Tuesday, June 02, 2026

Close-up: A Side-On Spiral Galaxy—UGC 11537 in Aquila | Hubble

Close-up: A Side-On Spiral GalaxyUGC 11537 in Aquila | Hubble

This astronomical portrait from the NASA/European Space Agency Hubble Space Telescope showcases an edge-on view of the majestic spiral galaxy UGC 11537. Hubble’s Wide Field Camera 3 has captured the tightly wound spiral arms swirling around the heart of UGC 11537 at infrared and visible wavelengths, showing both the bright bands of stars and the dark clouds of dust threading throughout the galaxy. 

UGC 11537 is 230 million light-years away in the constellation Aquila, and lies close to the plane of the Milky Way. Being so close to the starry band of the Milky Way means that foreground stars from our own galaxy have crept into the image—the two prominent stars in front of UGC 11537 are interlopers from within the Milky Way. These bright foreground stars are surrounded by diffraction spikes—imaging artifacts caused by starlight interacting with Hubble’s inner structure. 

This image came from a set of observations designed to help astronomers weigh supermassive black holes in distant galaxies. The combination of Hubble’s sharp-eyed observations and data from ground-based telescopes allowed astronomers to make detailed models of the mass of stars in these galaxies. This in turn helps constrain the mass of supermassive black holes.


Credit: ESA/Hubble & NASA, A. Seth
Duration: 30 seconds
Release Date: Nov. 15, 2021

#NASA #ESA #Hubble #Astronomy #Space #Science #Galaxies #UGC11537 #GalaxyClusters #SpiralGalaxies #BlackHoles #AGNs #AquilaConstellation #Cosmos #Universe #HST #HubbleSpaceTelescope #WFC3 #GSFC #STScI #UnitedStates #Europe #STEM #Education #HD #Video

Europe-China SMILE Solar Science Mission: From cleanroom to space | ESA

Europe-China SMILE Solar Science Mission: From cleanroom to space | ESA

SMILE successfully launched from Europe’s Spaceport in French Guiana on May 19, 2026.

This timelapse captures the excitement and precision of launch operations as the spacecraft begins its journey to study the connection between the Sun and Earth.

The Solar wind Magnetosphere Ionosphere Link Explorer (SMILE) is an international space science mission designed to investigate how the solar wind interacts with Earth's magnetosphere. By observing these dynamic processes from space, SMILE will help scientists better understand space weather and its effects on our planet's magnetic environment.

The European Space Agency (ESA) was responsible for providing SMILE’s payload module (carrying three of the four science instruments), one of the spacecraft’s four science instruments (the soft X-ray imager, SXI), the launcher, and the Assembly Integration and Testing facilities and services. ESA contributed to a second science instrument (the ultraviolet imager, UVI) and the mission operations once SMILE is in orbit.

The Chinese Academy of Sciences provided the other three science instruments and the spacecraft platform, and is responsible for operating the spacecraft in orbit.


Credit: European Space Agency (ESA)
Duration: 3 minutes, 31 seconds
Release Date: June 1, 2026

#NASA #Space #Astronomy #Science #Stars #Sun #Earth #SpaceWeather #MagneticField #Magnetosphere #Europe #China #中国 #CAS #中国科学院 #SMILEMission #Heliophysics #Physics #VegaCRocket #GuianaSpaceCentre #KourouSpaceport #FrenchGuiana #Avio #ArianeGroup #STEM #Education #HD #Video

Monday, June 01, 2026

A Side-On Spiral Galaxy: UGC 11537 in Aquila | Hubble Space Telescope

A Side-On Spiral Galaxy: UGC 11537 in Aquila | Hubble Space Telescope


This astronomical portrait from the NASA/European Space Agency Hubble Space Telescope showcases an edge-on view of the majestic spiral galaxy UGC 11537. Hubble’s Wide Field Camera 3 has captured the tightly wound spiral arms swirling around the heart of UGC 11537 at infrared and visible wavelengths, showing both the bright bands of stars and the dark clouds of dust threading throughout the galaxy. 

