The Vulcan provides industry-leading capabilities to deliver any payload, at any time, to any orbit."

As part of NASA’s Commercial Lunar Payload Services (CLPS) initiative and Artemis program, a United Launch Alliance (ULA) Vulcan rocket   successfully launched the first U.S. commercial robotic launch for Artemis lunar science missions. Vulcan has supported a NASA science mission via Astrobotic’s Peregrine lunar lander. This was the ULA Vulcan rocket's first certification mission (Cert-1).

Astrobotic’s Peregrine Mission One is designed to carry NASA and commercial payloads for studies of the lunar exosphere, thermal properties, and hydrogen abundance of the lunar regolith, magnetic fields, and the radiation environment of the lunar surface.

Learn more about Astrobotic’s Peregrine Lunar Lander (Adobe PDF):

https://www.astrobotic.com/wp-content/uploads/2023/12/Peregrine-Launch_Info_Packet-Web-1.pdf

Learn about NASA's Commercial Lunar Payload Services (CLPS) - Astrobotic's Peregrine Mission One:

https://www.nasa.gov/commercial-lunar-payload-services/ 


Credit: United Launch Alliance (ULA)

Duration: 2 minutes

Release Date: Jan. 8, 2024


#NASA #Space #Astronomy #Science #ArtemisProgram #Moon #SouthPole #MonsMouton #WaterIce #Astrobotic #PeregrineLunarLander #Robotics #Engineering #SpaceTechnology #DeepSpace #SpaceExploration #SolarSystem #ULA #VulcanRocket #Cert1FlightTest #CLPS #UnitedStates #STEM #Education #HD #Video

Monday, January 08, 2024

Quieting the Boom: Meet NASA's X-59 Supersonic Aircraft | 60 Second Science

Quieting the Boom: Meet NASA's X-59 Supersonic Aircraft | 60 Second Science

What if you could fly from coast to coast in half the time? NASA's Quesst Mission is working to see if that vision can become reality.

Meet the X-59, NASA's quiet supersonic aircraft that will turn sonic booms into sonic "thumps" and could one day cut flight times in half.

The X-59's goal is to expand supersonic flight and provide regulators with data to help change existing national and international aviation rules that ban commercial supersonic flight over land.

Learn more here:

https://www.nasa.gov/flightlog

X-59 Free Maker Bundle (STEM Education):

https://www.nasa.gov/sites/default/files/atoms/files/x-59-maker-bundle-v8.pdf

Hablas español? Visita: https://ciencia.nasa.gov/el-x-59-se-asemeja-una-aeronave-real para aprender mas sobre la mision Quesst


Video Credit: National Aeronautics and Space Administration (NASA)

Duration: 1 minute

Release Date: Jan. 8, 2024


#NASA #Aerospace #SupersonicFlight #SupersonicAircraft #X59 #Sonicboom #QuietAviation #Aviation #QuesstMission #CommercialAviation #Science #Physics #Engineering #AerospaceResearch #AeronauticalResearch #FlightTests #LockheedMartin #NASAArmstrong #AFRC #EdwardsAFB #California #UnitedStates #STEM #Education #HD #Video

ULA Vulcan Rocket Flight Test for NASA Artemis Robotic Moon Missions

ULA Vulcan Rocket Flight Test for NASA Artemis Robotic Moon Missions









As part of NASA’s Commercial Lunar Payload Services (CLPS) initiative and Artemis program, a United Launch Alliance (ULA) Vulcan rocket   successfully launched at 2:18 a.m. EST Monday, Jan. 8, 2024, from Launch Complex 41 at Cape Canaveral Space Force Station in Florida. This is the first U.S. commercial robotic launch for Artemis lunar science missions. Vulcan has supported a NASA science mission via Astrobotic’s Peregrine lunar lander. This was the ULA Vulcan rocket's first certification mission (Cert-1).

Astrobotic’s Peregrine Mission One is designed to carry NASA and commercial payloads for studies of the lunar exosphere, thermal properties, and hydrogen abundance of the lunar regolith, magnetic fields, and the radiation environment of the lunar surface.

