Wednesday, June 07, 2023

What might NASA's Artemis III astronauts encounter at the lunar south pole?

What might NASA's Artemis III astronauts encounter at the lunar south pole?

Join a livestream by the Lunar & Planetary Institute (LPI), belonging to the Universities Space Research Association (USRA), Thursday, June 8, 2023, at 7:30 p.m. CT (8:30pm ET) for a presentation by Dr. David Kring, Principal Scientist at the Lunar and Planetary Institute in Houston, Texas, via the LPI YouTube channel: https://lnkd.in/gddKsruv

Artemis III astronauts will land on a fascinatingly cold and rugged terrain in the lunar south polar region. Far different than terrains traversed by Apollo astronauts, the south polar terrain presents new and exciting scientific opportunities to learn more about the Moon. Dr. Kring will discuss this unique environment and what astronauts may encounter during traverses of this unexplored region.


Credit: USRA


#NASA #Space #Astronomy #Science #Moon #SouthPole #ArtemisProgram #ArtemisIIIMission #Astronauts #HumanSpaceflight #Geology #Lunar #Technology #Engineering #LPI #UnitedStates #Livestream #PublicEvent #STEM #Education

Starburst Galaxy Messier 94 | Hubble Space Telescope

Starburst Galaxy Messier 94 | Hubble Space Telescope


This image shows the galaxy Messier 94, which lies in the small northern constellation of the Hunting Dogs, about 16 million light-years away.

Within the bright ring around Messier 94 new stars are forming at a high rate and many young, bright stars are present within it—thanks to this feature called a starburst ring.

The cause of this peculiarly shaped star-forming region is likely a pressure wave going outwards from the galactic center, compressing the gas and dust in the outer region. The compression of material means the gas starts to collapse into denser clouds. Inside these dense clouds, gravity pulls the gas and dust together until temperature and pressure are high enough for stars to be born.


Credit: European Space Agency (ESA)/Hubble & NASA

Release Date: Oct. 19, 2015


#NASA #Astronomy #Space #Science #Galaxy #Messier94 #M94 #Spiral #Starburst #StarburstRing #DoubleRingGalaxy #CanesVenatici #Constellation #Cosmos #Universe #Hubble #HST #SpaceTelescope #ESA #Europe #STScI #GSFC #UnitedStates #STEM #Education

Spiral Galaxy Messier 94: A Double Ring Galaxy

Spiral Galaxy Messier 94: A Double Ring Galaxy

Most galaxies do not have any rings of stars and gas—why does Messier 94 (M94) have two? First, spiral galaxy M94 has an inner ring of newly formed stars surrounding its nucleus, giving it not only an unusual appearance but also a strong interior glow. A leading origin hypothesis holds that an elongated knot of stars known as a bar rotates in M94 and has generated a burst of star formation in this inner ring. Observations have also revealed another ring, an outer ring, one that is more faint, different in color, not closed, and relatively complex. What caused this outer ring is currently unknown. 

M94, pictured here, spans about 45,000 light years in total, lies about 15 million light years away, and can be seen with a small telescope toward the constellation of the Hunting Dogs (Canes Venatici).


Image Credit & Copyright: Brian Brennan

Brian's Instagram Page: https://www.instagram.com/astrolips2000/

Release Date: June 7, 2023


#NASA #Astronomy #Space #Science #Galaxy #Messier94 #M94 #Spiral #Starburst #DoubleRingGalaxy #CanesVenatici #Constellation #Astrophotography #Astrophotographer #BrianBrennan #CitizenScience #APoD #STEM #Education

Planet Mars: On the Floor of Mawrth Vallis | NASA's Mars Reconnaissance Orbiter

Planet Mars: On the Floor of Mawrth Vallis | NASA's Mars Reconnaissance Orbiter


Data from the Mars Reconnaissance Orbiter's CRISM instrument shows a localized, unique spectral phase consistent with polyhydrated sulfate or zeolite here on the Mawrth Vallis channel floor, with implications for the regional history. We want to look for potential textural differences between new hydrated mineral and adjacent clays.

Mawrth Vallis is a valley on Mars, located in the Oxia Palus quadrangle at 22.3°N, 343.5°E with an elevation approximately two kilometers below datum. Situated between the southern highlands and northern lowlands, the valley is a channel formed by massive flooding which occurred in Mars’ ancient past. It is an ancient water outflow channel with light-colored clay-rich rocks.