UGC 11537 is 230 million light-years away in the constellation Aquila, and lies close to the plane of the Milky Way. Being so close to the starry band of the Milky Way means that foreground stars from our own galaxy have crept into the image—the two prominent stars in front of UGC 11537 are interlopers from within the Milky Way. These bright foreground stars are surrounded by diffraction spikes—imaging artifacts caused by starlight interacting with Hubble’s inner structure. 

This image came from a set of observations designed to help astronomers weigh supermassive black holes in distant galaxies. The combination of Hubble’s sharp-eyed observations and data from ground-based telescopes allowed astronomers to make detailed models of the mass of stars in these galaxies. This in turn helps constrain the mass of supermassive black holes.


Credit: ESA/Hubble & NASA, A. Seth
Release Date: Nov. 15, 2021

#NASA #ESA #Hubble #Astronomy #Space #Science #Galaxies #UGC11537 #GalaxyClusters #SpiralGalaxies #BlackHoles #AGNs #AquilaConstellation #Cosmos #Universe #HST #HubbleSpaceTelescope #WFC3 #GSFC #STScI #UnitedStates #Europe #STEM #Education

What's Up for June 2026 | Skywatching Tips from NASA | Jet Propulsion Laboratory

What's Up for June 2026 | Skywatching Tips from NASA | Jet Propulsion Laboratory

Here are examples of skywatching highlights for the northern hemisphere in June 2026: 

Venus and Jupiter meet after sunset, the Moon passes in front of Venus, summer begins, and deep-sky treasures rise into view.

To start June, look west after sunset to spot Venus and Jupiter shining close together, with Mercury joining the view low in the sky. 

Around June 9, Venus and Jupiter appear especially close in a planetary conjunction. 

From June 11 through 15, Mercury joins the scene, creating a mini-parade of planets near the western horizon. 

On June 17, from certain locations, the Moon passes in front of Venus in an event called a lunar occultation. For viewers outside the exact viewing path, the Moon and Venus may still appear close together. [Important safety note: For many viewers, this event happens during the daytime. Never point binoculars, a telescope, or a camera near the Sun unless you are using proper solar-safe equipment.] 

June also brings the summer solstice, marking the start of astronomical summer in the Northern Hemisphere. 

And once the sky gets dark, look for the Summer Triangle and deep-sky objects like the Dumbbell Nebula, Ring Nebula, North America Nebula, and Veil Nebula.

0:00 Intro

0:11 Venus and Jupiter after sunset

0:23 Planetary conjunction

0:35 Mercury joins the lineup

1:09 Moon passes in front of Venus

2:03 Summer solstice

2:43 Summer Triangle and deep-sky objects

3:27 Moon phases


Video Credit: NASA's Jet Propulsion Laboratory
Duration: 4 minutes
Release Date: June 1, 2026


#NASA #Astronomy #Space #Science #SolarSystem #Planets #Mercury #Venus #Jupiter #Earth #SummerSolstice #Moon #Stars #Nebulae #Galaxies #MilkyWayGalaxy #Skywatching #JPL #Caltech #UnitedStates #Canada #Mexico #NorthernHemisphere #STEM #Education #HD #Video

Cosmonaut Photos: Kondyor Massif in Russian Far East | International Space Station

Cosmonaut Photos: Kondyor Massif in Russian Far East | International Space Station


Expedition 74 commander and Roscosmos cosmonaut Sergey-Kud Sverchkov of Russia: "Another landmark of the Far East. It's completely unpopular with tourists, and therefore little-known. But that doesn't make it any less remarkable.

. . . This is the Kondyor mountain range in Khabarovsk Krai. The local Evenki called this mountain Urgulya and considered it sacred, and in 1936, Soviet explorers of the Far East discovered it.

This perfect ring, approximately 8 kilometers in diameter and with an elevation difference of approximately 600 meters, is a true geological wonder.

