Tuesday, October 06, 2026

The Milky Way: View from Utah

The Milky Way: View from Utah



Astrophotographer Cary Bahora: "I'm 60 and never seen so many stars as I did in the extremely remote Henry Mountains of Utah at 10,500 ft. It was amazing walking around seeing clearly only by starlight. Two pics looking south. Other looking north. And is that a galaxy in the lower right on the northward looking pic?"

Generally speaking, the best time to see the Milky Way galaxy is during the Milky Way season from February to October, usually between 00:00 and 5:00, and on nights with a New Moon. This, however, will vary depending on the hemisphere, your latitude, and other factors like the moon phase.

The Henry Mountains is a mountain range located in the southeastern portion of the U.S. state of Utah that runs in a generally north-south direction, extending over a distance of about 30 miles (48 km). 

Utah is a landlocked state in the Mountain West subregion of the Western United States. It is one of the Four Corners states, sharing a border with Arizona, Colorado, and New Mexico. It also borders Wyoming to the northeast, Idaho to the north, and Nevada to the west.


Image Credit: Cary Bahora
Location: Henry Mountains, Utah, United States
Date: Oct. 1, 2026

#NASA #Astronomy #Space #Science #SolarSystem #Stars #SagittariusConstellation  #MilkyWayGalaxy #Cosmos #Universe #Astrophotography #CaryBahora #Astrophotographers #HenryMountains #Utah #UnitedStates #STEM #Education

The Northern Lights over Reykjavik, Iceland

The Northern Lights over Reykjavik, Iceland

Astrophotographer Wioleta Gorecka: "This time, I wanted to capture the aurora borealis in the center of Reykjavík. It is not an easy task due to light pollution; the aurora needs to be strong enough to be visible and allow for a proper exposure. I managed to capture the shot just as the famous Hallgrímskirkja church was illuminated in pink—a symbol of the fight against breast cancer. The colors harmonized beautifully."

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/

Iceland is a Nordic island country between the Arctic Ocean and the North Atlantic Ocean, located on the Mid-Atlantic Ridge between Europe and North America. Reykjavík is the capital and largest city of Iceland. It is located on the southern shore of the Faxaflói bay in southwest Iceland and has a latitude of 64°08′ N, making it the world's northernmost capital of a sovereign state.

Image Credit: Wioleta Gorecka
Location: Reykjavik, Hallgrimskirkja
Wioleta's website: https://instagram.com/wiola.gorecka?igshid=ff0xckzefdlb
Release Date: Oct. 5, 2026

#NASA #Astronomy #Space #Science #Sun #SolarSystem #SolarWind #Planet #Earth #Magnetosphere #GeomagneticStorms #Aurora #AuroraBorealis #NorthernLights #Astrophotography #WioletaGorecka #Astrophotographers #Reykjavík #Iceland #Ísland #STEM #Education

Journey to The Flower Bud Nebula—NGC 7129 in Cepheus | Webb Telescope

Journey to The Flower Bud Nebula—NGC 7129 in Cepheus | Webb Telescope

This video takes the viewer on a journey through space to a technicolor dreamscape. It reveals a new image from the NASA/European Space Agency/Canadian Space Agency James Webb Space Telescope. It portrays a stellar nursery known as NGC 7129, a nebula that holds numerous protostars and stars within its fields of gas and dust. Webb captured infrared light that pierces through the dense matter that scatters or absorbs other types of light. This region, rife with stellar objects at various stages of their lives, offers an opportunity to explore how stars shape their surrounding environment.

Also known as the Flower Bud Nebula or Small Cluster Nebula, NGC 7129 is a reflection nebula located about 3,300 light years away in the constellation Cepheus. A young open cluster is responsible for illuminating the surrounding nebula. The region to the left of the central star is filled with hot, atomic hydrogen gas. This creates a golden glow, while the region to the right is packed with cooler, molecular hydrogen. Embedded protostars in the rightmost region eject outflows that shock and heat the region, giving certain areas a red hue and a clumpy texture. Many of these red outflows, ejected as protostars accumulate mass, are visible throughout the image.

The central star and the stars embedded within the golden region are at a more mature stage in their life cycle than the protostars growing to the right of the central star. Their heat breaks down the molecular hydrogen into atoms, driving variations in temperature and color. The coldest, densest gas, where protostars have yet to form, is shown in grey.