Prior to the selection of Gale Crater for NASA's Mars Science Laboratory (MSL) Curiosity rover mission, Mawrth Vallis was considered as a potential landing site because of the detection of a stratigraphic section rich in clay minerals. Clay minerals have implications for past aqueous environments as well as the potential to preserve biosignatures, making them ideal targets for the search for life on Mars.

The University of Arizona, Tucson, operates the Mars Reconnaissance Orbiter's High Resolution Imaging Science Experiment (HiRISE) instrument, which 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.

Image cutout is less than 1 km (under a mile) top to bottom and the spacecraft altitude was 285 km (177 mi) and north is to the right.

Acquisition date

May 21, 2011

Local Mars time

14:05

Latitude (centered)

22.982°

Longitude (East)

341.496°

Spacecraft altitude

285.4 km (177.4 miles)


Credit: NASA/JPL-Caltech/University of Arizona

Release Date: June 6, 2023


#NASA #Space #Astronomy #Science #Mars #Planet #RedPlanet #MawrthVallis #Valley #Clays #Biosignatures #Geology #Landscape #Terrain #Geoscience #MRO #MarsReconnaissanceOrbiter #Spacecraft #HiRISE #Camera #JPL #Caltech #UniversityOfArizona #BallAerospace #STEM #Education

China's Lijian-1 Commercial Rocket Launches 26 Satellites Breaking National Record

China's Lijian-1 Commercial Rocket Launches 26 Satellites Breaking National Record

The second Lijian-1 launch vehicle (Lijian-1 Y2) successfully launched 26 small satellites from the Jiuquan Satellite Launch Center, Gansu Province, China, on June 7, 2023, at 04:10 UTC (12:10 local time). This set a record for the highest number of satellites launched atop a single rocket in the country. Lijian-1 is now China's largest and most powerful solid-fueled launch vehicle.

The Lijian-1 rocket, also known as ZK-1A and Kinetica-1, is a four-stage solid-propellant launch vehicle jointly developed by the Institute of Mechanics of the Chinese Academy of Sciences and CAS Space (Beijing Zhongke Aerospace Exploration Technology Co., Ltd.). 

Learn more about CAS Space:
https://en.cas-space.com/


Credit: China Central Television (CCTV)/CAS Space

Acknowledgement: SciNews

Duration: 1 minute, 51 seconds

Release Date: June 7, 2023


#NASA #Space #Science #Earth #China #中国 #CASSPace #Lijian1Y2Rocket #力箭一号遥二 #力箭一号 #Kinetica1Rocket #ZK1A #CarrierRocket #SolidPropellantRocket #Launch #Satellites #CommercialSatellites #ChineseTechnology #ChineseEngineering #JiuquanSatelliteLaunchCenter #GansuProvince #STEM #Education #HD #Video

Tuesday, June 06, 2023

The Phantom Galaxy: M74 | NASA's Webb Telescope & Chandra Observatory

The Phantom Galaxy: M74 | NASA's Webb Telescope & Chandra Observatory

Messier 74, nicknamed the Phantom Galaxy, is also a spiral galaxy—like our Milky Way—that we see face-on from our vantage point on Earth. It is about 32 million light-years away. Messier 74 is relatively dim, making it harder to spot with small telescopes than other galaxies in Charles Messier’s famous catalog from the 18th century. Webb outlines gas and dust in the infrared while Chandra data spotlights high-energy activity from stars at X-ray wavelengths. Hubble optical data showcases additional stars and dust along the dust lanes. (X-ray: purple; optical: orange, cyan, blue, infrared: green, yellow, red, magenta)

NASA's Marshall Space Flight Center manages the Chandra program. The Smithsonian Astrophysical Observatory's Chandra X-ray Center controls science operations from Cambridge, Massachusetts, and flight operations from Burlington, Massachusetts.

The James Webb Space Telescope is the world’s premier space science observatory. Webb will solve mysteries in our solar system, look beyond to distant worlds around other stars, and probe the mysterious structures and origins of our universe and our place in it. Webb is an international program led by NASA with its partners, the European Space Agency (ESA) and the Canadian Space Agency (CSA).