Where did it come from?

Various theories have been put forward regarding the formation of this unusual massif, from the fall of a giant meteorite to volcanic activity. The truth turned out to be much more prosaic: the massif was formed by a magmatic intrusion. To put it more clearly, a magma flow (a magmatic diapir—an inverted magma drop) rose under pressure along a fault in the Earth's crust, melting rocks, but ultimately failed to reach the surface. This process continued for over 60,000 years, resulting in the magma pushing out the upper layers of rock, lifting them into a dome. Erosion over 150 million years transformed the dome into a ring of durable ultramafic rocks (more precisely, a dunite-clinopyroxenite-gabbro complex). I intentionally inserted a geological term here to make it sound terrifying, beautiful, and powerful. And relatable to those who understand geology.

But shape isn't the only feature of this place. The material that rose from the depths to the surface brought with it large quantities of platinum, gold, chromium, and other valuable metals, such as iridium and rhodium. There's also an endemic mineral here—conderite. Until the 1970s, platinum was found in the Kondyor River bed, which flows out of the massif. Mining later extended to the primary source in the center of the massif. This is one of the largest platinum deposits in the world, with nuggets weighing between 1.5 and 3.5 kg found here. This is another reason why the area is closed to tourists."

The Kondyor Massif or Konder is a circular intrusion of igneous rock, about 8 kilometers (5 mi) in diameter. It is located in Khabarovsk Krai, Russia, c. 600 km (373 mi) west-southwest of Okhotsk, or c. 570 km (354 mi) south-east of Yakutsk. It is reached from Yakutsk by road via Amga. The Kondyor Massif is a textbook example of a ring intrusion, renowned for its remarkable geometric circularity and distinct ridge-and-depression topography. It serves as a global reference site for the study of alkaline-ultramafic magmatism and associated platinum-group element mineralization.


Expedition 74 Crew
Station Commander: Sergey-Kud Sverchkov (Russia)
Roscosmos (Russia) Flight Engineers:
Andrey Fedyaev, Sergei Mikaev
European Space Agency Flight Engineer: Sophie Adenot
NASA Flight Engineers: Jessica Meir, Jack Hathaway, Chris Williams

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 Credit: Roscosmos/Sergey-Kud Sverchkov
Release Date: May 16, 2026

#NASA #Space #Science #ISS #Earth #Geology #RussianFarEast #Siberia #KhabarovskKrai #KondyorMassif #горыКондёр #Astronauts #Cosmonauts #SergeyKudSverchkov #CosmonautPhotography #Russia #Россия #Roscosmos #Роскосмос #HumanSpaceflight #InternationalCooperation #Expedition74 #UnitedStates #ESA #Europe #STEM #Education

United Launch Alliance Atlas V Launch of Amazon LEO 7 Satellites: Highlights

United Launch Alliance Atlas V Launch of Amazon LEO 7 Satellites: Highlights

A United Launch Alliance (ULA) Atlas V rocket carrying the LEO 7 mission for Amazon lifted off on May 29, 2026, at 7:53 p.m. EDT from Space Launch Complex-41 at Cape Canaveral. This delivered another 29 LEO satellites to low Earth orbit, adding coverage and capacity to the network and "bringing LEO a step closer to connecting customers around the world."

Named LA-07 (LEO Atlas 7), the mission marks Amazon’s seventh launch on ULA’s Atlas V rocket and twelfth mission overall, bringing the total number of satellites deployed to 331.

Atlas V deployed the satellites at an altitude of approximately 289 miles (465 kilometers) above Earth, after which the Amazon LEO team assumed control of the mission from our mission operations center in Redmond, Washington. Teams have completed initial contact and health checks and will continue preparing the satellites to raise to their assigned operational altitude of 392 miles (630 kilometers).