Credit: ESA/Webb, NASA, CSA, WIYN and NOIRLab, NSF, AURA, DSS2, A. Pagan (STScI), N. Bartmann (ESA/Webb),  E. Slawik, N. Risinger, T. A. Rector, H. Schweiker, M. Zamani (ESA/Webb)
Duration: 1 minute, 30 seconds
Release Date: Oct. 6, 2026

#NASA #ESA #Astronomy #Space #Science #Stars #Protostars #Nebulae #StellarNurseries #NGC7129 #FlowerBudNebula #SmallClusterNebula #CepheusConstellation #Universe #JWST #NIRCam #InfraredAstronomy #SpaceTelescopes #Europe #NASAGoddard #STScI #UnitedStates #CSA #Canada #STEM #Education #HD #Video

Close-up: The Flower Bud Nebula—NGC 7129 in Cepheus | Webb Telescope

Close-up: The Flower Bud Nebula—NGC 7129 in Cepheus | Webb Telescope

A technicolor dreamscape is revealed in this new image from the NASA/European Space Agency/Canadian Space Agency James Webb Space Telescope. It portrays a stellar nursery known as NGC 7129, a nebula that holds numerous protostars and stars within its fields of gas and dust. Webb captured infrared light that pierces through the dense matter that scatters or absorbs other types of light. This region, rife with stellar objects at various stages of their lives, offers an opportunity to explore how stars shape their surrounding environment.

Also known as the Flower Bud Nebula or Small Cluster Nebula, NGC 7129 is a reflection nebula located about 3,300 light years away in the constellation Cepheus. A young open cluster is responsible for illuminating the surrounding nebula. The region to the left of the central star is filled with hot, atomic hydrogen gas. This creates a golden glow, while the region to the right is packed with cooler, molecular hydrogen. Embedded protostars in the rightmost region eject outflows that shock and heat the region, giving certain areas a red hue and a clumpy texture. Many of these red outflows, ejected as protostars accumulate mass, are visible throughout the image.

The central star and the stars embedded within the golden region are at a more mature stage in their life cycle than the protostars growing to the right of the central star. Their heat breaks down the molecular hydrogen into atoms, driving variations in temperature and color. The coldest, densest gas, where protostars have yet to form, is shown in grey.


Credit: NASA, ESA, CSA, STScI, N. Bartmann (ESA/Webb)
Image Processing: A. Pagan (STScI)
Duration: 30 seconds
Release Date: Oct. 6, 2026

#NASA #ESA #Astronomy #Space #Science #Stars #Protostars #Nebulae #StellarNurseries #NGC7129 #FlowerBudNebula #SmallClusterNebula #CepheusConstellation #Universe #JWST #NIRCam #InfraredAstronomy #SpaceTelescopes #Europe #NASAGoddard #STScI #UnitedStates #CSA #Canada #STEM #Education #HD #Video

The Flower Bud Nebula: NGC 7129 in Cepheus | James Webb Space Telescope

The Flower Bud Nebula: NGC 7129 in Cepheus | James Webb Space Telescope

The NASA/European Space Agency/Canadian Space Agency James Webb Space Telescope’s Near-InfraRed Camera (NIRCam) has revealed many protostars and stars within the glowing gases of NGC 7129. Also known as the Flower Bud Nebula or Small Cluster Nebula, NGC 7129 is a reflection nebula located about 3,300 light years away in the constellation Cepheus. A young open cluster is responsible for illuminating the surrounding nebula. The region to the left of the central star is filled with hot, atomic hydrogen gas. This creates a golden glow, while the region to the right is packed with cooler, molecular hydrogen. Embedded protostars in the rightmost region eject outflows that shock and heat the region, giving certain areas a red hue and a clumpy texture. Many of these red outflows, ejected as protostars accumulate mass, are visible throughout the image.

The central star and the stars embedded within the golden region are at a more mature stage in their life cycle than the protostars growing to the right of the central star. Their heat breaks down the molecular hydrogen into atoms, driving variations in temperature and color. The coldest, densest gas, where protostars have yet to form, is shown in grey.

