Monday, August 03, 2026

Rare Planetary Parade over Kitt Peak National Observatory in Arizona

Rare Planetary Parade over Kitt Peak National Observatory in Arizona

This image captured the planetary parade of Saturn, Neptune, Venus, and Mercury on March 2, 2026. 
Petr Horálek, the photographer, is a NOIRLab Audiovisual Ambassador.

A planetary conjunction occurs when two planets appear close together in the sky along the ecliptic, though they remain millions of miles apart in space. The ecliptic is the apparent path of the Sun across the celestial sphere over the course of a year, forming the plane of Earth's orbit and serving as a key reference in astronomy.


Image Credit: KPNO/NOIRLab/NSF/AURA/P. Horálek (Institute of Physics in Opava)
Release Date: July 22, 2026

#NASA #Astronomy #Space #Science #SolarSystem #Planets #Neptune #Saturn #Venus #Mercury #PlanetaryConjunctions #MilkyWayGalaxy #Cosmos #Universe #KPNO #KittPeakNationalObservatory #Arizona #NOIRLab #NSF #AURA #UnitedStates #Astrophotographers #PetraHorálek #Astrophotography #STEM #Education

Planet Mars: Dust Storm in South Polar Region | Europe's Mars Express Orbiter

Planet Mars: Dust Storm in South Polar Region | Europe's Mars Express Orbiter


Dust storms like this one start close to the ground and are spread by wind as they rise—warming the cold Martian atmosphere. A fleet of orbiting spacecraft monitor Martian dust storms. They serve as lifelines to Earth by relaying data from the rovers and lander on the ground back to science teams. There is evidence of extensive frozen water in Mars' south polar region. This polar region contains enough frozen water to cover the entire planet in a liquid layer approximately 11 meters (36 feet) deep. The Mars Express orbiter's radar instrument has made more than 300 virtual slices through layered deposits covering the pole to map the ice. The radar sees through icy layers to the lower boundary that is as deep as 3.7 kilometers (2.3 miles) below the surface.

"The south polar layered deposits of Mars cover an area bigger than Texas. The amount of water they contain has been estimated before, but never with the level of confidence this radar makes possible," said Jeffrey Plaut of NASA's Jet Propulsion Laboratory, Pasadena California.

The European Space Agency's Mars Express Mission (2003-2026) was launched on June 2, 2003, from Baikonur, Kazakhstan, aboard a Russian Soyuz rocket with a Fregat upper stage. In addition to being Europe’s first mission to Mars, Mars Express is the first fully European mission to any planet. The orbiter has been successfully performing scientific measurements since early 2004, namely, high-resolution imaging and mineralogical mapping of the surface, radar sounding of the subsurface structure down to the permafrost, precise determination of the atmospheric circulation and composition, and study of the interaction of the atmosphere with the interplanetary medium. Due to the valuable science return and the highly flexible mission profile, Mars Express has been granted several mission extensions.

Mission: ESA Mars Express
Orbit: 23290
Date: 2022-06-09T07:59:18.759Z
Instrument: High Resolution Stereo Camera (HRSC)

Image created processing data from: psa.esa.int

Raw Data:
HN290_0009_ND4
HN290_0009_GR4
HN290_0009_BL4

Credits: ESA/DLR/FUBerlin/AndreaLuck CC
Release Date: Aug. 3, 2026


#NASA #ESA #Space #Astronomy #Science #Planet #Mars #SouthPole #DustStorms #WaterIce #Geology #MarsExpress #MarsExpressSpacecraft #MarsOrbiters #HRSC #Europe #DLR #FUBerlin #Berlin #Germany #Deutschland #CitizenScience #AndreaLuck #CitizenScientists #STEM #Education

NASA & SpaceX Advance Wind Tunnel Tests for Starship's Super Heavy Booster V3

NASA & SpaceX Advance Wind Tunnel Tests for Starship's Super Heavy Booster V3

Engineers at NASA Ames conduct transonic and supersonic wind testing on a 1.2% scale model of the Super Heavy Version 3 rocket that will launch the Starship human landing system.
Engineers at NASA Ames conduct transonic and supersonic wind testing on a 1.2% scale model of the Super Heavy Version 3 rocket that will launch the Starship human landing system.
Engineers at NASA Ames conduct transonic and supersonic wind testing on a 1.2% scale model of the Super Heavy Version 3 rocket that will launch the Starship human landing system.
Engineers at NASA Ames conduct transonic and supersonic wind testing on a 1.2% scale model of the Super Heavy Version 3 rocket that will launch the Starship human landing system.

NASA and its industry partners are preparing for next year’s Artemis III demonstration mission by completing new wind tunnel tests on SpaceX’s Super Heavy Version 3 rocket booster. The tests, conducted at NASA’s Ames Research Center in California’s Silicon Valley, focused on better understanding the extreme aerodynamic forces the rocket can experience during re-entry. The recent test series builds on previous testing completed at NASA Ames in 2024.