Amazon LEO, formerly Project Kuiper, is Amazon’s low Earth orbit satellite network. "Its mission is to deliver fast, reliable internet to customers and communities beyond the reach of existing networks, and we began a full-scale deployment of our satellite constellation in April 2025."

Amazon LEO has completed 11 missions and launched more than 300 satellites in its first year of launch operations, making it the third-largest constellation in orbit, and Amazon plans to increase its launch rate over time with more than 100 launches secured to date.

Mission name: LA-07 (LEO Atlas 7)

Launch vehicle: ULA Atlas V 551

Launch date/time: Friday, May 29, 7:53 p.m. EDT

Number of satellites: 29

Launch site: Space Launch Complex-41, Cape Canaveral

ULA website: www.ulalaunch.com


Credit: United Launch Alliance (ULA)
Duration: 1 minute
Release Date: June 1, 2026

#NASA #Space #Satellites #Earth #CommercialSpace #UnitedLaunchAlliance #ULA #AtlasVRocket  #LockheedMartin #Boeing #Amazon #AmazonLEO #AmazonLEO7 #LEO #CommunicationsSatellites #CapeCanaveral #Florida #UnitedStates #STEM #Education #HD #Video

China Long March-12B Rocket before First Launch: Spacesail Constellation Satellites

China Long March-12B Rocket before First Launch: Spacesail Constellation Satellites








🚀 China's new Long March-12B Y1 rocket (a reusable capable variant) blasted off for the first time from the Dongfeng Commercial Space Innovation Pilot Zone in northwest China at 4:40pm Beijing Time (08:40 UTC) on June 1, 2026, sending the tenth batch of Spacesail (Qianfan Jigui) 08 Internet constellation satellites into a polar orbit. No booster recovery was attempted during this flight.

The mission was the maiden flight of Long March 12B rocket and marked the 647th flight mission of the Long March carrier rocket series. 

D4.37m, 9 YF-102V kerosene and liquid oxygen (kerolox) engines were in the first stage and 1 YF-102V in the second stage.

The Long March 12B (Chang Zheng 12B, abbreviated CZ-12B), is a Chinese reusable medium-lift to heavy-lift launch vehicle. The rocket has two stages and its first stage is designed to be reused after stage-recovery via a propulsive landing. Both stages of the rocket use kerosene and liquid oxygen (LOX) for propulsion. The rocket is being developed by the China Aerospace Science and Technology Corporation Commercial Rocket Co., Ltd. (CACL), operating under the state-owned China Aerospace Science and Technology Corporation (CASC).


Image Credit: China Aerospace Science and Technology Corporation (CACL)
Date: June 1, 2026

#NASA #Space #Science #Earth #Satellites #SpaceSailConstellation #QianfanConstellation #千帆星座 #China #中国 #Rockets #LongMarch12BRockets #长征十二号乙运载火箭 #MediumLiftRockets #CACL #CASC #SpaceTechnology #CommercialSpace #CommercialSpaceflight #Spaceports #InnerMongolia #STEM #Education

First China Long March-12B Rocket Launch: Spacesail Constellation Satellites

First China Long March-12B Rocket Launch: Spacesail Constellation Satellites










🚀 China's new Long March-12B Y1 rocket (a reusable capable variant) blasted off for the first time from the Dongfeng Commercial Space Innovation Pilot Zone in northwest China at 4:40pm Beijing Time (08:40 UTC) on June 1, 2026, sending the tenth batch of Spacesail (Qianfan Jigui) 08 Internet constellation satellites into a polar orbit. No booster recovery was attempted during this flight.

The mission was the maiden flight of Long March 12B rocket and marked the 647th flight mission of the Long March carrier rocket series. 

D4.37m, 9 YF-102V kerosene and liquid oxygen (kerolox) engines were in the first stage and 1 YF-102V in the second stage.