Image Description: A young star cluster filled with many stars that display Webb’s unique eight-pronged diffraction pattern. At its center is a yellow star which sports the largest diffraction pattern. To the left of the star, there is a region filled with yellow dust and gas that extends from the star to the left border of the image. This yellow region extends from the bottom, covering about two-thirds of the image. The yellow region has several blue stars of different sizes embedded within. The top third lies outside of the yellow region. It holds a few bright protostars within dense gray gas. Those stars illuminate the gas, making it appear blue. A few red outflows from other protostars are visible above this grayish-blue region. To the right of the central star, there is a clumpy, flame-like plume of red dust and gas with protostars that emit a soft white light within. The plume is surrounded by more dense gray gas and dust. There are several background galaxies strewn throughout the image.


Credit: NASA, ESA, CSA, STScI
Image Processing: A. Pagan (STScI)
Release Date: Oct. 6, 2026

#NASA #ESA #Astronomy #Space #Science #Stars #Protostars #Nebulae #StellarNurseries #NGC7129 #FlowerBudNebula #SmallClusterNebula #CepheusConstellation #Cosmos #Universe #JWST #NIRCam #InfraredAstronomy #SpaceTelescopes #Europe #NASAGoddard #STScI #UnitedStates #CSA #Canada #STEM #Education

Monday, October 05, 2026

Swirling Spiral Galaxy Messier 83 in Hydra (radio telescope view) | ALMA

Swirling Spiral Galaxy Messier 83 in Hydra (radio telescope view) | ALMA

Like a portal to another dimension, a hypnotizing swirl is featured in this picture of the spiral galaxy Messier 83 (M83), also known as the Southern Pinwheel, located approximately 15 million light-years away. It is one of the brightest galaxies in the night sky, but this image––taken with the Atacama Large Millimeter/submillimeter Array (ALMA). ALMA does not show how M83 looks in the light our eyes can see. Instead, it depicts the light emitted by cold gas molecules, the ingredients of star formation.

Nicolas-Louis de Lacaille discovered M83 on February 17, 1752, at the Cape of Good Hope.

Astronomers are interested in molecular gas clouds as virtually all stars are born from their collapse. Once stars form, they heat up their surroundings, making it harder for gas to condense and form further stars. This, combined with galactic dynamics that continually stirs gas, controls the growth of galaxies. ALMA allows astronomers to map how the density and temperature of these gas clouds change at locations within a galaxy, such as the central regions, the spiral arms, or the space between them. This in turn helps us understand star formation in a variety of galactic environments. The European Southern Observatory (ESO) is an ALMA partner. 

M83 closely resembles our own galaxy, the Milky Way. Since M83 appears nearly face-on in the sky, astronomers enjoy a privileged view to study whether the recipe to turn gas into stars is universal or changes within M83.

Image Description: This image shows an object made of two spiral arms connected at the center, in shades of orange against a black background. The object is brightest at the center and along the spiral arms. The spirals are composed of cloud-like threads that become more diffuse further away from the center of the image, spreading out like loose tufts of wool.

The Atacama Large Millimeter/submillimeter Array (ALMA), an international astronomy facility, is a partnership of the European Southern Observatory (ESO), the U.S. National Science Foundation (NSF), and the National Institutes of Natural Sciences (NINS) of Japan in cooperation with the Republic of Chile. ALMA is funded by ESO on behalf of its Member States, by NSF in cooperation with the National Research Council of Canada (NRC) and the National Science and Technology Council (NSTC) in Taiwan, and by NINS in cooperation with the Academia Sinica (AS) in Taiwan and the Korea Astronomy and Space Science Institute (KASI).

ALMA construction and operations are led by ESO on behalf of its Member States; by the National Radio Astronomy Observatory (NRAO), managed by Associated Universities, Inc. (AUI), on behalf of North America; and by the National Astronomical Observatory of Japan (NAOJ) on behalf of East Asia. The Joint ALMA Observatory (JAO) provides the unified leadership and management of ALMA's construction, commissioning, and operation. 