Image Credits: 

X-ray: Chandra: NASA/CXC/SAO

Infrared: NASA/ESA/CSA/STScI

Release Date: May 23, 2023


#NASA #ESA #Astronomy #Space #Science #Galaxy #Spiral #Messier74 #M74 #PhantomGalaxy #NGC628 #Pisces #Constellation #Hubble #HST #JamesWebb #WebbTelescope #JWST #Infrared #SpaceTelescopes #ChandraXrayObservatory #Universe #UnfoldTheUniverse #Europe #CSA #Canada #GSFC #MSFC #STScI #UnitedStates #STEM #Education

"A Hole in the Sky": Molecular Cloud LDN1774 (visible & infrared view) | ESO

"A Hole in the Sky": Molecular Cloud LDN1774 (visible & infrared view) | ESO


Rather than showing spectacular objects, some of the most surprising images of the Universe instead focus on emptiness. This image from the 2.2-meter MPG/ESO telescope shows dark tentacles swirling outwards from a dark, blank spot of space in the center of the frame, particularly conspicuous against the dense peppering of bright gold and red stars across the rest of the image. This molecular cloud is cataloged as LDN1774.

This region is not a hole in the cosmos, or an empty patch of sky. The dark lanes are actually made up of thick, opaque dust lying between us and the packed star field behind it. This obscuring dust forms part of a dark molecular cloud, cold and dense areas where large quantities of dust and molecular gas mingle and block the visible light emitted by more distant stars.

It is still unclear how these clouds form, but they are thought to be the very early stages of new star formation—in the future, the subject of this image may well collapse inwards on itself to form a new star system.

This image was taken by the Wide Field Imager, an instrument mounted on the European Southern Observatory’s 2.2-meter MPG/ESO telescope at La Silla, Chile.


Credit: European Southern Observatory (ESO)

Release Date: May 4, 2015


#NASA #ESO #Astronomy #Space #Science #Stars #Nebulae #StarFormation #MolecularCloud #Infrared #Visible #Ophiuchus #Constellation #MilkyWayGalaxy #Cosmos #Universe #Telescope #VLT #LaSilla #Chile #SouthAmerica #Europe #STEM #Education

Recientemente: Regreso de una tripulación comercial | NASA

Recientemente: Regreso de una tripulación comercial | NASA

FriendsofNASA.org: "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." 

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

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

Credit: National Aeronautics and Space Administration (NASA)

Duration: 2 minutes, 23 seconds

Release Date: June 6, 2023


#NASA #Space #ISS #NASAenespañol #español #Axiom #AxiomSpace #Ax2Mission #Ax2 #AX2Crew #Astronauts #PeggyWhitson #JohnShoffner #AliAlqarni #RayyanahBarnawi #SpaceX #CrewDragon #Science #MicrogravityResearch #SpaceLaboratory #UAE #SaudiArabia #SaudiSpaceCommission #Cosmonauts #Russia #UnitedStates #STEM #Education #HD #Video

NGC 4839 Galaxy Group Leaves Fiery Tail Behind | NASA Chandra

NGC 4839 Galaxy Group Leaves Fiery Tail Behind | NASA Chandra

A group of galaxies is plunging into the Coma galaxy cluster and leaving behind an extraordinary tail of superheated gas. Astronomers have confirmed this is the longest known tail behind a galaxy group and used it to gain a deeper understanding of how galaxy clusters—some of the largest structures in the Universe—grow to their enormous sizes.

Astronomers trained NASA’s Chandra X-ray Observatory on the galaxy group NGC 4839. Galaxy groups are collections of about 50 galaxies or less that are bound together by gravity. Galaxy clusters are even larger and can contain hundreds or thousands of individual galaxies.

Both galaxy clusters and galaxy groups are enveloped by huge amounts of hot gas that are best studied using X-rays. These superheated pools of gas, though extremely thin and diffuse, represent a significant portion of the mass in galaxy groups or clusters and are crucial for understanding these systems.

NGC 4839 is located near the edge of the Coma galaxy cluster, one of the largest known clusters in the Universe about 340 million light-years away. As NGC 4839 moves toward the center of the Coma cluster, the hot gas in the galaxy group is stripped away by its collision with gas in the cluster. This results in a tail forming behind the galaxy group.