The Long March 12B (Chang Zheng 12B, abbreviated CZ-12B), is a Chinese reusable medium-lift to heavy-lift launch vehicle. The rocket has two stages and its first stage is designed to be reused after stage-recovery via a propulsive landing. Both stages of the rocket use kerosene and liquid oxygen (LOX) for propulsion. The rocket is being developed by the China Aerospace Science and Technology Corporation Commercial Rocket Co., Ltd. (CACL), operating under the state-owned China Aerospace Science and Technology Corporation (CASC).


Image Credit: China Aerospace Science and Technology Corporation (CACL)
Date: June 1, 2026

#NASA #Space #Science #Earth #Satellites #SpaceSailConstellation #QianfanConstellation #千帆星座 #China #中国 #Rockets #LongMarch12BRockets #长征十二号乙运载火箭 #MediumLiftRockets #CACL #CASC #SpaceTechnology #CommercialSpace #CommercialSpaceflight #Spaceports #InnerMongolia #STEM #Education

First China Long March-12B Rocket Launch: Spacesail Constellation Satellites

First China Long March-12B Rocket Launch: Spacesail Constellation Satellites


🚀 China's new Long March-12B Y1 rocket (a reusable capable variant) blasted off for the first time from the Dongfeng Commercial Space Innovation Pilot Zone in northwest China at 4:40pm Beijing Time (08:40 UTC) on June 1, 2026, sending the tenth batch of Spacesail (Qianfan Jigui) 08 Internet constellation satellites into a polar orbit. No booster recovery was attempted during this flight.

The mission was the maiden flight of Long March 12B rocket and marked the 647th flight mission of the Long March carrier rocket series. 

D4.37m, 9 YF-102V kerosene and liquid oxygen (kerolox) engines were in the first stage and 1 YF-102V in the second stage.

The Long March 12B (Chang Zheng 12B, abbreviated CZ-12B), is a Chinese reusable medium-lift to heavy-lift launch vehicle. The rocket has two stages and its first stage is designed to be reused after stage-recovery via a propulsive landing. Both stages of the rocket use kerosene and liquid oxygen (LOX) for propulsion. The rocket is being developed by the China Aerospace Science and Technology Corporation Commercial Rocket Co., Ltd. (CACL), operating under the state-owned China Aerospace Science and Technology Corporation (CASC).


Video Credit: China Aerospace Science and Technology Corporation (CACL)
Duration: 1 minute, 15 seconds
Release Date: June 1, 2026

#NASA #Space #Science #Earth #Satellites #SpaceSailConstellation #QianfanConstellation #千帆星座 #China #中国 #Rockets #LongMarch12BRockets #长征十二号乙运载火箭 #MediumLiftRockets #CACL #CASC #SpaceTechnology #CommercialSpace #CommercialSpaceflight #Spaceports #InnerMongolia #STEM #Education #HD #Video

First Flight of NASA's Quiet Supersonic X-59 Aircraft | Lockheed Martin

First Flight of NASA's Quiet Supersonic X-59 Aircraft | Lockheed Martin

As the X-59 quickly advances towards more historic firsts, we are taking a look back at the flight that started it all, with NASA test pilot David "Nils" Larson.

More about X-59's revolutionary design and mission: https://www.lockheedmartin.com/en-us/products/x-59-quiet-supersonic.html

Since the aircraft’s first flight, the X-59 team has spent months evaluating its performance and handling qualities across a growing range of flight conditions. Take a look at the milestones achieved so far that mark steady progress as NASA moves closer to the aircraft’s first supersonic flight.

The upcoming supersonic flights will help engineers evaluate the aircraft’s performance across more of its operating range as teams advance toward later phases of the Quesst mission.

The X-59 aircraft builds on decades of supersonic flight research and is the centerpiece of NASA’s Quesst mission. The vast amount of data collected over the years has given designers the tools they needed to craft the shape of the X-59. The goal is to enable the aircraft to fly at supersonic speeds and reduce a loud sonic boom to a quieter “sonic thump.”

Data gathered during X-59 research flights will be shared with the U.S. and international regulators to inform the establishment of new, data-driven acceptable noise thresholds related to supersonic commercial flight over land.