Learn more about the Atacama Large Millimeter/submillimeter Array (ALMA):
https://www.almaobservatory.org/en/about-alma/

Credit: ALMA(ESO/NAOJ/NRAO)/J. Koda et al.
Release Date: Oct. 5, 2026

#NASA #Astronomy #Science #Space #Messier83 #M83 #SouthernPinwheelGalaxy #NGC5236 #SpiralGalaxies #HydraConstellation #Cosmos #Universe #ALMA #RadioAstronomy #Chile #NSF #AUI #NRAO #UnitedStates #NAOJ #Japan #ESO #Europe #STEM #Education

The Sombrero Galaxy's Tidal Streams: Messier 104 in Virgo | View from Namibia

The Sombrero Galaxy's Tidal Streams: Messier 104 in Virgo | View from Namibia


A deep image of the Sombrero galaxy reveals surprises. Messier 104 (M104) is named the Sombrero galaxy because, on shorter exposures, it looks like a hat. A key defining feature of this huge galaxy is a dark brim of dust that circles the disk galaxy's center. A much longer exposure, however, brings up a hairy past where a bright, hazy halo is revealed that extends well past the central disk and contains many unresolved stars. Surprisingly, in this stellar haze, structures can be seen that include a diagonal ring. These structures and tidal streams provide fresh evidence that M104 had a violent past and is surely the result of collisions and mergers of smaller galaxies. Light takes about 30 million years to reach us from the Sombrero galaxy. It fully spans about 150 thousand light years across. This image was taken over seven days in mid-2026 from Namibia.

Namibia, officially the Republic of Namibia, is a country in southern Africa. Its borders include the Atlantic Ocean to the west, Angola and Zambia to the north, Botswana to the east and South Africa to the south; in the northeast, approximating a quadripoint, Zimbabwe lies less than 200 meters (660 feet) away along the Zambezi River near Kazungula, Zambia.


Credit & Copyright: Engelbert Vollmer
Engelbert's website: https://app.astrobin.com/u/Fox368
Authors & Editors: Robert Nemiroff, Jerry Bonnell, Cecilia Chirenti, Keighley Rockcliffe
A service of the Astrophysics Science Division (ASD) at NASA's Goddard Space Flight Center, NASA Science Activation & Michigan Technological University (MTU)
Release Date: Oct. 5, 2026

#NASA #Astronomy #Space #Science #Galaxies #Messier104 #M104 #NGC4594 #SombreroGalaxy #VirgoConstellation #Cosmos #Universe #Astrophotographers #EngelbertVollmer #Astrophotography #NASAGoddard #MTU #UnitedStates #STEM #Education #APoD

Aurora Borealis over Four Mile Lake in Alberta, Canada

Aurora Borealis over Four Mile Lake in Alberta, Canada




Astrophotographer John David McKinnon: "The Aurora Borealis dancing over Four Mile Lake on a perfectly peaceful fall night."

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/

Alberta is a province in Canada. It is a part of Western Canada and is one of the three prairie provinces. Alberta is bordered by British Columbia to its west, Saskatchewan to its east, the Northwest Territories to its north, and the U.S. state of Montana to its south.

Canada is a country in North America. Its ten provinces and three territories extend from the Atlantic Ocean to the Pacific Ocean and northward into the Arctic Ocean, making it the second-largest country by total area with the longest coastline of any country. Its border with the United States is the longest international land border.

Image Credit: John David McKinnon 
Location: Four Mile Lake, Dënéndeh, Alberta, Canada
Date: Oct. 2, 2026

#NASA #Astronomy #Space #Science #Stars #Sun #SolarSystem #Planets #Earth #Aurorae #AuroraBorealis #NorthernLights #MagneticFields #Magnetosphere #SolarWind #Astrophotography #JohnDavidMcKinnon #Astrophotographers #CitizenScience #FourMileLake #Dënéndeh #Alberta #Canada #NorthAmerica #STEM #Education

Planet Mars Images: Sept. 30-Oct. 5, 2026 | NASA's Curiosity & Perseverance Rovers

Planet Mars Images: Sept. 30-Oct. 5, 2026 | NASA's Curiosity & Perseverance Rovers

Mars 2020 - sol 1999
Mars 2020 - sol 1999
Mars 2020 - sol 1999
Mars 2020 - sol 1999
Mars 2020 - sol 1994
Mars 2020 - sol 1994
Mars 2020 - sol 1994
MSL - sol 5032

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Celebrating 14+ Years on Mars (2012-2026)
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
Release Dates: Sept. 30-Oct. 5, 2026

#NASA #Space #Astronomy #Science #Planets #Mars #Astrobiology #Geology #CuriosityRover #MSL #MountSharp #GaleCrater #PerseveranceRover #Mars2020 #JezeroCrater #Robotics #SpaceTechnology #SpaceEngineering #MSSS #JPL #Caltech #UnitedStates #CitizenScience #KevinGill #SpaceExploration #SolarSystem #STEM #Education

Dying Star Creates Brand New Planet | Hubble Space Telescope

Dying Star Creates Brand New Planet | Hubble Space Telescope

What if a star’s death could give rise to an entirely new planet?

