Monday, August 24, 2026

Nancy Grace Roman Space Telescope: Launch Preparations | NASA Kennedy

Nancy Grace Roman Space Telescope: Launch Preparations | NASA Kennedy

NASA’s Nancy Grace Roman Space Telescope is photographed after encapsulation inside its payload fairing in the Payload Hazardous Servicing Facility at NASA’s Kennedy Space Center in Florida on Monday, Aug. 24, 2026.
Teams inside the Payload Hazardous Servicing Facility at NASA’s Kennedy Space Center in Florida encapsulate the agency’s Nancy Grace Roman Space Telescope within the payload fairing on Friday, Aug. 21, 2026, ahead of mating to a SpaceX Falcon Heavy rocket.






Dr. Nancy Grace Roman visits James Webb Space Telescope (JWST) and the Hubble Project Team on March 31, 2017.

NASA’s Nancy Grace Roman Space Telescope is photographed during the encapsulation process inside its payload fairing in the Payload Hazardous Servicing Facility at NASA’s Kennedy Space Center in Florida on Monday, Aug. 24, 2026, ahead of mating to a SpaceX Falcon Heavy rocket. Encapsulation shields the spacecraft during rollout, ascent, and the early phases of flight. Roman will investigate dark energy and dark matter, conduct a statistical census of planetary systems, and enable a broad range of additional astrophysics research. Liftoff from Launch Complex 39A at Kennedy is targeted for no earlier than Sunday, Aug. 30, 2026. 

Roman’s primary mission is to settle essential questions about dark energy, exoplanets, and infrared astrophysics by conducting wide-field surveys that explore the universe’s structure, evolution, and composition. 

The Roman telescope and the discoveries it will support:
https://www.stsci.edu/roman

Roman’s namesake—Dr. Nancy Grace Roman, NASA’s first chief astronomer—made it her personal mission to make cosmic vistas readily accessible to all by paving the way for telescopes based in space.

“The mission will acquire enormous quantities of astronomical imagery that will permit scientists to make groundbreaking discoveries for decades to come, honoring Dr. Roman’s legacy in promoting scientific tools for the broader community,” said Jackie Townsend, Roman’s deputy project manager at NASA Goddard. “I like to think Dr. Roman would be extremely proud of her namesake telescope and thrilled to see what mysteries it will uncover in the coming years.”


Image Credit: NASA/Sydney Rohde (Rocz)
Image Date: Aug. 24, 2026

#NASA #Space #Astronomy #Science #NASARoman #RomanSpaceTelescope #Encapsulation #NancyGraceRomanSpaceTelescope #NancyGraceRoman #Exoplanets #Planets #SolarSystem #Stars #MilkyWayGalaxy #Galaxies #Cosmos #Universe #SpaceTelescopes #NASAGoddard #GSFC #STScI #NASAKennedy #Florida #UnitedStates #STEM #Education

Gullies at the Start of Martian Spring | NASA's Mars Reconnaissance Orbiter

Gullies at the Start of Martian Spring | NASA's Mars Reconnaissance Orbiter

NASA's Mars Reconnaissance Orbiter (MRO) regularly takes repeat images of gullies to look for changes. Carbon dioxide (CO₂) ice blocks on Mars may dig gullies as they slide and sublimate in the thin atmosphere. Sublimation is the transition of a substance from solid to gas without becoming liquid.

This site is one of the most frequent monitoring sites with more than 70 images to date. It is imaged frequently due to the latitude. The gullies have a long season with carbon dioxide frost (dry ice) moving rocks and dust around the surface. In past images, we have seen many changes to the frost patterns and the underlying ground.

This image is the first one for this Mars year. However, you can already see dark spots where gas is breaking out from under the frost and taking sand and dust with it. MRO will try to take more images this year to see how the surface changes.

This HiRISE enhanced color camera image (less than 1 km in size) was captured by NASA's Mars Reconnaissance Orbiter (MRO) at an altitude of 252 km (~157 miles).

NASA's Mars Reconnaissance Orbiter has spent over twenty years (2006-2026) orbiting the Red Planet, collecting valuable scientific data. 

The University of Arizona, in Tucson, operates the High Resolution Imaging Science Experiment (HiRISE). It was built by BAE Systems in 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 (SMD), Washington.

For more information on MRO, visit:

Image Credit: NASA/JPL-Caltech/University of Arizona
Image Date: 
Nov. 23, 2025
Release Date: Aug. 24, 2026

#NASA #Space #Astronomy #Science #Mars #Planets #RedPlanet #Geology #Geoscience #Landscapes #Terrain #Gullies #CarbonDioxide #CO2 #CarbonDioxideIce #MRO #MarsOrbiter #MarsSpacecraft #HiRISECamera #JPL #Caltech #UA #UnitedStates #STEM #Education

Expedition 75: Menon & Adenot on Spacewalk | International Space Station

Expedition 75: Menon & Adenot on Spacewalk | International Space Station

From left, Expedition 75 flight engineers Sophie Adenot of the European Space Agency (ESA) and Anil Menon of NASA work together during a six‑hour, 23‑minute spacewalk outside the International Space Station. Adenot worked at the Z1 truss segment while Menon rode the Canadarm2 robotic arm and carried a space-to-ground antenna that the duo later tied down to the Z1. 