The X-59’s engine, a modified F414-GE-100, packs 22,000 pounds of thrust. This will enable the X-59 to achieve the desired cruising speed of Mach 1.4 (925 miles per hour) at an altitude of approximately 55,000 feet. It sits in a nontraditional spot–atop the aircraft—to aid in making the X-59 quieter.

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

Learn more about NASA's Quesst mission: https://www.nasa.gov/blogs/quesst/


Video Credit: Lockheed Martin
Duration: 2 minutes, 54 seconds
Release Date: June 1, 2026

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

Shenzhou-21 Crew Delivers New Batch of Research Samples | China Space Station

Shenzhou-21 Crew Delivers New Batch of Research Samples China Space Station

The latest batch of scientific samples from China's space station, totaling approximately 41 kilograms, was brought back to Earth aboard the Shenzhou-22 return capsule carrying the Shenzhou-21 crew, according to the Technology and Engineering Center for Space Utilization (CSU) under the Chinese Academy of Sciences (CAS).

Marking the 10th transfer of materials from the orbiting laboratory, the samples came from 23 experiments in space life sciences, materials science and combustion research, including nine types of biological samples, 12 material samples and two combustion samples.

Among the most notable findings, scientists observed that zebrafish embryos had successfully hatched into tiny fishes aboard the space station.

"Life science experiments in orbit were highly demanding. Cell development happens very quickly, so we had to constantly refocus and take photos to track changes in the biological samples. When we saw that the zebrafish embryos had hatched into small fishes and started swimming, the entire team was thrilled. Notably, our experiment on 'artificial embryos' (stem cell-derived artificial human embryos) was fully recorded in orbit, and the embryos are in very good condition," said Sun Yuanyuan, a senior engineer at the CSU.

The artificial embryo experiment is among the most anticipated. Researchers will use transcriptome sequencing and proteomic analysis to understand how the space environment affects early human embryo development and stem cell behavior. The studies will also explore the effects of microgravity on kidney organoid development and fibrosis, as well as the molecular mechanisms behind bone metabolism imbalance and cardiovascular dysfunction under weightless conditions.

Another experiment focuses on chirality, the property of molecules that are mirror images but not identical, similar to left and right hands.

"Chirality is a project we sent to the space station on a previous Shenzhou-21 mission. It explores the chiral characteristics that appear during the formation of amino acids in living organisms. As we know, humans have a left hand and a right hand. They are mirror images, but they don't perfectly overlap. Many chemical molecules in nature share this mirror-symmetry property. That phenomenon is called chirality. In this experiment, we focus on how small biological molecules select their chiral partners, so that we can understand how chirality selection differs between Earth and space environments," said Liu Wei, another senior engineer at the center.

These findings will help scientists understand how living organisms adapt to space environments, providing critical theoretical knowledge for long-term human space habitation and deep-space exploration.

For the returned materials science samples, including new titanium alloys, high-strength steel and relaxor ferroelectric single crystals, researchers will examine their microstructures, chemical composition and elemental distribution, the CSU said. These analyses will clarify how gravity influences material growth, composition segregation, solidification defects and overall performance.

Combustion experiment samples, including burners and soot collection plates, will be analyzed to study semiconductor nanomaterial synthesis, soot formation and nanocarbon particle characteristics. The results are expected to advance aerospace technology, high-end equipment manufacturing, new energy systems and space fire safety.