NASA is working with SpaceX to develop the company’s Starship Human Landing System (HLS) to safely carry astronauts from lunar orbit to the Moon’s surface and back. The upgraded Super Heavy rocket booster is part of SpaceX’s Starship launch system. Version 3 of Starship and Super Heavy is expected to be the basis for the Starship HLS for Artemis III in 2027 and a later crewed lunar landing in 2028.

Although Starship HLS is a lunar lander designed and built by SpaceX, NASA collaborates with commercial companies to provide access to specialized testing facilities, like the wind tunnels at NASA Ames, and technical expertise, such as the team that set up the wind tunnel testing and helped analyze the results.

“NASA has a lot of experience with unsteady aerodynamics,” said Manish Mehta, discipline lead engineer for the HLS Plume and Aero Environments team, NASA’s Marshall Space Flight Center in Huntsville, Alabama. “We used the agency’s broad experience base of conducting wind tunnel tests for the space shuttle, the Space Launch System (SLS) rocket, and Orion spacecraft to efficiently set up and analyze the wind tunnel testing for the Super Heavy Version 3. In fact, similar testing at the Ames Unitary Plan Wind Tunnel resulted in adding strakes to SLS for Artemis II, so what we learned for Artemis II is helping us get to Artemis III and beyond.”

Testing
SpaceX’s Starship consists of a 33-engine first-stage Super Heavy rocket, or booster, and the second-stage Starship. Version 3 of Super Heavy incorporates many new and upgraded systems, including:
1) New propulsion systems and new Raptor 3 rocket engines
2) No engine section skirt, individual engine shrouds, or integrated large-scale base heat shield
3) Three gridfins on the Super Heavy booster instead of four, with each fin now 50% larger
4) An integrated hot stage replacing the previous single-use protective interstage

With significant changes to Super Heavy, NASA and SpaceX engineers wanted more information about the steady and unsteady aerodynamic forces the rocket will experience during atmospheric re-entry as it returns to the launch site for refurbishment and re-use.

“When a rocket, or an airplane, flies through air at high speed, it’s subjected to steady aerodynamic forces and moments, and unsteady aerodynamic forces and moments,” explained Jayanta Panda, unsteady aerodynamics subject matter expert at NASA Ames and part of the Human Landing System Plume and Aero Environments team. “An example of a steady aerodynamic force would be when air smoothly flows over the surface of the rocket as it ascends. An unsteady aerodynamic force would be air ‘buffeting,’ or hitting, certain areas the rocket at less predictable times and potentially causing vibrations.”

Wind Tunnels
NASA and SpaceX used a 1.2% scale model of the Super Heavy Version 3 in the transonic wind tunnel and the supersonic wind tunnel at NASA Ames for testing. The transonic tunnel blasts scale models of rockets or aircraft with air at speeds ranging from Mach 0.2 to Mach 1.4 (Mach 1 is the speed of sound, or about 761 miles per hour). The smaller supersonic tunnel fires winds at higher speeds, from Mach 1.55 to Mach 2.5. The wind tunnel tests on Super Heavy Version 3, conducted in late 2025, used both tunnels to measure steady and unsteady air flows on the surfaces of Super Heavy. 

“Resulting wind tunnel data on steady forces and moments helps predict how the rocket will react to forces in the atmosphere during re-entry so the flight software can effectively guide the rocket during flight,” Mehta said. “The unsteady pressure data helps engineers understand the environment around the rocket as it re-enters Earth’s atmosphere. Engineers use that information as one input into software that analyzes loads on the rocket.”

Through the Artemis program, NASA is returning humans to the Moon for scientific discovery, economic opportunity, to establish an enduring human presence on the lunar surface, and build the foundation for the first crewed missions to Mars—for the benefit of all.

To learn more about Artemis, visit: https://www.nasa.gov/artemis


Image Credit: NASA/Brandon Torres
Release Date: July 31, 2026

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

A Memorable Aurora Australis | International Space Station

A Memorable Aurora Australis | International Space Station

Expedition 75 flight engineer and NASA astronaut Anil Menon: "I’ll never forget this sight. Tonight I saw my first aurora from space. Luckily, there is a video to help remember and captured it perfectly.  The KP index was over 5 tonight because of a solar event and the sky over Australia lit up and the green snaked across the atmosphere.  I was filled with awe and gratitude. It’s a beautiful planet we share."

This is Anil Menon's first spaceflight mission after he was selected as part of NASA’s 2021 astronaut class.

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.

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


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.