NASA astronaut and Expedition 75 flight engineer Anil Menon on a spacewalk working on a space-to-ground antenna.
European Space Agency astronaut Sophie Adenot and Expedition 75 flight engineer on a spacewalk.
European Space Agency astronaut Sophie Adenot and Expedition 75 flight engineer on a spacewalk during orbital night.
European Space Agency (ESA) astronaut and Expedition 75 flight engineer Sophie Adenot is pictured inside the International Space Station's Quest airlock with her helmet visor down as she nears the end of a six‑hour, 23‑minute spacewalk.
European Space Agency (ESA) astronaut and Expedition 75 flight engineer Sophie Adenot is pictured inside the International Space Station's Quest airlock as she nears the end of a six‑hour, 23‑minute spacewalk.
European Space Agency astronaut and Expedition 74 flight engineer Sophie Adenot is pictured inside the Quest airlock preparing to try on a spacesuit to verify its comfort, mobility, and functionality. Adenot was conducting an on-orbit fit verification of the suit before conducting her first spacewalk outside of the International Space Station.
Expedition 75 emblem

Flight engineers Anil Menon of NASA and Sophie Adenot of the European Space Agency (ESA) completed a six-hour and 23-minute spacewalk on Tuesday, August 18, 2026. During their extravehicular activity (EVA), the duo finished the removal of a failed space-to-ground antenna and performed a long-duration tie down of the unit on the space station truss structure. The crew members needed more time than expected to disconnect electrical cables and loosen bolts, delaying work to install a replacement antenna. The installation work is expected to be undertaken during another spacewalk.

U.S. Spacewalk 97 was Menon’s second career spacewalk and first for Adenot. She is the first French woman to conduct a spacewalk. It also was the 282nd spacewalk in support of space station assembly, maintenance, and upgrades.


Expedition 75 Crew
Station Commander: Jessica Meir
Roscosmos (Russia) Flight Engineers:
Andrey Fedyaev,
Anna Kikina, Pyotr Dubrov
European Space Agency Flight Engineer: Sophie Adenot
NASA Flight Engineers: Jack Hathaway, Anil Menon

An international partnership of space agencies provides and operates the elements of the International Space Station (ISS). The principals are the space agencies of the United States, Russia, Europe, Japan, and Canada.


Image Credits: NASA's Johnson Space Center/J. Hathaway/A. Menon/S. Adenot/Roscosmos/Anna Kikina
Image Dates: July 28-Aug. 6, 2026


#NASA #Space #Science #ISS #Planets #Earth #Astronauts #Spacewalks #USSpacewalk97 #EVAs #Spacesuits #AnilMenon #SophieAdenot #France #CNES #AstronautPhotography #Cosmonauts #Russia #Россия #Roscosmos #Роскосмос #HumanSpaceflight #Expedition75 #InternationalCooperation #UnitedStates #STEM #Education

US Astronaut Mike Fincke Departs NASA | International Space Station

US Astronaut Mike Fincke Departs NASA | International Space Station

NASA astronaut Edward M. (Mike) Fincke: Expedition 9 science officer and flight engineer, wearing a Russian Orlan spacesuit, participates in the third of four sessions of extravehicular activities (EVA) performed by the Expedition 9 crew during their six-month mission. Fincke and cosmonaut Gennady I. Padalka (out of frame), commander representing Russia's Federal Space Agency (Roscosmos), spent 4.5 hours outside the Station swapping out experiments and installing hardware associated with Europe's Automated Transfer Vehicle (ATV). Image Date: August 3, 2004
Commercial Crew Program Astronaut Training - Mike Fincke
Boeing CFT crew member Mike Fincke with backup Barry "Butch" Wilmore during Boeing CFT/59S BU ISS EVA Maintenance 1 PRF training.
Image Date: Feb. 1, 2019
Official Portrait of Astronaut Mike Fincke
Astronaut Edward Michael (Mike) Fincke, commander
Image Date: Feb. 16, 2004
Fincke wears his Russian Sokol pressure suit in the U.S. Lab module during Expedition 9
Astronaut Edward M. (Mike) Fincke, Expedition 9 NASA ISS science officer and flight engineer, wearing a Russian Sokol suit, gives a thumb's up as he floats in the Destiny laboratory of the International Space Station (ISS).
Image Date: July 7, 2004
Boeing OFT-2 Crew & Science Briefing
E. Michael “Mike” Fincke, NASA astronaut, Crew Flight Test, participates in a crew and science media briefing ahead of Boeing’s Orbital Flight Test-2 (OFT-2) during a crew and science briefing at the agency’s Kennedy Space Center in Florida, July 29, 2021.
Image Date:  July 29, 2021
NASA astronaut and SpaceX Crew-11 Pilot Mike Fincke waves to officials at Ellington Field in Houston, Texas. He departed the International Space Station and returned to Earth the day before aboard the Dragon spacecraft for a parachute-assisted splashdown off the coast of San Diego, California.
Image Date: Jan. 16, 2026
NASA astronaut Mike Fincke flashes a smile during leak checks for his SpaceX spacesuit inside the crew suit-up room in the Neil A. Armstrong Operations and Checkout Building at the agency’s Kennedy Space Center in Florida on Thursday, July 31, 2025, during the first attempt of NASA’s SpaceX Crew-11 mission to the International Space Station.
Image Date: July 31, 2025
Astronaut Edward M. (Mike) Fincke, Expedition 9 NASA ISS science officer and flight engineer, is pictured near fresh fruit floating freely in the Zvezda Service Module of the International Space Station (ISS).
Image Date: May 27, 2004

NASA astronaut Mike Fincke is departing the agency on Wednesday after 30 years of service. Throughout his career, he flew four missions, spent 549 days in space, and completed nine spacewalks in support of the International Space Station.