Video Credit: CCTV
Duration: 2 minutes, 35 seconds
Release Date: May 30, 2026


#NASA #Space #Science #China #中国 #Shenzhou22CrewCapsule #Shenzhou21Mission #神舟二十一号 #Shenzhou21 #Taikonauts #Astronauts #ZhangLu #WuFei #ZhangHongzhang #ChinaSpaceStation #中国空间站 #TiangongSpaceStation #SpaceLaboratory #MicrogravityExperiments #CMSA #中国载人航天工程办公室 #HumanSpaceflight #STEM #Education #HD #Video

The Rosette Nebula in Monoceros | Kitt Peak National Observatory

The Rosette Nebula in Monoceros | Kitt Peak National Observatory


The appropriately named Rosette Nebula is, not unlike a newly bloomed flower, a place of newfound life. Many of the stars within this wreath of gas have just formed. Their energetic winds and emissions of ultraviolet (UV) radiation are quickly blowing away the surrounding clouds of gas to reveal a new cluster of stars. Many thicker parts of the cloud resist their ultimate demise, and remain in radial structures stubborn to relent to the impressive forces arrayed against them. The initial mass of gas clouds such as this determine how many stars are formed within. A very massive cloud will likely form many stars. Here, the stars in the heart of the Rosette nebula are blowing away the building blocks of more stars and have halted most other star formation. However, there are many globules of gas (Bok globules) that may contain individual stars still in the process of forming. Bok globules are isolated and relatively small dark nebulae containing dense cosmic dust and gas where star formation can take place.

The Rosette Nebula (also known as Caldwell 49) is an H II region located near one end of a giant molecular cloud in the Monoceros region of the Milky Way Galaxy. An H II region is a region of interstellar atomic hydrogen that is ionized. The open cluster NGC 2244 (Caldwell 50) is closely associated with the nebulosity, the stars of the cluster having been formed from the nebula's matter. The nebula has a shape reminiscent of a human skull, and is sometimes referred to as the "Skull Nebula". It is not to be confused with NGC 246 that is also nicknamed the "Skull Nebula".

This image was taken as part of Advanced Observing Program (AOP) program at Kitt Peak Visitor Center in Arizona.

Learn more about Kitt Peak National Observatory (KPNO):
https://kpno.noirlab.edu/


Credit: KPNO/NOIRLab/NSF/AURA/Walter Mulligan/Flynn Haase
Release Date: June 12, 2014

#NASA #Astronomy #Space #Science #Stars #Nebulae #RosetteNebula #Caldwell49 #StellarNurseries #BokGlobules #MonocerosConstellation #Cosmos #Universe #KPNO #KittPeakNationalObservatory #Arizona #NOIRLab #NSF #AURA #UnitedStates #STEM #Education

Sunday, May 31, 2026

Cosmonaut Photos: Mount Everest & The Himalayas | International Space Station

Cosmonaut Photos: Mount Everest & The Himalayas | International Space Station




Expedition 74 commander and Roscosmos cosmonaut Sergey-Kud Sverchkov of Russia: "Yes, because it exists!"

"That's how George Mallory answered the question of why people climb Everest. And it seems nothing has changed in a hundred years."

"Everest is the highest mountain on Earth, at 8,848.86 meters. A Himalayan giant on the border of Nepal and Tibet, the peak has become a symbol of the limits of human possibility."

For local people, the mountain has always been Chomolungma—'Divine Mother of the World' in Tibetan. In Nepal, it is called Sagarmatha—'Forehead of Heaven.' The name 'Everest' was coined in the 19th century in honor of British surveyor George Everest after the Great Trigonometric Survey of India.

The first attempts to climb it began in the 1920s. 73 years ago, on May 29, 1953, Edmund Hillary and Tenzing Norgay made the first official ascent. There are approximately 20 routes to the summit, although two remain the main ones: the southern route through Nepal and the northern route through Tibet.

Today, Everest is considered an 'accessible' eight-thousander technically, thanks to commercial expeditions, fixed ropes, and a large number of routes. But the altitude here remains unforgiving."