Astronomers revisiting decades-old observations from NASA’s Hubble Space Telescope found an unexpected chemical clue around a white dwarf: niobium, a heavy element forged during the final stages of a star’s life. 

Combined with observations from other NASA missions, the evidence points to an intriguing possibility: a Jupiter-sized world may have formed from material expelled when the star died.

If confirmed, this “second-generation” planet could reveal that the death of a star is not always the end of its planetary system. It may result in the beginning of a new one.


Credit: NASA's Goddard Space Flight Center 
Paul Morris: Lead Producer
Cassandra Morris: Narrator
Video Credits:
Tracks Stars. They Look Like Meteors Video by NikitaMaykov via Pond5
White Dwarf and Exoplanet Animations created by Chris Smith and Scott Wiessinger
Death Valley National Park Milky Way Galaxy Time Lapse Night Sky Above Telescope Video by Lovemushroom via Pond5
Duration: 2 minutes, 35 seconds
Release Date: Oct. 5, 2026

#NASA #ESA #Astronomy #Space #Science #Stars #WhiteDwarfStars #Niobium #StellarEvolution #PlanetarySystems #Cosmos #Universe #HubbleSpaceTelescope #HST #NASAGoddard #STScI #UnitedStates #Europe #STEM #Education #HD #Video

Crew-12 Farewell & Change of Command Ceremony | International Space Station

Crew-12 Farewell & Change of Command Ceremony | International Space Station

Aboard the International Space Station, Crew-12 NASA astronauts Jessica Meir and Jack Hathaway as well as European Space Agency astronaut Sophie Adenot and Roscosmos cosmonaut Andrey Fedyaev of Russia, provided farewell remarks on Oct. 4, 2026, ahead of their upcoming departure from the space station.

Joining Crew-12 for the farewell remarks were NASA astronauts Jessica Watkins, Luke Delaney, and Anil Menon as well as Canadian Space Agency astronaut Josh Kutryk and Roscosmos cosmonauts Sergey Teteryatnikov, Andrey Fedyaev, Pyotr Dubrov, and Anna Kikina of Russia. Following the farewell remarks a change of command ceremony took place where Meir handed over command of the space station to Dubrov. 

Crew-12 is slated to undock on Oct. 5 and splash down off the coast of California Oct. 6 after completing a long-duration science mission living and working aboard the microgravity laboratory to advance scientific knowledge and demonstrate new technologies for future human and robotic exploration missions. Such research benefits people on Earth and lays the groundwork for future human exploration through the agency’s Artemis missions that will send astronauts to the Moon to prepare for future expeditions to Mars.


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

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


Video Credit: NASA's Johnson Space Center
Duration: 10 minutes
Date: Oct. 4, 2026


#NASA #Space #Science #Earth #ISS #SpaceXCrewDragonSpacecraft #Crew12 #Astronauts #JessicaMeir #JackHathaway #SophieAdenot #Europe #ESA #Cosmonauts #AndreyFedyaev #Russia #Россия #Roscosmos #Роскосмос #HumanSpaceflight #InternationalCooperation #Expedition75 #UnitedStates #STEM #Education #HD #Video

Sunday, October 04, 2026

Planetary Nebula IC 4634 in Ophiuchus: Glowing Waves | Hubble

Planetary Nebula IC 4634 in Ophiuchus: Glowing Waves | Hubble

This striking Hubble image of the planetary nebula IC 4634 reveals two shining, S-shaped ejections from a dying star. This star, awash in glowing material at the center of the picture, bloated as it aged and launched its outer layers off into space. The star’s very hot, exposed core has since beamed intense ultraviolet radiation at these lost shells of gas, making them glow in rich colors.