“Few people have had the opportunity to shape as many chapters of NASA’s history as Mike Fincke,” said NASA Administrator Jared Isaacman. “Over a remarkable career, Mike served our nation as a pilot, engineer, astronaut, and mentor. From long-duration missions aboard the International Space Station to helping prepare the Artemis generation, his contributions have helped position NASA for what comes next. The success we’re building on today is possible because of people like Mike, who dedicated their careers to moving our space program forward and preparing the next generation to carry the mission even further. I’d like to congratulate Mike on an incredible career and thank him for his decades of service to NASA, our nation, and the countless people who had the opportunity to learn from and fly alongside him.”

He ranks fourth among NASA astronauts in accumulated time in space, and his spacewalks total 48 hours and 37 minutes. Most recently, Fincke piloted NASA’s SpaceX Crew‑11 mission that launched in August 2025 and returned in January. During the mission, he served as a flight engineer for International Space Station Expedition 73 and commander of Expedition 74.

Fincke joined NASA’s 16th astronaut class in 1996 and first flew to space in 2004 aboard Soyuz TMA‑4 in support of the space station’s Expedition 9. Serving as a science officer and flight engineer, he helped maintain station systems and performed four spacewalks. He returned to space in 2008 on Soyuz TMA‑13 as commander of Expedition 18, preparing the space station for its transition to six‑person crews at the time and completing two more spacewalks.

In 2011, Fincke flew on STS‑134, the final flight of space shuttle Endeavour. As mission specialist and robotic arm operator, he completed three spacewalks and helped deliver and install the Alpha Magnetic Spectrometer.

“Mike’s remarkable career reflects three decades of dedication to NASA’s mission and the advancement of human spaceflight,” said Vanessa Wyche, director of NASA’s Johnson Space Center in Houston. “From his time aboard the International Space Station to his commitment to mentoring the next generation, Mike has made an immense impact across our agency. His legacy of service, mentorship, and dedication to exploration will continue to inspire the generations to come.”

Throughout his career, Fincke bridged spacecraft development, flight testing, and mission operations. Early in the International Space Station Program, he helped test and integrate several of the station’s initial modules before launch. His flight experience spanned multiple generations of human spacecraft, including two missions aboard Soyuz, one aboard the space shuttle, and later piloting the SpaceX Dragon.

Fincke was a foundational contributor to NASA’s Commercial Crew Program. As chief of the Astronaut Office’s Commercial Crew Branch, he worked to ensure astronaut needs, crew safety, and human spaceflight experience informed development of the nation’s next generation of crewed spacecraft. He spent five years supporting Boeing’s Crew Flight Test program training as a crew member and backup pilot, contributing to flight software, systems integration, integrated testing, and spacecraft interfaces.

Fincke also supported station operations from the ground as a crew test support team member in Russia, a capsule communicator, or capcom, and crew procedures team lead. He helped translate complex engineering and operational requirements into clear instructions for crews working in orbit. His continuity across development, integration, mission support, and long‑duration flight gave him an end‑to‑end perspective on space station assembly and operation.

“Mike approached every assignment with experience, humility, and an unwavering focus on the mission,” said Scott Tingle, chief of the Astronaut Office at NASA Johnson. “Whether flying aboard the station, supporting crews from the ground, or helping shape the spacecraft that future crews will rely on, he consistently strengthened our team. His legacy is woven into the way we fly today.”

A native of Emsworth, Pennsylvania, Fincke holds bachelor’s degrees in aeronautics and astronautics and in Earth, atmospheric, and planetary sciences from the Massachusetts Institute of Technology, where he also studied in the Soviet Union through an exchange program with the Moscow Aviation Institute. He earned master’s degrees in aeronautics and astronautics from Stanford University and in planetary geology from the University of Houston, Clear Lake.

Fincke is a retired U.S. Air Force colonel and distinguished graduate of the U.S. Air Force Test Pilot School. He served as a space systems engineer and flight test engineer at Edwards and Eglin Air Force Bases and later as the U.S. flight test liaison to the Japanese‑U.S. XF‑2 fighter program at Gifu Air Base in Japan. He accumulated more than 2,000 flight hours in more than 30 aircraft types.

“After exactly 30 years, I am departing NASA, but I remain deeply committed to the work of exploration.” Fincke said. “NASA gave me the extraordinary privilege of serving alongside remarkable people, flying and helping develop spacecraft, and contributing to the International Space Station from its earliest days through command in orbit. I am profoundly grateful to my crewmates, the teams on the ground, our international partners, and the families who make this work possible. I am excited to carry those lessons forward and help prepare the next generation of engineers, explorers, and leaders. Together, we will return humanity to the Moon, travel to Mars, journey outward to the planets and moons beyond Earth, and someday reach for the stars – all while caring for Earth, the most beautiful planet in our solar system.”

To learn more about NASA’s astronauts and space exploration, visit:
https://www.nasa.gov/astronauts


Credit: NASA's Johnson Space Center
Image Dates: Feb. 16, 2004-Jan. 16, 2026

 #NASA #Space #ISS #Science #Planets #Earth #DragonCrewSpacecraft #SpaceXCrew11 #Astronauts #MikeFincke #Cosmonauts #Russia #Россия #Roscosmos #Роскосмос #HumanSpaceflight #InternationalCooperation #Expedition9 #STS134 #Expedition74 #BoeingCCP #OFT2 #JSC #Houston #UnitedStates #STEM #Education

Sunday, August 23, 2026

Planet Mars: Mysterious, wind-blown features | NASA's Mars Reconnaissance Orbiter

Planet Mars: Mysterious, wind-blown features | NASA's Mars Reconnaissance Orbiter

Transverse aeolian ridges—or TAR—are mysterious, wind-blown features that are intermediate in size between ripples and much larger sand dunes.