Credit: NASA's Johnson Space Center/A. Menon
Duration: 35 seconds
Date: Aug. 2, 2026


#NASA #Space #Science #ISS #Planets #Earth #Aurora #AuroraAustralis #Australia #Astronauts #AnilMenon #AstronautPhotography #Cosmonauts #Russia #Россия #Roscosmos #Роскосмос #HumanSpaceflight #Expedition75 #InternationalCooperation #UnitedStates #STEM #Education #HD #Video

Sunday, August 02, 2026

Planet Earth: Pacific Ocean view | International Space Station

Planet Earth: Pacific Ocean view | International Space Station

Expedition 75 flight engineer and NASA astronaut Anil Menon: "The Pacific Ocean this morning from the cupola . . ."

This is Anil Menon's first spaceflight mission after he was selected as part of NASA’s 2021 astronaut class. Among the hundreds of experiments planned during his mission, he will participate in studies to better understand astronaut vein structure, blood flow, and blood composition in microgravity. He also will test producing intravenous fluids using the space station’s potable water.

NASA astronaut Anil Menon's Official Biography:
https://www.nasa.gov/people/nasa-astronaut-anil-menon/

The Cupola is a panoramic control tower for the International Space Station, a dome-shaped module with windows where operations on the outside of the station can be observed and guided. It is a pressurized observation and work area that accommodates command and control workstations and other hardware.


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.


Credit: NASA's Johnson Space Center/A. Menon
Date: Aug. 2, 2026


#NASA #Space #Science #ISS #Planets #Earth #Atmospheres #PacificOcean #Weather #Meteorology #Storms #Typhoons #Astronauts #AnilMenon #AstronautPhotography #Cosmonauts #Russia #Россия #Roscosmos #Роскосмос #HumanSpaceflight #Expedition75 #InternationalCooperation #UnitedStates #STEM #Education

NASA Astronaut Deniz Burnham: Training in Russia for International Space Station

NASA Astronaut Deniz Burnham: Training in Russia for International Space Station


NASA astronaut Deniz Burnham: "It’s been an incredible experience serving as part of the backup crew for Soyuz MS-29 over the past year! This short clip captures just a glimpse of the training and teamwork that have shaped this journey. I’m grateful for the opportunity to represent NASA as a crewmember on Soyuz MS-30 and Expedition 76 on the ISS! Can’t wait to share more of my training experiences as we continue the countdown to launch.🚀"

NASA astronaut Deniz Burnham will embark on her first mission to the International Space Station, serving as an Expedition 76 flight engineer. Burnham will launch aboard the Roscosmos Soyuz MS-30 spacecraft with cosmonauts Dmitri Petelin and Konstantin Borisov of Russia. Launch is targeted for March 2027, from the Baikonur Cosmodrome in Kazakhstan, and the trio will spend about seven months aboard the orbiting laboratory.

During her expedition, Burnham will conduct scientific investigations and technology demonstrations to help prepare humans for future exploration missions to the Moon and Mars and to help benefit people on Earth.

Selected as a NASA astronaut in 2021, Burnham graduated with the agency’s 23rd astronaut class in 2024. Born at Incirlik Air Base in Adana, Turkey, Burnham moved frequently while growing up in a military family. She was living in Wasilla, Alaska, at the time of her selection.

A former intern at NASA’s Ames Research Center in California’s Silicon Valley, Burnham earned a bachelor’s degree in chemical engineering from the University of California, San Diego, and a master’s degree in mechanical engineering from the University of Southern California in Los Angeles. An experienced leader in the energy industry, she spent more than a decade managing onsite drilling operations on oil rigs across North America. Burnham also served in the U.S. Navy Reserves as an engineering duty officer. She is a licensed private pilot with ratings for airplane single engine land and sea, instrument airplane, and rotorcraft-helicopter.

NASA Astronaut Deniz Burnham's Biography
https://www.nasa.gov/people/nasa-astronaut-deniz-burnham/

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.

"For more than 25 years, people have lived and worked continuously aboard the International Space Station, advancing scientific knowledge and making research breakthroughs not possible on Earth. The space station helps NASA understand and overcome the challenges of human spaceflight, expand commercial opportunities in low Earth orbit, and build on the foundation for long-duration missions to the Moon, as part of the Artemis program, and to Mars."

To learn more about International Space Station research, operations, and its crews, visit:
https://www.nasa.gov/station

Video Credit: Roscosmos/D. Burnham
Duration: 32 seconds
Release Date: July 30, 2026

#NASA #Space #Science #ISS #Earth #SoyuzMS30 #CrewSpacecraft #Kazakhstan #Astronauts #DenizBurnham #MechanicalEngineers #Engineers #Pilots #Cosmonauts #DmitriPetelin #KonstantinBorisov #Russia #Россия #Roscosmos #Роскосмос #HumanSpaceflight #Expedition76 #InternationalCooperation #NASAJohnson #JSC #Texas #UnitedStates #STEM #Education #HD #Video

NASA Astronaut Deniz Burnham: First International Space Station Mission via Russia