This comet-like tail is 1.5 million light-years long, or hundreds of thousands of times the distance between the Sun and the nearest star, making it the longest tail ever seen trailing behind a group of galaxies. This gas is a key ingredient in making future generations of stars and planets.

The current brightness of the tail gives astronomers a special chance to study the tail’s gas before it mixes in with the hot gas in the cluster and becomes too faint to study. The gas in the tail behind NGC 4839 will ultimately merge with the large amount of hot gas already present in the Coma Cluster.


Credit: NASA's Chandra X-ray Observatory

Duration: 2 minutes, 35 seconds

Release Date: June 6, 2023


#NASA #Astronomy #Space #Science #Chandra #Xray #Galaxy #NGC4839 #TypecDGalaxy  #ComaCluster #GalaxyGroup #Eridanus #Constellation #Cosmos #Universe #Observatory #SpaceTelescope #MSFC #JPL #Caltech #UnitedStates #STEM #Education #HD #Video

Global Mars: Celebrating 20 Years of Europe's Mars Express Orbiter

Global Mars: Celebrating 20 Years of Europe's Mars Express Orbiter

To mark 20 years of Europe’s Mars Express mission, the High Resolution Stereo Camera (HRSC) team produced a new global color mosaic revealing the planet’s surface color and composition in spectacular detail.

This graphic highlights the Mars Express mission’s most impressive numbers to date, from the 1.1 billion km travelled over 24 000+ Mars orbits to the 170+ PhD students trained and 1800+ scientific papers published using Mars Express data.

Two decades ago, on June 2, 2003, the European Space Agency’s Mars Express orbiter launched and began its journey to the Red Planet—Europe’s first ever mission to Mars. The spacecraft entered orbit around Mars in December 2003. It used its vantage point to study the martian atmosphere and climate, unravel the planet’s structure, mineralogy and geology, and search for traces of water across its surface. The mission carried a state-of-the-art package of eight instruments to achieve this, enabling it to probe surface, subsurface, atmosphere and more.

Mars Express has now been in space for two decades, despite a planned initial lifetime of just 687 Earth days. It has achieved its aforementioned aims and revealed a wealth of knowledge about Mars in that time, making it undeniably one of the most successful missions ever sent to the Red Planet.

The orbiter will continue its study of Mars until at least the end of 2026, with an indicative extension from January 1, 2027 to December 31, 2028 to support the JAXA-led Mars Moons eXploration (MMX) mission (Japan), followed by two years of post-operations.

Mars Express has conducted data relay for seven rovers and landing platforms (more information), and enabled scientific collaboration with a further five orbiters.

The past 20 years of observations from Mars Express have solidified our picture of Mars as a once-habitable planet, with warmer and wetter epochs that may have been oases for ancient life. This is a monumental shift from our previous view of the planet, which characterized it as an eternally cold and arid world.

Mars Express has identified and mapped signs of past water across Mars—from minerals that only form in the presence of water to water-carved valleys, groundwater systems, and ponds lurking below ground—and traced its influence and prevalence through martian history. It has peered deep into the martian atmosphere, mapping how gases (water, ozone, methane) are distributed and escape to space, and watching as dust is whipped up from the surface into the air. The mission has seen giant dust storms engulf the planet, creating familiar clouds like those we see on Earth, and tracked rare ultraviolet auroras. 

The orbiter has seen signs of recent and episodic volcanism and tectonics, and explored the planet’s unique surface features, mapping 98.8% of Mars and creating thousands of 3D images of impact craters, canyons (including the Valles Marineris system), the planet’s icy poles, immense volcanoes and more.

This is a simulated view of Mars from a vantage point 2,500 km above the colossal Valles Marineris canyon system, with enhanced color and contrast (at this relatively low altitude, the planet’s polar caps are not visible). It is a composite of red, green and blue filter mosaics with the color band values stretched individually, and has a spatial resolution of 2 km per pixel (although higher resolution data products are possible and already in the works).

Darker grey-toned areas of Mars represent grey-black basaltic sands of volcanic origin; lighter patches show clay and sulphate minerals; and the large scar across the planet's face is Valles Marineris.