Expedition 74 Crew
Station Commander: Sergey-Kud Sverchkov (Russia)
Roscosmos (Russia) Flight Engineers:
Andrey Fedyaev, Sergei Mikaev
European Space Agency Flight Engineer: Sophie Adenot
NASA Flight Engineers: Jessica Meir, Jack Hathaway, Chris Williams

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 Credit: Roscosmos/Sergey-Kud Sverchkov
Release Date: May 29, 2026

#NASA #Space #Science #ISS #Earth #MountEverest #Chomolungma #Sagarmatha #Himalayas #Nepal #China #中国 #Astronauts #Cosmonauts #SergeyKudSverchkov #CosmonautPhotography #Russia #Россия #Roscosmos #Роскосмос #HumanSpaceflight #InternationalCooperation #Expedition74 #UnitedStates #ESA #Europe #STEM #Education

Moonrise Blues over New York

Moonrise Blues over New York

Astrophotographer James Perez-Rogers: "A rare blue moon was set to rise yesterday evening and I set out to photograph it lined up with the Ferncliff Firetower in Rhinebeck, NY. The micro moon looked visually smaller than normal, but with the long lens and cropping it appears quite large."

When you hear someone say, "Once in a blue moon …" you know they are talking about something rare. A blue moon is not blue in color. In fact, a blue moon does not look any different than a regular, monthly full moon.

Rather, a blue moon is special because it is the "extra" Moon in a season with four full moons. This usually only happens every two-and-a-half years. Since the 1940s, the term "blue moon" has also been used for the second full moon in a calendar month. This usually happens only every two-and-a-half years.

New York, also called New York State, is a state located in the northeastern United States. Bordering New England to its east, Canada to its north, and Pennsylvania and New Jersey to its south, it extends into the Atlantic Ocean and the Great Lakes.


Image Credit: James Perez-Rogers
Location: Kingston, New York
Image Details: EXIF: Sony A6500 Sony 200-600mm F6.3 ISO800 1/30s
James' Website: https://www.jamesperezrogers.com
Date: May 30, 2026

#NASA #Astronomy #Space #Science #Earth #Moon #BlueMoon #Sun #SolarSystem #Cosmos #Universe #Astrophotographers #JamesPerezRogers #Astrophotography #UnitedStates #Kingston #NewYork #STEM #Education

The Snake Nebula in Ophiuchus

The Snake Nebula in Ophiuchus

The Snake Nebula, also known as Barnard 72 and LDN 66, is an iconic dark nebula in the Ophiuchus constellation. It is part of the much larger Dark Horse Nebula (occupies the edge of the belly). The Snake Nebula is around 650 light years from Earth. It is a small dust lane that snakes out in front of Milky Way star clouds. 


Credit: Giuseppe Donatiello (Oria Amateur Astrophysical Observatory - OAAO)
Image Details: 127ED f/9 refractor + EOS 4000D 
Capture Location: Piano Visitone, Pollino National Park, Italy
Image Date: 2025
Release Date: May 30, 2026

#NASA #Astronomy #Space #Science #Nebulae #SnakeNebula #Barnard72 #LDN66 #Barnard68 #OphiuchusConstellation #Cosmos #Universe #Astrophotographers #GiuseppeDonatiello #Astrophotography #Italy #Italia #STEM #Education

Planet Mars Images: May 26-31, 2026 | NASA's Curiosity & Perseverance Rovers

Planet Mars Images: May 26-31, 2026 | NASA's Curiosity & Perseverance Rovers

Mars 2020 - sol 1875
Mars 2020 - sol 1875
Mars 2020 - sol 1875
Mars 2020 - sol 1871
Mars 2020 - sol 1872
MSL - sol 4907
MSL - sol 4905
Mars 2020 - sol 1871


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Celebrating 13+ Years on Mars (2012-2025)
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 5+ Years on Mars
Mission Name: Mars 2020
Rover Name: Perseverance
Main Job: Seek signs of ancient life and collect samples of rock and regolith (broken rock and soil) for return to Earth.
Launch: July 30, 2020
Landing: Feb. 18, 2021, Jezero Crater, Mars

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

Image Credits: NASA/JPL-Caltech/ASU/MSSS
Processing: Kevin M. Gill
Release Dates: May 26-31, 2026

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