This process has been far from orderly or calm, however, as revealed by the distinct, separate waves of thrown-off gases. One is more distant and therefore was spewed first, followed by a more recently ejected tide of matter that formed the tighter S-shape. The result is remarkably symmetric on each side of the central star.

The NASA/ESA Hubble Space Telescope’s Wide Field Planetary Camera 2 (WFPC2) captured this image of IC 4634. It is found more than about 7,500 light-years away in the constellation of Ophiuchus (the Serpent Holder). IC 4634 and other objects like it are known as planetary nebulae due to their appearance through early telescopes as rounded, faintly luminous discs similar to the distant planets Uranus and Neptune. 

This picture was created from images through five filters (F487N, F502N, F574M, F656N and F658N) that captured light emitted by elements in the gaseous features. The total aggregate exposure time was 4,000 seconds and the field of view is just 29 arcseconds across.


Credit: European Space Agency/Hubble and NASA
Release Date: May 10, 2010


#NASA #ESA #Astronomy #Space #Science #Nebulae #PlanetaryNebulae #IC4634 #OphiuchusConstellation #MilkyWayGalaxy #Cosmos #Universe #HubbleSpaceTelescope #HST #HubbleWFPC2 #NASAGoddard #STScI #UnitedStates #Europe #STEM #Education

Close-up: Nebula NGC 7380 in Cepheus | Kitt Peak National Observatory

Close-up: Nebula NGC 7380 in Cepheus | Kitt Peak National Observatory

NGC 7380 is a typical star-forming region in the direction of an outer spiral arm of our galaxy (around 7,000 light years distant). It is a young open cluster of stars in the northern circumpolar constellation of Cepheus, discovered by Caroline Herschel in 1787. This field contains many young energetic stars that make the natal gas surrounding them glow an intense pink/red. The majority of stars in this newly formed group are out of the field to the upper left. Their winds and radiation sculpt clouds of gas and dust into the mountainous ridges seen here. The darkest parts of this image are foreground clouds of dust thick enough to extinct the light beyond them. Also note the bright star (left of center) that is in a bluish bubble of gas. This may be a Wolf-Rayet star beginning to blow a bubble. Other famous examples of this action include The Bubble Nebula and Thor's Helmut.

This image was taken as part of Advanced Observing Program (AOP) program at Kitt Peak Visitor Center during 2014.


Credit: KPNO/NOIRLab/NSF/AURA/Kris Sandburg and Peter Jacobs/Adam Block
Release Date: June 11, 2014

#NASA #Space #Astronomy #Science #Nebulae #NGC7380 #WizardNebula #CepheusConstellation #MilkyWayGalaxy #Cosmos #Universe #KPNO #KittPeakNationalObservatory #Arizona #NOIRLab #NSF #AURA #UnitedStates #STEM #Education

NASA’s DAVINCI Probe Model Beats The Heat for Blistering Planet Venus Descent

NASA’s DAVINCI Probe Model Beats The Heat for Blistering Planet Venus Descent

This close-up photo shows the engineering development model for NASA’s Deep Atmosphere Venus Investigation of Noble gases, Chemistry, and Imaging (DAVINCI) probe. It was photographed prior to a major thermal evaluation, where the DAVINCI team demonstrated that it could insulate the instruments the probe will carry from the intense heat of planet Venus. The probe probe passed a key test that ran from Aug. 28 to Sept. 10, 2026.

The DAVINCI team took the engineering model to a furnace at Rex Heat Treat in Bedford, Pennsylvania. It is one of few facilities capable of heating up to Venus-like temperatures as rapidly as the probe would experience. They slid the yoga ball-sized vessel into a ceramic-lined chamber with heat-scorched walls and ratcheted up the temperature to 869 F, or 465 C, over the course of about an hour—the same pace the probe will heat up during its descent to the surface of Venus.

They repeated the thermal cycling process five more times. The engineering model made it through every cycle unscathed, indicating that the probe can withstand extreme temperatures and protect its delicate scientific instruments while traveling through Venus’ atmosphere. During the testing, hardware simulating the instruments was closely monitored via more than a hundred thermal sensors.