Image Credit: ESA/DLR/FU Berlin/G. Michael, CC BY-SA 3.0 IGO

Release Date: May 23-June 6, 2023


#NASA #ESA #Space #Astronomy #Science #Planet #Mars #GlobalMap #Geology #MarsExpress #MarsExpressSpacecraft #HRSC #20thAnniversary #Europe #DLR #FUBerlin #Berlin #Germany #Deutschland #Infographic #STEM #Education

NASA Artemis III Moon Rocket Hardware Production: LVSA

NASA Artemis III Moon Rocket Hardware Production: LVSA

Technicians apply thermal protection material to launch vehicle stage adapter (LVSA)




These photos show the launch vehicle stage adapter (LVSA) of NASA’s Space Launch System (SLS) rocket for Artemis III before technicians at NASA’s Marshall Space Flight Center in Huntsville, Alabama, applied the thermal protection system to it. Artemis III will land astronauts, including the first woman and first person of color, on the Moon to advance long-term lunar exploration and scientific discovery and to inspire the Artemis Generation. 

 Teams at Marshall began applying the thermal protection system material in the spring of 2023. Unlike other parts of the SLS rocket, the thermal protection system material for the LVSA is applied entirely by hand using a spray gun. During application, the technicians use a thin measuring rod to gauge the proper thickness. Once the thermal protection system has cured, certain areas are sanded down to meet parameters. The entire process takes several months.

The LVSA is fully manufactured at Marshall by NASA, lead contractor Teledyne Brown Engineering, and the Jacobs Space Group’s ESSCA contract. The LVSA for Artemis III is the last of its kind as future SLS rockets will transition to its next, more powerful Block 1B configuration beginning with Artemis IV.

NASA is working to land the first woman and first person of color on the Moon under Artemis. SLS is part of NASA’s backbone for deep space exploration, along with the Orion spacecraft, advanced spacesuits and rovers, the Gateway in orbit around the Moon, and commercial human landing systems. SLS is the only rocket that can send Orion, astronauts, and supplies to the Moon in a single mission.

The LVSA for Artemis III is the last of its kind as future SLS rockets will transition to its next, more powerful Block 1B configuration beginning with Artemis IV. SLS is part of NASA’s backbone for deep space exploration, along with the Orion spacecraft, advanced spacesuits and rovers, the Gateway in orbit around the Moon, and commercial human landing systems.

Image Credit: Brandon Hancock/NASA 

Location: NASA's Marshall Space Flight Center (MSFC)

Image Date: April 26, 2023


#NASA #Space #Earth #Moon #Artemis #ArtemisIII #SLS #Boeing #MoonRocket #LVSA #TeledyneBrownEngineering #DeepSpace #MoonToMars #Astronauts #Science #Engineering #Technology #SpaceExploration #SolarSystem #NASAMarshall #MSFC #Alabama #UnitedStates #STEM #Education

Planet Mars Images: June 2023 | NASA's Curiosity & Perseverance Rovers | JPL

Planet Mars Images: June 2023 | NASA's Curiosity & Perseverance Rovers | JPL

MSL - sol 3848

MSL - sol 3848

MSL - sol 3848

MSL - sol 3848

MSL - sol 3846

MSL - sol 3846

Mars2020 - sol 813

Mars2020 - sol 812

Celebrating 10 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 (2021-2023)

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 possible 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/Arizona State University/Malin Space Science Systems (MSSS)

Processing: Kevin M. Gill

Image Release Dates: June 3-5, 2023


#NASA #Space #Astronomy #Science #Mars #RedPlanet #Planet #Astrobiology #Geology #CuriosityRover #MSL #MountSharp #GaleCrater #PerseveranceRover #Mars2020 #IngenuityHelicopter #JezeroCrater #Robotics #Technology #Engineering #JPL #Caltech #ASU #MSSS #UnitedStates #MoonToMars #CitizenScience #KevinGill #STEM #Education

Axiom Space Ax-2 Post-Return Crew Press Conference

Axiom Space Ax-2 Post-Return Crew Press Conference

After returning to Earth from a 10-day mission in space, the astronauts of the Axiom Mission 2 (Ax-2) will participate in a press conference to share their experience and highlight the work conducted during the second all-private astronaut mission to the International Space Station (ISS). 

The Ax-2 crew includes Axiom Space’s Director of Human Spaceflight and Commander Peggy Whitson, a former NASA astronaut, Pilot John Shoffner, and Mission Specialists Ali Alqarni and Rayyanah Barnawi, from the Saudi Space Commission (SSC). Both are members of the inaugural Saudi national astronaut class.  