NASA Astronaut Deniz Burnham: First International Space Station Mission via Russia

NASA astronaut Deniz Burnham portrait
NASA astronaut Deniz Burnham portrait
NASA astronaut Deniz Burnham portrait
NASA astronaut Deniz Burnham portrait
NASA astronaut candidate Deniz Burnham poses for a photograph in front of NASA’s Artemis I Space Launch System and Orion spacecraft atop the mobile launcher on the pad at Launch Complex 39B at the agency’s Kennedy Space Center in Florida on Sept. 2, 2022. 
NASA Artemis Underway Recovery Tests
NASA astronaut Deniz Burnham is seen as she prepares to take part in practicing Artemis recovery procedures during Underway Recovery Test-12 onboard USS Somerset off the coast of California, Friday, March 28, 2025.
NASA Artemis Underway Recovery Tests
NASA astronaut Deniz Burnham is seen as she prepares to take part in practicing Artemis recovery procedures during Underway Recovery Test-12 onboard USS Somerset off the coast of California, Friday, March 28, 2025.
NASA announced that Deniz Burnham would join its 2021 astronaut candidate class on Dec. 6, 2021.

NASA astronaut Deniz Burnham will embark on her first mission to the International Space Station, serving as an Expedition 76 flight engineer. Burnham will launch aboard the Roscosmos Soyuz MS-30 spacecraft with cosmonauts Dmitri Petelin and Konstantin Borisov of Russia. Launch is targeted for March 2027, from the Baikonur Cosmodrome in Kazakhstan, and the trio will spend about seven months aboard the orbiting laboratory.

During her expedition, Burnham will conduct scientific investigations and technology demonstrations to help prepare humans for future exploration missions to the Moon and Mars and to help benefit people on Earth.

Selected as a NASA astronaut in 2021, Burnham graduated with the agency’s 23rd astronaut class in 2024. Born at Incirlik Air Base in Adana, Turkey, Burnham moved frequently while growing up in a military family. She was living in Wasilla, Alaska, at the time of her selection.

A former intern at NASA’s Ames Research Center in California’s Silicon Valley, Burnham earned a bachelor’s degree in chemical engineering from the University of California, San Diego, and a master’s degree in mechanical engineering from the University of Southern California in Los Angeles. An experienced leader in the energy industry, she spent more than a decade managing onsite drilling operations on oil rigs across North America. Burnham also served in the U.S. Navy Reserves as an engineering duty officer. She is a licensed private pilot with ratings for airplane single engine land and sea, instrument airplane, and rotorcraft-helicopter.

NASA Astronaut Deniz Burnham's Biography
https://www.nasa.gov/people/nasa-astronaut-deniz-burnham/

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.

"For more than 25 years, people have lived and worked continuously aboard the International Space Station, advancing scientific knowledge and making research breakthroughs not possible on Earth. The space station helps NASA understand and overcome the challenges of human spaceflight, expand commercial opportunities in low Earth orbit, and build on the foundation for long-duration missions to the Moon, as part of the Artemis program, and to Mars."

To learn more about International Space Station research, operations, and its crews, visit:
https://www.nasa.gov/station


Credit: NASA/Robert Markowitz
Release Date: July 30, 2026

#NASA #Space #Science #ISS #Earth #SoyuzMS30 #CrewSpacecraft #Kazakhstan #Astronauts #DenizBurnham #MechanicalEngineers #Engineers #Pilots #Cosmonauts #DmitriPetelin #KonstantinBorisov #Russia #Россия #Roscosmos #Роскосмос #HumanSpaceflight #Expedition76 #InternationalCooperation #NASAJohnson #JSC #Texas #UnitedStates #STEM #Education

Noctilucent Clouds over The Bering Sea & Central Alaska | Earth Science

Noctilucent Clouds over The Bering Sea & Central Alaska | Earth Science



Astrophotographer Jared Aicher: "The evening sky over the Bering Sea and central Alaska was completely veiled by noctilucent clouds last night. The view from the flight deck lasted for a couple of hours as the sunset slowly turned to sunrise with nightfall never actually arriving at 63 degrees north latitude."

At high latitudes in the summer months, iridescent clouds form in a part of the atmosphere roughly 50 to 86 kilometers (30 to 54 miles) above the surface of our planet. Their high altitude allows them to reflect sunlight after the Sun has set. These are called noctilucent or polar mesospheric clouds.

Noctilucent clouds (NLCs), or night shining clouds are tenuous cloud-like phenomena in the upper atmosphere. They consist of ice crystals and from the ground are only visible during astronomical twilight. Noctilucent roughly means "night shining" in Latin. They are most often observed during the summer months from latitudes between ±50° and ±70°. Too faint to be seen in daylight, they are visible only when the observer and the lower layers of the atmosphere are in Earth's shadow while these very high clouds are still in sunlight. Recent studies suggest that increased atmospheric methane emissions produce additional water vapor through chemical reactions once the methane molecules reach the mesosphere—creating, or reinforcing existing, noctilucent clouds.