“The experiment was a rousing success with six runs to Venus’ surface temperature on our descent timeline of 55–60 minutes with full internal instrumentation,” said Jim Garvin, the principal investigator for DAVINCI at NASA’s Goddard Space Flight Center in Greenbelt, Maryland. “There hasn’t been such a complete assessment of spacecraft-scale hardware at Venus temperatures in the U.S. since the mid-1970s.”

The DAVINCI spacecraft is being developed to travel to Venus to investigate numerous unsolved puzzles, including whether the planet once had oceans and was habitable, like Earth. To explore these mysteries, the spacecraft will release a probe that will withstand hellish temperatures for nearly an hour as it descends through Venus’ toxic atmosphere, collecting data along the way.

“It’s a huge engineering challenge given how harsh the Venus environment is,” said Kristen Brown, the DAVINCI probe manager at NASA Goddard. “We had to create a system that can protect the instruments from the planet’s overwhelming heat while strategically letting in its high-temperature gases to study through special inlet ports.”

Encased in a corrosion resistant, strong-yet-lightweight titanium shell, the DAVINCI probe will be equipped with a suite of instruments to sample the composition of the gases of the Venusian atmosphere to determine what molecules they are made of and learn about the atmosphere’s structure. It will also contain cameras that will snap the highest-resolution images of Venus’ surface ever. Scientists will use these to make a new 3D map. The probe also has a radio system to send data back to its orbiting spacecraft 5,600 miles (9,000 kilometers) overhead.

This heat testing follows on the heels of a campaign earlier this summer to demonstrate the probe’s imaging system. The mission is currently working toward gaining approval to move into the final design and fabrication phase. “The DAVINCI team has now met both of the major mission milestones this year on an accelerated timeline,” Garvin said. Showing that the DAVINCI probe can withstand the Venusian heat, brings scientists one step closer to learning why Earth’s “twin” varies greatly from our home.


Previous Probe Missions at Planet Venus


NASA's Pioneer Venus Program (1978)
It consisted of two spacecraft—the Pioneer Venus Orbiter and the Pioneer Venus Multiprobe. The orbiter mapped Venus’ atmosphere and surface using radar, while the probes measured atmospheric composition and pressure with one probe transmitting data for over an hour after impacting the surface.

The Soviet Union's Venera Program (1961-1984)
The Venera program was a series of space probes developed by the Soviet Union between 1961 and 1984 to gather information about the planet Venus. A total of eighteen probes were sent, including two related Vega probes.

Thirteen probes successfully entered the Venusian atmosphere, including the two Venera-Halley probes. Ten of those successfully landed on the surface of the planet. Due to the extreme conditions, the probes could only survive for a short period on the surface, from 23 minutes to two hours.

The Venera program established a number of precedents in space exploration, among them being the first man-made devices to enter the atmosphere of another planet (Venera 3 on March 1, 1966), the first to make a soft landing on another planet (Venera 7 on December 15, 1970), the first to return images from another planet's surface (Venera 9 on June 8, 1975), the first to record sounds on another planet (Venera 13 on October 30, 1981), and the first to perform high-resolution radar mapping scans (Venera 15 on June 2, 1983). The intense pressures that led to the short lifespans of many of the probes was itself an important finding.


Image Credit: NASA/Mike Guinto
Release Date: Sept. 24, 2026

#NASA #Space #Astronomy #Science #SolarSystem #Planets #Venus #NASADAVINCIMission #PioneerVenusProgram #Atmospheres #Geology #VeneraProgram #Вене́ра #SovietUnion #History #Russia #Россия #VenusExploration #SpaceTechnology #Engineering #NASAGoddard #UnitedStates #STEM #Education

China's Rocket Launches Hit Record as Commercial Space Firms Scale Up

China's Rocket Launches Hit Record as Commercial Space Firms Scale Up

China carried out a record 70 rocket launch missions in the first nine months of 2026, up by about 19 percent from a year earlier, as its commercial space industry accelerated mass production, advanced reusable rocket technology and expanded satellite services overseas.

Ten launches took place in September alone. The Pallas-1 rocket made its maiden flight, adding a new model to China's commercial launch fleet, while Zhuque-2E and Gravity-1 became the first privately developed rockets to support the deployment of a low-Earth-orbit satellite internet constellation.