Rayyanah Barnawi made history as the first Arab woman aboard the International Space Station. She  became the 600th astronaut.

Mission Commander Peggy Whitson  (United States) Axiom Space Biography

https://www.axiomspace.com/astronaut/peggy-whitson

Mission Specialist Ali Alqarni (Saudi Arabia) Axiom Space Biography

https://www.axiomspace.com/astronaut/ali-alqarni

Mission Specialist Rayyanah Barnawi (Saudi Arabia) Axiom Space Biography

https://www.axiomspace.com/astronaut/rayyanah-barnawi

Pilot John Shoffner (United States) Axiom Space Biography

https://www.axiomspace.com/astronaut/john-shoffner 

More information about Axiom and the Ax-2 Mission can be found at: www.axiomspace.com


Credit: Axiom Space

Duration: 52 minutes

Release Date: June 1, 2023

#NASA #Space #ISS #Axiom #AxiomSpace #Ax2Mission #Ax2 #AX2Crew #Astronauts #PeggyWhitson #JohnShoffner #AliAlqarni #RayyanahBarnawi #SpaceX #CrewDragon #CommercialSpace #Science #MicrogravityResearch #SpaceLaboratory #InternationalCooperation #SaudiArabia #SaudiSpaceCommission #UnitedStates #STEM #Education #History #HD #Video

Monday, June 05, 2023

Reducing Satellite Interference in Hubble Space Telescope Images

Reducing Satellite Interference in Hubble Space Telescope Images

NGC 4676: Example of Satellite Trail in Hubble Space Telescope Exposure

Earth-Orbiting Objects Leave the Equivalent of "Scratch Marks" on Space Photos

Image Description: A large pair of colliding galaxies, sporting long tails of blue stars and gas emanating from each galaxy, is shown at the center of a primarily dark background. The trail of an artificial satellite is seen as the bright white band running across the top of the galaxies diagonally from the middle-left of the image towards the upper-right corner of the image. NGC 4676, or the Mice Galaxies, are two spiral galaxies in the constellation Coma Berenices. About 290 million light-years distant, they have begun the process of colliding and merging. 

When the Hubble Space Telescope was launched in 1990, there were about 470 artificial satellites orbiting Earth. By 2000, that number doubled. But by 2023, the rising number has grown almost exponentially to nearly 8,000 satellites. For Hubble this means that satellites photobomb about 10% of its exposures on celestial targets. However, a typical satellite trail is very thin and will affect less than 0.5% of a single Hubble exposure.

Nevertheless, these denizens leave annoying pencil-thin, white streaks across a Hubble image as they zoom overhead. And, they are not the only image artifacts Hubble astronomers have to contend with. Cosmic rays rain onto Hubble's camera detectors. These leave what looks like "scratch marks" too. In fact, they are a bigger nuisance than satellite trails.

Astronomers at the Space Telescope Science Institute in Baltimore, Maryland have developed tools for cleaning up this clutter. Hubble observations consist of more than just one exposure. And so, artifacts can be identified and subtracted between exposures because they are not in the same place on a detector.

It is estimated that by 2030 there could be ten times as many satellites circling Earth as there are now. Even as the number of satellites increases, the Space Telescope Science Institute's tools for cleaning the Hubble pictures will remain useful. To date not one Hubble science program has been affected by satellite trails.

Artificial satellites are photobombing the Hubble Space Telescope's snapshots as much as every two to four hours, according to researchers at Baltimore's Space Telescope Science Institute (STScI).

As they whirl around Earth, the satellites leave streaks across an image, like scratches on photographic film. Hubble is in a low-Earth orbit and so many satellites in higher orbits sweep overhead. As many as 8,000 satellites circle Earth—more than half for telecommunications.

But not to worry—experts say that they are not a threat to the celebrated telescope's ongoing observations of the universe.

"We developed a new tool to identify satellite trails that is an improvement over the previous satellite software because it is much more sensitive. So we think it will be better for identifying and removing satellite trails in Hubble images," said Dave Stark of STScI.

Stark applied the new tool, based on the image analysis technique known as the Radon Transform, to identify satellite trails across Hubble's camera with the widest field of view, the Advanced Camera for Surveys (ACS).

