Sunday, August 02, 2026

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.


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