The Bering Sea is a marginal sea of the Northern Pacific Ocean. It forms, along with the Bering Strait, the divide between the two largest landmasses on Earth: Eurasia and the Americas. It comprises a deep water basin that then rises through a narrow slope into the shallower water above the continental shelves. The Bering Sea is named after Vitus Bering, a Danish-born Russian navigator, that in 1728, was the first European to systematically explore it, sailing from the Pacific Ocean northward to the Arctic Ocean.

Alaska is a non-contiguous U.S. state on the northwest extremity of North America. Part of the Western United States region, it is one of the two non-contiguous U.S. states, alongside Hawaii. Alaska is considered to be the northernmost, westernmost, and easternmost state in the United States. It borders the Canadian territory of the Yukon and the province of British Columbia to the east. It shares a western maritime border in the Bering Strait with Russia. The Chukchi and Beaufort Seas of the Arctic Ocean lie to the north, and the Pacific Ocean lies to the south.


Image Credit: Jared Aicher
Date: July 30, 2026

#NASA #Space #Science #Sun #Planets #Earth #Weather #Meteorology #Atmosphere #WaterVapor #Clouds #IceCrystals #NoctilucentClouds #PolarMesosphericClouds #Astrophotography #Astrophotographers #JaredAicher #CitizenScience #BeringSea #PacificOcean #Alaska #UnitedStates #STEM #Education

A Fire Rainbow over West Virginia | Earth Science

A Fire Rainbow over West Virginia | Earth Science

What's happening to this cloud? 

Ice crystals in a distant cirrus cloud are acting like little floating prisms. Known informally as a fire rainbow for its flame-like appearance, a circumhorizon arc appears parallel to the horizon. For a circumhorizontal arc to be visible, the Sun must be at least 58 degrees high in a sky where cirrus clouds present below—in this case cirrus fibratus. The numerous, flat, hexagonal ice-crystals that compose the cirrus cloud must be aligned horizontally to properly refract sunlight in a collectively similar manner. Therefore, circumhorizontal arcs are somewhat unusual to see. The featured fire rainbow was photographed in 2021 near North Fork Mountain in West Virginia, USA.

West Virginia is a mountainous, landlocked state in the Southern and Mid-Atlantic regions of the United States. It is bordered by Pennsylvania and Maryland to the northeast, Virginia to the southeast, Kentucky to the southwest, and Ohio to the northwest. 


Image Credit & Copyright: Christa Harbig
Location: North Fork Mountain, West Virginia, United States
Christa's website: 

#NASA #Science #Stars #Sun #SolarSystem #Planets #Earth #EarthScience #PlanetaryAtmospheres #CirrusClouds #CirrusFibratus #Sunlight #WaterDroplets #WaterIceCrystals #CircumhorizontalArcs #WestVirginia #UnitedStates #Photography #ChristaHarbig #Photographers #NASAGoddard #GSFC #STEM #Education #APoD

Shenzhou-23 Crew Advances Multi-generational Rice Cultivation | China Space Station

Shenzhou-23 Crew Advances Multi-generational Rice Cultivation | China Space Station

More than two months after arriving at China's Tiangong Space Station, the three astronauts of the Shenzhou-23 spaceflight mission—Zhu Yangzhu, Zhang Zhiyuan, and Lai Ka-ying—are all in good condition and have made steady progress on multiple space science experiments, including a groundbreaking study on multi-generational rice cultivation in microgravity.

Launched on May 24, the Shenzhou-23 spacecraft carried rice seeds and other experimental materials to the Tiangong Space Station.

After over two months of careful cultivation, the crew successfully harvested the first batch of rice samples.

The experiment aims to achieve the first-ever continuous cultivation of two generations of rice in orbit, completing two full life cycles "from seed to seed to seed," to study how long-term microgravity affects the molecular mechanisms and genetic stability of rice.

In the field of space medicine, the crew used ultrasound diagnostic equipment to conduct bilateral carotid, radial, and dorsalis pedis artery ultrasound examinations. The collected data will support research projects including pan-vascular hemodynamic profiling and spatiotemporal evolution mapping of blood flow.

The astronauts also carried out experiments related to light environment factors, adjusting and intervening in the cabin's lighting conditions and conducting performance tests before and after modifications to investigate how light environments in special space settings affect human psychological perception and work efficiency.

Last week, the crew completed emergency rescue training in orbit as scheduled, conducting emergency evacuation drills under simulated fire conditions to reinforce their emergency response and fault handling capabilities.

For health management, the crew completed multiple medical examinations including electrocardiography, vision tests, intraocular pressure measurements, and fundus examinations.

They used a "space body mass measuring device" to measure body mass in orbit, comprehensively monitoring physiological changes in microgravity.