Ripples form from hopping sand grains, and dunes form from sand grains being blown over longer distances. One hypothesis for TAR formation is that larger grains like pebbles are rolled on top of smaller ripples. Then, finer dust settles into the cracks, “inflating” the pebbles, making the TAR larger than typical ripples.

Looking between the TAR, one sees a network of ancient, beaten-up channels that were carved by water, lava, or both.

This whole area is located in Solis Planum, an interesting, tectonic terrain south of Noctis Labryinthus that generally slopes toward the south. Solis Planum is a planum on Mars which has a diameter of 1811.23 km. Its center latitude is 26.4 S and its center longitude is 270.33 E. Noctis Labyrinthus (Latin for 'Labyrinth of the Night') is a region of Mars located in the Phoenicis Lacus quadrangle, between Valles Marineris and the Tharsis upland. The region is notable for its maze-like system of deep, steep-walled valleys. 

This HiRISE enhanced color camera image (less than 1 km in size) was captured by NASA's Mars Reconnaissance Orbiter (MRO) at an altitude of 252 km (~157 miles).

NASA's Mars Reconnaissance Orbiter (MRO) has spent over twenty years (2006-2026) orbiting the Red Planet, collecting valuable scientific data. 

The University of Arizona, in Tucson, operates the High Resolution Imaging Science Experiment (HiRISE). It was built by BAE Systems in 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 (SMD), Washington.

For more information on MRO, visit:

Image Credit: NASA/JPL-Caltech/University of Arizona
Image Date: Aug. 30, 2015
Release Date: Aug. 23, 2026

#NASA #Space #Astronomy #Science #Mars #Planets #RedPlanet #Geology #Geoscience #Landscapes #Terrain #TransverseAeolianRidges #TAR #SolisPlanum #SouthernHemisphere #MRO #MarsOrbiter #MarsSpacecraft #HiRISECamera #JPL #Caltech #UA #UnitedStates #STEM #Education

Shenzhou-23 Crew Advances Experiments, Health Monitoring | China Space Station

Shenzhou-23 Crew Advances Experiments, Health Monitoring | China Space Station

China's Shenzhou-23 astronauts have pressed ahead with a full slate of space science experiments, while also carrying out routine station upkeep and comprehensive health management tasks over the past week as they will mark their first three months in orbit, according to the China Manned Space Agency (CMSA).

According to the mission schedule, the three crew members of Zhu Yangzhu, Zhang Zhiyuan and Lai Ka-ying have carried out a series of hands-on scientific operations. They replaced and cleaned experimental samples, and performed electrode maintenance as well as lens cleaning. In addition, the trio completed gas cylinder replacement and vacuum pumping and exhaust removal.

On the station maintenance front, the crew conducted routine microbial monitoring aboard the space station. They collected and tested samples from cabin air, surfaces, and water systems to assess microbial growth conditions, providing critical data for in-orbit contamination prevention and control.

In terms of health management, the astronauts completed scheduled visual function assessments and non-invasive cardiac function tests, offering valuable reference data for researchers monitoring the long-term health effects of spaceflight. Meanwhile, all the three crew members have maintained regular in-orbit exercise routines and have been using specialized equipment such as bone loss countermeasure devices to mitigate the physiological impacts of microgravity.

Meanwhile, they took a well-deserved break, eating together to replenish energy, relaxing body and mind, shedding the fatigue of intense work, and recharging for the missions ahead.

China launched the Shenzhou-23 crewed spaceship on May 24, 2026. The mission includes a one-year in-orbit study designed to gather data for future long-duration human space missions.

Shenzhou-23 Crew
Zhu Yangzhu 朱杨柱, Commander & Flight Engineer (second spaceflight)
Zhang Zhiyuan 张志远, Pilot (first spaceflight)
Lai Ka-ying/Li Jiaying 黎家盈, Payload Specialist (first spaceflight) [Hong Kong SAR]

Video Credit: CCTV
Duration: 1 minute, 16 seconds
Release Date: Aug. 23, 2026

#NASA #Space #Science #China #中国 #Shenzhou23Mission #神舟二十三号 #Shenzhou23 #Taikonauts #Astronauts #ZhuYangzhu #ZhangZhiyuan #LiJiaying #LaiKaying #ChinaSpaceStation #中国空间站 #TiangongSpaceStation #MicrogravityExperiments #SpaceLaboratory #CMSA #中国载人航天工程办公室 #HumanSpaceflight #STEM #Education #HD #Video

View towards 'The Great Attractor' in Our Local Universe | ESO

View towards 'The Great Attractor' in Our Local Universe | ESO

The Great Attractor is a region of heightened gravitational attraction in the local universe. It lies in the general direction of the Norma Cluster and the Hydra–Centaurus Supercluster, approximately 150–250 million light-years from the Milky Way. Its presence was inferred from the peculiar motions of galaxies that deviate from the motion expected solely from the expansion of the universe. The Great Attractor lies in the direction of the constellations Norma and Triangulum Australe.

The term does not refer to a single galaxy, galaxy cluster, or compact astronomical object. Instead, it describes a broad concentration of matter and an associated minimum in the local gravitational-potential and velocity fields. 