Learn more about Astrobotic’s Peregrine Lunar Lander (Adobe PDF):

https://www.astrobotic.com/wp-content/uploads/2023/12/Peregrine-Launch_Info_Packet-Web-1.pdf

Learn about NASA's Commercial Lunar Payload Services (CLPS) - Astrobotic's Peregrine Mission One:

https://www.nasa.gov/commercial-lunar-payload-services/ 


Image Credits: United Launch Alliance (ULA)

Image Date: Jan. 8, 2023


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NASA Telescopes Chase Down "Green Monster" in Cassiopeia A Star's Debris

NASA Telescopes Chase Down "Green Monster" in Cassiopeia A Star's Debris

Cassiopeia A (Cas A) is a supernova remnant located about 11,000 light-years from Earth in the constellation Cassiopeia. It spans approximately 10 light-years. A curious structure there was first identified in Webb’s infrared data from April 2023. The origin of this feature, dubbed the “Green Monster” because of its resemblance to the wall in the left field of Fenway Park, was not clear. However, by combining the Webb data with x-rays from NASA's Chandra X-ray Observatory, researchers think they have hunted down the source of the Green Monster.

While the astronomers already suspected the Green Monster was created by a blast wave from the exploded star slamming into material surrounding it, the Chandra data helped clinch the case. They showed that the properties of the X-rays from the Green Monster are similar to the X-rays from the blast wave rather than from the supernova debris.

When a massive star exploded to create Cas A about 340 years ago, from Earth’s perspective, it created a ball of matter and light that expanded outward. In the outer parts of Cas A the blast wave is striking surrounding gas that was ejected by the star between about 10,000 and 100,000 years before the explosion.

Chandra detects debris from the star because it is heated to tens of millions of degrees by shock waves, akin to sonic booms from a supersonic plane. Webb can see some material that has not been affected by shock waves, what can be called “pristine” debris. Much of this lies behind the Green Monster. This means the combination of Webb and Chandra data gives a fuller census of debris from the exploded star.

Astronomers will continue to use every tool available—including Chandra and Webb—to study this object that has fascinated them for years.


Video Credit: Chandra X-ray Observatory

Duration: 3 minutes

Release Date: Jan. 8, 2024


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Arp 122: A "Herculean" Galactic Merger | Hubble Space Telescope

Arp 122: A "Herculean" Galactic Merger | Hubble Space Telescope

This Hubble image features Arp 122, a peculiar galaxy that is made up of two galaxies—NGC 6040, the tilted, warped spiral galaxy and LEDA 59642, the round, face-on spiral—that are in the middle of a collision in the constellation Hercules. This dramatic cosmic encounter is located at the very safe distance of roughly 570 million light-years from Earth. Peeking in at the corner is the elliptical galaxy NGC 6041, a central member of the galaxy cluster that Arp 122 resides in, but otherwise not participating in this monster merger.

Image Description: Two spiral galaxies are merging together at the right side of the image. One is seen face-on and is circular in shape. The other seems to lie in front of the first one. This galaxy is seen as a disc tilted away from the viewer and it is partially warped. In the lower-left corner, cut off by the frame, a large elliptical galaxy appears as light radiating from a point. Many small galaxies cover the background.

Galactic collisions and mergers are monumentally energetic and dramatic events, but they take place on a very slow timescale. For example, the Milky Way is on track to collide with its nearest galactic neighbor, the Andromeda Galaxy (M31), but these two galaxies have a good four billion years to go before they actually meet. The process of colliding and merging will not be a quick one either. It may  take hundreds of millions of years to unfold. These collisions take so long because of the truly massive distances involved.

Galaxies are composed of stars and their solar systems, dust and gas. In galactic collisions, therefore, these constituent components may experience enormous changes in the gravitational forces acting on them. In time, this completely changes the structure of the two (or more) colliding galaxies, and sometimes ultimately results in a single, merged galaxy. This may well be what results from the collision pictured in this image. Galaxies that result from mergers are thought to have a regular or elliptical structure, as the merging process disrupts more complex structures (such as those observed in spiral galaxies). It would be fascinating to know what Arp 122 will look like once this collision is complete . . . but that will not happen for a long, long time. 


Credit: European Space Agency/Hubble & NASA, J. Dalcanton, Dark Energy Survey/DOE/FNAL/DECam/CTIO/NOIRLab/NSF/AURA

Acknowledgement: L. Shatz

Release Date: Jan. 8, 2024


#NASA #ESA #Hubble #Astronomy #Space #Science #Stars #Galaxies #Galaxy #Arp122 #NGC6040 #NGC6041 #SpiralGalaxies #MergingGalaxies #Hercules #Constellation #Cosmos #Universe #HST #HubbleSpaceTelescope #GSFC #STScI #NOIRLab #AURA #NSF #DOE #UnitedStates #Europe #STEM #Education