The astronauts also actively engaged in physical exercise using space treadmills and other equipment.

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, 34 seconds
Release Date: Aug. 2, 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

Saturday, August 01, 2026

Interstellar Comet 3I/ATLAS | Vera C. Rubin Observatory—LSST Camera

Interstellar Comet 3I/ATLAS | Vera C. Rubin ObservatoryLSST Camera

The faint coma and tail glow of comet 3I/ATLAS were captured by the National Science Foundation–Department of Energy Vera C. Rubin Observatory, jointly funded by the U.S. National Science Foundation (NSF) and the U.S. Department of Energy's Office of Science (DOE/SC), on December 19, 2025. Comet 3I/ATLAS is only the third known visitor from another star system to pass through our Solar System. The comet reappeared from behind the Sun in November 2025 after spending several weeks out of view from Earth. By the time of this observation, the object was at its closest point to Earth on its outward journey toward interstellar space. Rubin incidentally imaged this object months earlier during testing activities, before it was identified as an interstellar comet.

What makes this NOIRLab image special is the amount of detail captured in a single 30-second exposure. Usually, revealing the faint glow of a comet’s tail requires a much longer exposure—one that would show the background stars and galaxies as blurry streaks. However, Rubin’s light-collecting power and highly sensitive LSST Camera capture the comet’s delicate tail in just 30 seconds while keeping the distant background objects crisp and clear.

Objects like 3I/ATLAS are rare and scientifically valuable. Unlike the common comets and asteroids that formed alongside our Sun, interstellar objects were formed in other planetary systems. At a point in their distant past, they were ejected from their home systems by gravitational interactions. After being cast out, these objects travel through interstellar space, occasionally passing through another planetary system like our own. When they appear in our neighborhood, they give scientists a rare opportunity to study material formed around other stars—assuming we can catch a glimpse of them while they are close by.

This is where the Rubin Observatory shines. Unlike telescopes that focus on individual targets or small regions of space, Rubin is a survey telescope that repeatedly scans large portions of the sky. With its extremely wide field of view and ability to detect very faint light sources, Rubin catches dim, moving objects that might otherwise go unnoticed. Additionally, Rubin sends out an alert for every change it detects, so scientists can be on the lookout for unusual objects moving through our Solar System. 

With Rubin data, researchers expect to discover many more interstellar visitors passing through our neighborhood, each carrying clues about the processes that shape planets and small bodies around other stars. Studying these objects in greater numbers will help scientists better understand how planetary systems, including our own, form and evolve.

Learn more about the new Vera Rubin Observatory:

The LSST Camera (LSSTCam)

An Introduction to Vera Rubin:

Credits:
NSF–DOE Vera C. Rubin Observatory/NOIRLab/SLAC/AURA
Acknowledgement: C. O. Chandler (University of Washington)
Image Date: Dec. 19, 2025
Release Date: July 15, 2026

#NASA #Astronomy #Space #Science #InterstellarObjects #InterplanetaryBodies #InterstellarComets #InterstellarComet3I #Comet3I #Comet3IATLAS #StarSystems #SolarSystem #MilkyWayGalaxy #Universe #LSSTCam #SimonyiSurveyTelescope #RubinObservatory #VeraRubin #CerroPachón #Chile #NOIRLab #NSF #DOE #AURA #UnitedStates #Chile #Europe #STEM #Education 

Highlights of The COSMOS Field | Vera C. Rubin Observatory—LSST Camera

Highlights of The COSMOS Field | Vera C. Rubin ObservatoryLSST Camera

This exceptionally deep image from NSF–DOE Vera C. Rubin Observatory reveals the renowned COSMOS field and its surroundings in the constellation Sextans. The view is crowded with galaxies and galaxy clusters spanning an immense range of distances and cosmic ages, while only a handful of foreground stars belong to our own Milky Way. It was created by combining multiple observations from Rubin’s LSST Camera into a deep coadded image and is being released to mark Early Data Preview 2, the first Rubin data preview based on LSST Camera observations.

Packed into this single image from Rubin Observatory are many kinds of galaxies: spirals with delicate arms, smooth elliptical galaxies, distorted merging galaxies, and faint red galaxies from the distant Universe. Only a relatively small number of bright stars from our own Milky Way appear in the foreground, leaving an unusually clear view of galaxies stretching far into the distance.

This image was captured with Rubin’s 3.2-gigapixel LSST Camera—the largest digital camera in the world, mounted on the 8.4-meter Simonyi Survey Telescope. It was created by stacking hundreds of individual observations and contains more than half a million galaxies and more than 50,000 stars.