This image covers a field of 0.5° x 0.5° in the Southern constellation of Norma (The Level) and in the direction of the "Great Attractor". This region is at an angular distance of about 7° from the main plane of the Milky Way, i.e. less than 15 times the width of the image shown. In this color composite, the foreground stars in the Milky Way mostly appear as whitish spots (the "crosses" around brighter stars are caused by reflections in the telescope optics). Many background galaxies are also seen. They form a huge cluster (ACO 3627) with a number of bright galaxies near the center — they stand out by their larger size and yellowish color. North is up and East is left.

Five exposures each were made in blue (B-band filter; 5 x 300 sec), red (R-band filter; 5 x 180 sec) and near-infrared (narrow-band filter centered at 816 nm; 5 x 240 sec) light and combined into a false-color composite by using blue, green, and red color for the three images, respectively. A logarithmic intensity scale is used to better show the inner as well as the outer regions of the galaxies in this field.

Learn more about the European Southern Observatory's MPG/ESO 2.2-meter telescope:
https://www.eso.org/public/teles-instr/lasilla/mpg22/


Credit: European Southern Observatory (ESO)
Release Date: Dec. 21, 1999


#NASA #Astronomy #Space #Science #Galaxies #GalaxyClusters #GreatAttractor #Abell3827 #ACO3627 #NormaCluster #HydraCentaurusSupercluster #NormaConstellation #TriangulumAustraleConstellation #Cosmology #Cosmos #Universe #MPGESOTelescope #LaSillaObservatory #Chile #Europe #STEM #Education

Wide-field view: Distant Galaxy Cluster Abell 3827 | Victor Blanco Telescope

Wide-field view: Distant Galaxy Cluster Abell 3827 | Victor Blanco Telescope


This image features Abell 3827, a galaxy cluster, about 222 million light years distant, that offers a wealth of exciting possibilities for study. Looking at this cluster of hundreds of galaxies, it is amazing to recall that until less than 100 years ago, many astronomers thought that the Milky Way was the only galaxy in the Universe. The possibility of other galaxies had been debated previously, but the matter was not truly settled until Edwin Hubble confirmed that the Great Andromeda Nebula was in fact far too distant to be part of the Milky Way. The Great Andromeda Nebula became the Andromeda Galaxy, and astronomers recognized that our Universe was much, much larger than humanity had imagined. We can only imagine how Edwin Hubble—after whom the Hubble Space Telescope was named—would have felt if he had seen this spectacular image of Abell 3827.

Abell 3827 is a rich cluster of galaxies located near the center of the Great Attractor; it is about 222 million light years distant. Although it is both nearby and bright, it is difficult to observe because it is located in the Zone of Avoidance, a region near the plane of the Milky Way. Consequently, the cluster is severely obscured by interstellar dust at optical wavelengths.

This wide-field image was collected as part of the Local Volume Complete Cluster Survey (LoVoCCS), a program investigating 107 nearby galaxy clusters. It took advantage of an astrophysical phenomenon called weak gravitational lensing to measure the mass and matter distributions of these clusters.

Learn about the Víctor M. Blanco Telescope:
https://noirlab.edu/science/programs/ctio/telescopes/victor-blanco-4m-telescope


Credit: CTIO/NOIRLab/NSF/AURA
Release Date:
June 4, 2020

#NASA #Astronomy #Space #Science #Galaxies #GalaxyClusters #Abell3827 #GravitationalLensing #LoVoCCS #IndusConstellation #Cosmos #Universe #VictorBlancoTelescope #CTIO #CerroTololo #Chile #NOIRLab #NSF #AURA #UnitedStates #STEM #Education

Distant Galaxy Cluster Abell 3827: 'Our Giant Universe' | Victor Blanco Telescope

Distant Galaxy Cluster Abell 3827: 'Our Giant Universe' | Victor Blanco Telescope

This image features Abell 3827, a galaxy cluster that offers a wealth of exciting possibilities for study, about 222 million light years distant. Looking at this cluster of hundreds of galaxies, it is amazing to recall that until less than 100 years ago, many astronomers thought that the Milky Way was the only galaxy in the Universe. The possibility of other galaxies had been debated previously, but the matter was not truly settled until Edwin Hubble confirmed that the Great Andromeda Nebula was in fact far too distant to be part of the Milky Way. The Great Andromeda Nebula became the Andromeda Galaxy, and astronomers recognized that our Universe was much, much larger than humanity had imagined. We can only imagine how Edwin Hubble—after whom the Hubble Space Telescope was named—would have felt if he had seen this spectacular image of Abell 3827.

Abell 3827 is a rich cluster of galaxies located near the center of the Great Attractor. Although it is both nearby and bright, it is difficult to observe because it is located in the Zone of Avoidance, a region near the plane of the Milky Way. Consequently, the cluster is severely obscured by interstellar dust at optical wavelengths.

This image was collected as part of the Local Volume Complete Cluster Survey (LoVoCCS). It takes advantage of an astrophysical phenomenon called weak gravitational lensing to measure the mass and matter distributions of these clusters.