In 2002 the satellite streaks were present in five percent of ACS exposures, with many of those too faint to discern easily. This rose to ten percent by 2022, although the typical brightness of the detected trails remained unchanged.

As the number of artificial satellites encircling Earth rises, sky contamination for all telescopes based on the ground or in Earth orbit becomes increasingly worse.

"To date, these satellite trails have not had a significant impact on research with Hubble," said Tom Brown, Head of STScI's Hubble Mission Office. "The cosmic rays that strike the telescope's detectors are a bigger nuisance."

Previous studies regarding Hubble do not pick up the fainter satellite trails. The new software is up to ten times more sensitive than prior software developed by STScI to detect satellite trials, and it identifies roughly twice as many trails as other studies.

"We have a toolbox of things that people use to clean Hubble data and calibrate it. And our new application is another tool that will help us make the best out of every Hubble exposure," said Stark.

Read the full release: 

https://www.stsci.edu/contents/media/images/2023/017/01H1Q4K5J650PPH3HM9Y88N7TA 


Credit: NASA, European Space Agency (ESA), Space Telescope Science Institute (STScI)

Image Date: June 5, 2023


#NASA #Hubble #Astronomy #Space #Satellites #Science #Galaxies #NGC4676 #MiceGalaxies #InteractingGalaxies #ComaBerenices #Constellation #Cosmos #Universe #HST #SpaceTelescope #ESA #Europe #GSFC #STScI #UnitedStates #STEM #Education

NASA SpaceX CRS-28 ISS Cargo Resupply Launch | Kennedy Space Center

NASA SpaceX CRS-28 ISS Cargo Resupply Launch | Kennedy Space Center






A SpaceX Falcon 9 rocket launched the CRS-28 Dragon spacecraft from Launch Complex 39A (LC-39A) at NASA’s Kennedy Space Center in Florida, on June 5, 2023 at 11:47 ET. The CRS-28 Dragon cargo spacecraft is scheduled to autonomously dock to the International Space Station (ISS) on June 6, 2023, at approximately 5:50 ET. 

Following stage separation, Falcon 9’s first stage landed on the “A Shortfall of Gravitas” droneship, stationed in the Atlantic Ocean. Falcon 9’s first stage (B1077) previously supported four missions: Crew-5, GPS III SV06, Inmarsat-6 F2 and one Starlink mission. CRS-28 is the fourth flight for this Dragon spacecraft, which previously flew CRS-21, CRS-23 and CRS-25 to the space station.

Dragon will deliver approximately 7,000 pounds of crew supplies, equipment, and science experiments to the orbiting laboratory. Dragon is also carrying two new roll-out solar arrays that will be extracted from its unpressurized trunk about two days after its docking then staged on a pallet attached to the station’s starboard-side truss structure. 

The Dragon spacecraft is expected to spend about a month attached to the orbiting outpost before it returns to Earth with research and return cargo, splashing down off the coast of Florida.


Credit: NASA/SpaceX

Release Date: June 5, 2023


#NASA #Space #ISS #Earth #SpaceX #Falcon9Rocket #DragonSpacecraft #CRS28 #CommercialResupplyServices #ElonMusk #GwynneShotwell #Astronauts #Cosmonauts #HumanSpaceflight #Technology #Engineering #Spaceport #CapeCanaveral #Florida #UnitedStates #Russia #UAE #STEM #Education

Markarian's Chain's in Virgo | Canada-France-Hawaii Telescope

Markarian's Chain's in Virgo | Canada-France-Hawaii Telescope

Markarian's Chain is a stretch of galaxies that forms part of the Virgo Cluster. When viewed from Earth, the galaxies lie along a smoothly curved line. Near the center there appear the pair of interacting galaxies NGC 4438 and NGC 4435, about 50 million light-years away, known to some as Markarian's Eyes.


Credit & Copyright © 2022 Canada-France-Hawaii Telescope (CFHT)

- Data obtained using the CFHT MegaCam camera

- Image by Jean-Charles Cuillandre (CFHT) & Giovanni Anselmi (Coelum)

Release Date: June 2022


#NASA #Space #Astronomy #Science #Galaxies #Messier84 #Messier86 #MarkariansChain #Virgo #Constellation #CanadaFranceHawaiiTelescope #Telescope #Hawaii #UnitedStates #STEM #Education