The COSMOS field was selected more than two decades ago to provide astronomers with a relatively unobstructed window into the distant Universe. Located away from the crowded plane of the Milky Way, it contains comparatively few bright stars and little intervening dust, and it is accessible to major observatories on Earth and in space. Even in this exceptionally clear region, Rubin’s remarkable sensitivity reveals traces of faint, glowing galactic cirrus: wisps of interstellar dust within our own Milky Way superimposed on the much more distant cosmic landscape.

Early Data Preview 2 comes on the heels of the beginning of the Legacy Survey of Space and Time (LSST). With its ability to observe the southern sky deeply, widely, and repeatedly, Rubin Observatory is poised to transform many areas of astronomy.

Learn more about the new Vera Rubin Observatory:

The LSST Camera (LSSTCam)

An Introduction to Vera Rubin:

Credit: NSF–DOE Vera C. Rubin Observatory/NOIRLab/SLAC/AURA
Release Date: July 31, 2026

#NASA #Astronomy #Space #Science #Stars #Galaxies #GalaxyClusters #CosmosField #SextansConstellation #Cosmos #Universe #LSSTCam #SimonyiSurveyTelescope #RubinObservatory #VeraRubin #CerroPachón #Chile #NOIRLab #NSF #DOE #AURA #UnitedStates #STEM #Education

A Journey Deep into The COSMOS Field | Vera C. Rubin Observatory

A Journey Deep into The COSMOS Field | Vera C. Rubin Observatory


This exceptionally deep image from NSF–DOE Vera C. Rubin Observatory reveals the renowned COSMOS field and its surroundings in the constellation Sextans. The view is crowded with galaxies and galaxy clusters spanning an immense range of distances and cosmic ages, while only a handful of foreground stars belong to our own Milky Way. It was created by combining multiple observations from Rubin’s LSST Camera into a deep coadded image and is being released to mark Early Data Preview 2, the first Rubin data preview based on LSST Camera observations.

Packed into this single image from Rubin Observatory are many kinds of galaxies: spirals with delicate arms, smooth elliptical galaxies, distorted merging galaxies, and faint red galaxies from the distant Universe. Only a relatively small number of bright stars from our own Milky Way appear in the foreground, leaving an unusually clear view of galaxies stretching far into the distance.

This image was captured with Rubin’s 3.2-gigapixel LSST Camera—the largest digital camera in the world, mounted on the 8.4-meter Simonyi Survey Telescope. It was created by stacking hundreds of individual observations and contains more than half a million galaxies and more than 50,000 stars.

The COSMOS field was selected more than two decades ago to provide astronomers with a relatively unobstructed window into the distant Universe. Located away from the crowded plane of the Milky Way, it contains comparatively few bright stars and little intervening dust, and it is accessible to major observatories on Earth and in space. Even in this exceptionally clear region, Rubin’s remarkable sensitivity reveals traces of faint, glowing galactic cirrus: wisps of interstellar dust within our own Milky Way superimposed on the much more distant cosmic landscape.

Early Data Preview 2 comes on the heels of the beginning of the Legacy Survey of Space and Time (LSST). With its ability to observe the southern sky deeply, widely, and repeatedly, Rubin Observatory is poised to transform many areas of astronomy.

Learn more about the new Vera Rubin Observatory:

The LSST Camera (LSSTCam)

An Introduction to Vera Rubin:

Credit: NSF–DOE Vera C. Rubin Observatory/NOIRLab/SLAC/AURA
Duration: 1 minute
Release Date: July 31, 2026

#NASA #Astronomy #Space #Science #Stars #Galaxies #GalaxyClusters #CosmosField #SextansConstellation #Cosmos #Universe #LSSTCam #SimonyiSurveyTelescope #RubinObservatory #VeraRubin #CerroPachón #Chile #NOIRLab #NSF #DOE #AURA #UnitedStates #STEM #Education #HD #Video

Close-up Looks Deep into The COSMOS Field | Vera C. Rubin Observatory

Close-up Looks Deep into The COSMOS Field | Vera C. Rubin Observatory

This exceptionally deep image from NSF–DOE Vera C. Rubin Observatory reveals the renowned COSMOS field and its surroundings in the constellation Sextans. The view is crowded with galaxies and galaxy clusters spanning an immense range of distances and cosmic ages, while only a handful of foreground stars belong to our own Milky Way. It was created by combining multiple observations from Rubin’s LSST Camera into a deep coadded image and is being released to mark Early Data Preview 2, the first Rubin data preview based on LSST Camera observations.

Packed into this single image from Rubin Observatory are many kinds of galaxies: spirals with delicate arms, smooth elliptical galaxies, distorted merging galaxies, and faint red galaxies from the distant Universe. Only a relatively small number of bright stars from our own Milky Way appear in the foreground, leaving an unusually clear view of galaxies stretching far into the distance.

This image was captured with Rubin’s 3.2-gigapixel LSST Camera—the largest digital camera in the world, mounted on the 8.4-meter Simonyi Survey Telescope. It was created by stacking hundreds of individual observations and contains more than half a million galaxies and more than 50,000 stars.