Learn about the Víctor M. Blanco Telescope:
https://noirlab.edu/science/programs/ctio/telescopes/victor-blanco-4m-telescope


Credit: CTIO/NOIRLab/NSF/AURA
Release Date: 
June 4, 2020

#NASA #Astronomy #Space #Science #Galaxies #GalaxyClusters #Abell3827 #NormaCluster #ACO3627 #GravitationalLensing #LoVoCCS #IndusConstellation #Cosmos #Universe #VictorBlancoTelescope #CTIO #CerroTololo #Chile #NOIRLab #NSF #AURA #UnitedStates #STEM #Education

Central Region of Distant Galaxy Cluster Abell 3827 | Gemini South Telescope

Central Region of Distant Galaxy Cluster Abell 3827 | Gemini South Telescope

Central region of Abell 3827 as imaged using the Gemini Multi-Object Spectrograph on the Gemini South telescope in Chile. The central supermassive galaxy (ESO 146-IG 005) is clearly visible among its cluster companions as well as the remains of at least four nuclei that are being “digested” by the large galaxy. The central galaxy is thought to be the most massive galaxy in our local universe (out to about 1.5 billion light years). The field of view of this image is approximately 5 x 5 arcminutes and is a color composite made from g-, r- and i-band images combined and processed by Travis Rector (University of Alaska Anchorage).

Abell 3827 is a rich cluster of galaxies located near the center of the Great Attractor; it is about 222 million light years distant. Although it is both nearby and bright, it is difficult to observe because it is located in the Zone of Avoidance, a region near the plane of the Milky Way. Consequently, the cluster is severely obscured by interstellar dust at optical wavelengths.

Gemini South Telescope:
https://noirlab.edu/public/programs/gemini-observatory/gemini-south/


Credit: R. Carrasco et al., International Gemini Observatory/AURA
Release Date: May 12, 2010

#NASA #Astronomy #Space #Science #Galaxies #GalaxyClusters #Abell3827 #NormaCluster #ACO3627 #ESO146IG005 #IndusConstellation #Cosmos #Universe #InternationalGeminiObservatory #GeminiSouthTelescope #GeMS #OpticalAstronomy #GeminiObservatory #CerroPachón #Chile #NOIRLab #AURA #NSF #UnitedStates #STEM #Education

Saturday, August 22, 2026

Thermal Imaging: China Landspace Zhuque-3 Reusable Rocket 1st Stage Landing

Thermal Imaging: China Landspace Zhuque-3 Reusable Rocket 1st Stage Landing

Thermal imaging helps engineers monitor intense heat distribution, evaluate thermal protection systems, and analyze engine plume dynamics. 
🚀China achieved its first recovery of a rocket's first stage on land after launching and recovering part of the Zhuque-3 reusable rocket on Wednesday morning, Aug. 19, 2026. The Landspace Zhuque-3 (ZQ-3) Y2 rocket blasted off at 07:35 (Beijing Time) from the Dongfeng Commercial Space Innovation Pilot Zone in northwest China, placing the Honghu03 satellite into its designated orbit. The flight mission was a complete success.

This mission followed the successful sea-based net recovery of the China Long March-10B rocket's first stage on July 10.

Today marked China's first successful land-based controlled recovery of a rocket's first stage using deployable landing legs, highlighting a major breakthrough in the country's reusable rocket technology.

Approximately 137 seconds after lift-off, the first and second stages separated. The second stage continued its flight and successfully delivered the Honghu 03 satellite, independently developed by Hongqing Technology, into its assigned orbit. At approximately 07:41, the first stage performed a successful soft touchdown at the LandSpace Landing Site#1 in Minqin County, Gansu Province, following the planned trajectory.

The Landspace ZhuQue-3 Y2 reusable launch vehicle achieved full success in orbital insertion and first-stage recovery with the power of its nine TQ-12A engines.

🎉This is China's first successful flight verification of land recovery for the first stage of a reusable launch vehicle, as well as its first successful verification of a landing using deployable landing legs.

The Honghu 03 satellite will trial its unfoldable thermal radiator, sizeable solar panels, electric propulsion system, and a 100-gigabit optical laser link ahead of mass production for connectivity constellations. 

This Landspace mission was the 2nd for the partially reusable Zhuque-3, and LandSpace’s 10th orbital launch attempt in the company’s history. This was also the 59th launch from China in 2026.


Video: Landspace
Duration: 26 seconds
Date: Aug. 19, 2026


#NASA #Space #Satellites #InternetSatellites #Honghu03Satellite #HongqingTechnology #SatelliteConstellations #Earth #China #中国 #LandSpace #蓝箭 #Zhuque3Rocket #ZQ3 #Zhuque3Y2Rocket #ReusableRockets #ThermalImaging #JSLC #InnerMongolia #Gansu #CommercialSpace #STEM #Education #History #HD #Video

Journey to Spiral Galaxy Messier 96 in Leo | Victor Blanco Telescope

Journey to Spiral Galaxy Messier 96 in Leo | Victor Blanco Telescope


Among the nearly four billion objects in the DESI Legacy Imaging Surveys’ map is Messier 96 (NGC 3368), a majestic spiral galaxy nestled in the constellation Leo approximately 35 million light-years from Earth. Spanning 100,000 light-years, slightly larger than our own Milky Way in size, it is the brightest member of the Messier 96 Group, the closest grouping of galaxies to our own Local Group. The Messier 96 data were extracted from the DESI Legacy Survey and captured by the U.S. Department of Energy-fabricated Dark Energy Camera (DECam), a CCD camera affixed to the U.S. National Science Foundation (NSF) Víctor M. Blanco 4-meter Telescope at NSF Cerro Tololo Inter-American Observatory (CTIO), a Program of NSF NOIRLab.

The asymmetrical appearance of Messier 96 hints at its history of gravitational interactions—dark dust trails are distributed unevenly throughout the spiral arms. These appear smeared in certain areas. Alhough it is not obvious in this image, astronomers agree that the bright core is not exactly at the center of the galaxy where they would expect it to be. These distorted spiral patterns and the misplaced central core point to disruption caused by the gravitational pull exerted by other galaxies in the Messier 96 Group that have drifted farther away from this preeminent group member.

Learn about the Víctor M. Blanco Telescope:
https://noirlab.edu/science/programs/ctio/telescopes/victor-blanco-4m-telescope


Credit: DESI Legacy Imaging Surveys/LBNL/DOE & KPNO/CTIO/NOIRLab/NSF/AURA
Image Processing: M. Rodriguez (Gemini Observatory/NSF NOIRLab), J. Miller (Gemini Observatory/NSF NOIRLab), T.A. Rector (University of Alaska Anchorage/NSF NOIRLab) & M. Zamani (NSF NOIRLab)
Motion Graphics: N. Bartmann
Duration: 1 minute
Release Date: Aug. 10, 2026


#NASA #Astronomy #Space #Science #Stars #Galaxies #Messier96 #M96 #NGC3368 #InteractingGalaxies #Messier96Group #LeoConstellation #Cosmos #Universe #VictorBlancoTelescope #DECam #CTIO #CerroTololo #Chile #NOIRLab #NSF #DOE #AURA #UnitedStates #STEM #Education #HD #Video

Close-up: Spiral Galaxy Messier 96 in Leo | Victor Blanco Telescope

Close-up: Spiral Galaxy Messier 96 in Leo | Victor Blanco Telescope

Among the nearly four billion objects in the DESI Legacy Imaging Surveys’ map is Messier 96 (NGC 3368), a majestic spiral galaxy nestled in the constellation Leo approximately 35 million light-years from Earth. Spanning 100,000 light-years, slightly larger than our own Milky Way in size, it is the brightest member of the Messier 96 Group, the closest grouping of galaxies to our own Local Group. The Messier 96 data were extracted from the DESI Legacy Survey and captured by the U.S. Department of Energy-fabricated Dark Energy Camera (DECam), a CCD camera affixed to the U.S. National Science Foundation (NSF) Víctor M. Blanco 4-meter Telescope at NSF Cerro Tololo Inter-American Observatory (CTIO), a Program of NSF NOIRLab.

The asymmetrical appearance of Messier 96 hints at its history of gravitational interactions—dark dust trails are distributed unevenly throughout the spiral arms. These appear smeared in certain areas. Alhough it is not obvious in this image, astronomers agree that the bright core is not exactly at the center of the galaxy where they would expect it to be. These distorted spiral patterns and the misplaced central core point to disruption caused by the gravitational pull exerted by other galaxies in the Messier 96 Group that have drifted farther away from this preeminent group member.

Learn about the Víctor M. Blanco Telescope:
https://noirlab.edu/science/programs/ctio/telescopes/victor-blanco-4m-telescope


Credit: DESI Legacy Imaging Surveys/LBNL/DOE & KPNO/CTIO/NOIRLab/NSF/AURA
Image Processing: M. Rodriguez (Gemini Observatory/NSF NOIRLab), J. Miller (Gemini Observatory/NSF NOIRLab), T.A. Rector (University of Alaska Anchorage/NSF NOIRLab) & M. Zamani (NSF NOIRLab)
Duration: 30 seconds
Release Date: Aug. 10, 2026


#NASA #Astronomy #Space #Science #Stars #Galaxies #Messier96 #M96 #NGC3368 #InteractingGalaxies #Messier96Group #LeoConstellation #Cosmos #Universe #VictorBlancoTelescope #DECam #CTIO #CerroTololo #Chile #NOIRLab #NSF #DOE #AURA #UnitedStates #STEM #Education #HD #Video

Spiral Galaxy Messier 96 in Leo | Victor Blanco Telescope

Spiral Galaxy Messier 96 in Leo | Victor Blanco Telescope

Among the nearly four billion objects in the DESI Legacy Imaging Surveys’ map is Messier 96 (NGC 3368), a majestic spiral galaxy nestled in the constellation Leo approximately 35 million light-years from Earth. Spanning 100,000 light-years, slightly larger than our own Milky Way in size, it is the brightest member of the Messier 96 Group, the closest grouping of galaxies to our own Local Group. The Messier 96 data were extracted from the DESI Legacy Survey and captured by the U.S. Department of Energy-fabricated Dark Energy Camera (DECam), a CCD camera affixed to the U.S. National Science Foundation (NSF) Víctor M. Blanco 4-meter Telescope at NSF Cerro Tololo Inter-American Observatory (CTIO), a Program of NSF NOIRLab.

The asymmetrical appearance of Messier 96 hints at its history of gravitational interactions—dark dust trails are distributed unevenly throughout the spiral arms. These appear smeared in certain areas. Alhough it is not obvious in this image, astronomers agree that the bright core is not exactly at the center of the galaxy where they would expect it to be. These distorted spiral patterns and the misplaced central core point to disruption caused by the gravitational pull exerted by other galaxies in the Messier 96 Group that have drifted farther away from this preeminent group member.