The COSMOS field was selected more than two decades ago to provide astronomers with a relatively unobstructed window into the distant Universe. Located away from the crowded plane of the Milky Way, it contains comparatively few bright stars and little intervening dust, and it is accessible to major observatories on Earth and in space. Even in this exceptionally clear region, Rubin’s remarkable sensitivity reveals traces of faint, glowing galactic cirrus: wisps of interstellar dust within our own Milky Way superimposed on the much more distant cosmic landscape.

Early Data Preview 2 comes on the heels of the beginning of the Legacy Survey of Space and Time (LSST). With its ability to observe the southern sky deeply, widely, and repeatedly, Rubin Observatory is poised to transform many areas of astronomy.

Learn more about the new Vera Rubin Observatory:

The LSST Camera (LSSTCam)

An Introduction to Vera Rubin:

Credit: NSF–DOE Vera C. Rubin Observatory/NOIRLab/SLAC/AURA
Duration: 52 seconds
Release Date: July 31, 2026

#NASA #Astronomy #Space #Science #Stars #Galaxies #GalaxyClusters #CosmosField #SextansConstellation #Cosmos #Universe #LSSTCam #SimonyiSurveyTelescope #RubinObservatory #VeraRubin #CerroPachón #Chile #NOIRLab #NSF #DOE #AURA #UnitedStates #STEM #Education #HD #Video

Looking Deep into The COSMOS Field | Vera C. Rubin Observatory

Looking Deep into The COSMOS Field | Vera C. Rubin Observatory

This exceptionally deep image from NSF–DOE Vera C. Rubin Observatory reveals the renowned COSMOS field and its surroundings in the constellation Sextans. The view is crowded with galaxies and galaxy clusters spanning an immense range of distances and cosmic ages, while only a handful of foreground stars belong to our own Milky Way. It was created by combining multiple observations from Rubin’s LSST Camera into a deep coadded image and is being released to mark Early Data Preview 2, the first Rubin data preview based on LSST Camera observations.

Packed into this single image from Rubin Observatory are many kinds of galaxies: spirals with delicate arms, smooth elliptical galaxies, distorted merging galaxies, and faint red galaxies from the distant Universe. Only a relatively small number of bright stars from our own Milky Way appear in the foreground, leaving an unusually clear view of galaxies stretching far into the distance.

This image was captured with Rubin’s 3.2-gigapixel LSST Camera—the largest digital camera in the world, mounted on the 8.4-meter Simonyi Survey Telescope. It was created by stacking hundreds of individual observations and contains more than half a million galaxies and more than 50,000 stars.

The COSMOS field was selected more than two decades ago to provide astronomers with a relatively unobstructed window into the distant Universe. Located away from the crowded plane of the Milky Way, it contains comparatively few bright stars and little intervening dust, and it is accessible to major observatories on Earth and in space. Even in this exceptionally clear region, Rubin’s remarkable sensitivity reveals traces of faint, glowing galactic cirrus: wisps of interstellar dust within our own Milky Way superimposed on the much more distant cosmic landscape.

Early Data Preview 2 comes on the heels of the beginning of the Legacy Survey of Space and Time (LSST). With its ability to observe the southern sky deeply, widely, and repeatedly, Rubin Observatory is poised to transform many areas of astronomy.

Learn more about the new Vera Rubin Observatory:

The LSST Camera (LSSTCam)

An Introduction to Vera Rubin:

Credit: NSF–DOE Vera C. Rubin Observatory/NOIRLab/SLAC/AURA
Release Date: July 31, 2026

#NASA #Astronomy #Space #Science #Stars #Galaxies #GalaxyClusters #CosmosField #SextansConstellation #Cosmos #Universe #LSSTCam #SimonyiSurveyTelescope #RubinObservatory #VeraRubin #CerroPachón #Chile #NOIRLab #NSF #DOE #AURA #UnitedStates #STEM #Education

Friday, July 31, 2026

Milky Way Galaxy Dreams | International Space Station

Milky Way Galaxy Dreams | International Space Station

Expedition 71/72 flight engineer and NASA astronaut Don Pettit: "I finally have all 1.2 million raw image files from my latest mission to ISS! Here is a sample of one of my favorite Milky Way photos, taken from the Cupola with Nikon Z9, Arri Zeiss 15mm lens, T1.8 with custom sidereal drive that cancelled out star motion relative to our orbit."

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.


Image Credits: NASA/JSC/D. Pettit
Release Date: July 31, 2026


#NASA #Space #Science #ISS #Earth #Galaxies #MilkyWay #Astronauts #DonPettit #AstronautPhotography #Cosmonauts #Russia #Россия #Roscosmos #Роскосмос #HumanSpaceflight #Expedition75 #InternationalCooperation #UnitedStates #STEM #Education