Learn about the Víctor M. Blanco Telescope:
https://noirlab.edu/science/programs/ctio/telescopes/victor-blanco-4m-telescope


Credit: DESI Legacy Imaging Surveys/LBNL/DOE & KPNO/CTIO/NOIRLab/NSF/AURA
Image Processing: M. Rodriguez (Gemini Observatory/NSF NOIRLab), J. Miller (Gemini Observatory/NSF NOIRLab), T.A. Rector (University of Alaska Anchorage/NSF NOIRLab) & M. Zamani (NSF NOIRLab)
Release Date: Aug. 10, 2026


#NASA #Astronomy #Space #Science #Stars #Galaxies #Messier96 #M96 #NGC3368 #InteractingGalaxies #Messier96Group #LeoConstellation #Cosmos #Universe #VictorBlancoTelescope #DECam #CTIO #CerroTololo #Chile #NOIRLab #NSF #DOE #AURA #UnitedStates #STEM #Education

Peering Down Deep into Earth's Green Aurora | International Space Station

Peering Down Deep into Earth's Green Aurora | International Space Station

Expedition 71/72 flight engineer and NASA astronaut Don Pettit: "Orbiting over wavy green auroras! Moments like these are some of the most surreal in spaceflight. What a view!"

Also known as the northern lights (aurora borealis) or southern lights (aurora australis), auroras are colorful, dynamic, and often visually delicate displays of an intricate dance of particles and magnetism between the Sun and Earth called space weather. When energetic particles from space collide with atoms and molecules in the atmosphere, they can cause the colorful glow that we call auroras. Excited by solar energy outflows, oxygen molecules within planet Earth's atmosphere can produce green aurora colors roughly between 60 to 120 miles (100-200 km) altitude.

Learn more about auroras: 
https://science.nasa.gov/sun/auroras/

NASA astronaut Don Pettit returned to Earth on April 19, 2025, concluding a seven-month science mission aboard the International Space Station. Pettit spent 220 days in space, earning him a total of 590 days in space over the course of his four spaceflights. He orbited the Earth 3,520 times, traveling 93.3 million miles in low-Earth orbit.


Expedition 75 Crew
Station Commander: Jessica Meir
Roscosmos (Russia) Flight Engineers:
Andrey Fedyaev,
Anna Kikina, Pyotr Dubrov
European Space Agency Flight Engineer: Sophie Adenot
NASA Flight Engineers: Jack Hathaway, Anil Menon

An international partnership of space agencies provides and operates the elements of the International Space Station (ISS). The principals are the space agencies of the United States, Russia, Europe, Japan, and Canada.


Video Credits: NASA/JSC/D. Pettit
Duration: 24 seconds
Release Date: Aug. 22, 2026

#NASA #Space #Science #ISS #Earth #Aurora #GreenAurora #Astronauts #DonPettit #AstronautVideography #Cosmonauts #Russia #Россия #Roscosmos #Роскосмос #HumanSpaceflight #Expedition75 #InternationalCooperation #UnitedStates #STEM #Education #HD #Video

SpaceX Starship Six-Engine Static Fire Pre-flight Test#14

SpaceX Starship Six-Engine Static Fire Pre-flight Test#14


To prepare for SpaceX's Flight Test#14: "Starship completed a full-duration, 60-second static fire with all six Raptor engines" on Friday, August 21, 2026.

Starship Flight Test#13 Summary:

On Friday, July 24, 2026, at 5:51 p.m. CT, Starship lifted off from Starbase, Texas on its thirteenth flight test. This was the second flight of the Starship and Super Heavy V3 vehicles and the first Starship flight to deploy the next generation Starlink V3 satellites.

The flight test began with Super Heavy igniting all 33 Raptor 3 engines and ascending over the Gulf of America. The successful first-stage ascent was followed by a hot-staging maneuver with Starship’s upper stage igniting its six Raptor engines to continue its flight to space.

Following stage separation, the Super Heavy booster performed a directional flip maneuver. The startup sequence was modified for this flight to be more robust to timing variability in engine startup and flip in the desired direction. This is done to increase overall performance. The booster successfully completed the high thrust portion of the boostback burn with all 33 engines, the first time with a Super Heavy V3, before ending the burn early. It attempted to relight its engines for the landing burn with a subset successfully igniting before experiencing a hard splashdown in the Gulf.

After completing a full-duration ascent burn on all six Raptor engines, Starship achieved its planned velocity and trajectory. Starship then successfully deployed all 20 Starlink V3 satellites. SpaceX engineers were able to successfully communicate with every satellite using radio frequency and laser links and downloaded key telemetry from the satellites. The Starlink satellites were deployed on the pre-planned trajectory and are expected to have demised upon reentry approximately 20 minutes after deployment.

The vehicle also reignited a single Raptor engine in an in-space demonstration of a core capability for future orbital missions.

Starship re-entered the Earth’s atmosphere and was able to gather critical data on the performance of its heatshield before executing a dynamic banking move to mimic the trajectory that future missions returning to Starbase will fly. Starship then guided itself using its four flaps to the pre-planned splashdown zone in the Indian Ocean. After relighting all three Raptor engines, Starship executed a landing flip, landing burn, and soft splashdown, coming to rest intact in the Indian Ocean and providing critical views of an intact heatshield for the first time.

NASA plans to use a lunar lander version of Starship to deliver astronauts and cargo to the Moon during the Artemis IV mission and beyond through the Human Landing System (HLS) Program.


Download the Free Starship User Guide (PDF):
https://www.spacex.com/media/starship_users_guide_v1.pdf

Video Credit: SpaceX
Duration: 1 minute, 18 seconds
Date: Aug. 21, 2026

#NASA #SpaceX #Space #Earth #Mars #Moon #MoonToMars #ArtemisProgram #ArtemisIII #ArtemisIV #Starship #StarshipV3 #FlightTest13 #ReusableSpacecraft #SuperHeavy #SuperHeavyV3 #ElonMusk #Engineering #SpaceTechnology #HumanSpaceflight #CommercialSpace #SpaceExploration #StarbaseTexas #UnitedStates #STEM #Education #HD #Video