The surge in constellation launches is putting pressure on rocket makers to deliver vehicles faster and at lower cost. On Sept. 20, the Lijian-1 Y18 rocket placed nine satellites into orbit, continuing a launch cadence that has become roughly monthly for the model.

CAS Space, the commercial rocket maker behind Lijian-1, has cut the vehicle's final assembly cycle from three months to about 15 days by reorganizing production.

"We have adopted a pulse-line production model, dividing the final assembly of each rocket among six or seven fixed workstations, with different assembly tasks carried out at each one," said Xiang Zebin, deputy chief designer of the Lijian-1 carrier rocket at CAS Space.

Other commercial rocket companies are also beginning production before orders are finalized, shortening the time between receiving a contract and carrying out a launch. Several are developing multiple rocket models in parallel while building the capacity for batch deliveries.

"As we move from one rocket to 100, we have to think in industrial terms: can we produce rockets at scale while continuing to deliver successful launches? This depends on ensuring consistency from one vehicle to the next," said Bu Xiangwei, chairman of private Chinese launch company Orienspace.

Reusable technology is another focus as companies seek to lower costs and increase launch frequency for large satellite constellations.

On July 10, the Long March-10B completed the world's first recovery of a rocket stage using a net system at sea. On Aug. 19, LandSpace's Zhuque-3 Y2 carried out China's first controlled land recovery of an orbital-class rocket's first stage using landing legs. The two recovered stages are being inspected and refurbished in preparation for future flights.

"Reusing rockets multiple times can significantly reduce overall launch costs. I believe that within five to 10 years, we will be able to match international benchmarks for launch costs per kilogram," said Wang Xinyan, general manager of supply chain management at private rocket developer LandSpace.

China's commercial satellite companies are also looking overseas as domestic launch capacity expands. GalaxySpace's Lingzhi-09 Thai CubeSat was launched in August, marking the first time a Chinese commercial space company had completed satellite development, launch and in-orbit delivery for a Southeast Asian country.

 "This demonstrates that our satellite products, end-to-end satellite solutions and service capabilities are ready for overseas markets. Over the next three to five years, we aim to build a well-developed network of resources and deliver successful projects in Belt and Road partner countries, particularly across ASEAN," said Huang Heping, general manager of international business development at commercial satellite maker GalaxySpace.

China's first-nine-month launch total was 11 higher than the 59 recorded in the same period last year. The rise reflects a broader shift from individual satellite missions toward constellation deployment, batch launches and a more diverse range of space-based services.

"The string of successful launches across multiple rocket types shows that both state-backed developers and private companies have reached a high level of technological maturity. Rocketry's advanced technologies are also helping drive upgrades in related products and manufacturing," said Yang Yuguang, chairman of the Space Transportation Committee of the International Astronautical Federation.


Video Credit: CCTV
Duration: 2 minutes, 34 seconds
Release Date: Oct. 4, 2026

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NASA Flies in California’s Pacific Airshow

NASA Flies in California’s Pacific Airshow

NASA test pilot Mike Lippert flies an F/A‑18 with videographer Lori Losey in the back seat during a Pacific Airshow flyover at Huntington Beach, California, Friday, Oct. 2, 2026.



NASA photographer Jim Ross rides in the back seat of the agency’s newly painted F‑15, which honors America’s 250th birthday, during a transit flight to Huntington Beach, California, piloted by NASA test pilot Wayne Ringelberg, Thursday, Oct. 1, 2026.

Photographer Jim Ross captures images of NASA’s F/A‑18 from the back seat of an F‑15 flying alongside during the Pacific Airshow at Huntington Beach, California, Friday, Oct. 2, 2026.
NASA test pilot Mike Lippert takes a photo with two young visitors at the NASA exhibit during the Pacific Airshow at Huntington Beach, California, Friday, Oct. 2, 2026.

These pictures show NASA test pilot Mike Lippert flying an F/A‑18 aircraft with videographer Lori Losey in the back seat during a Pacific Airshow flyover at Huntington Beach, California, Friday, October 2, 2026. We also see NASA photographer Jim Ross riding in the back seat of the agency’s newly painted F‑15 aircraft, honoring America’s 250th birthday, during a transit flight to Huntington Beach, California, piloted by NASA test pilot Wayne Ringelberg, Thursday, October 1, 2026. 

Both aircraft will fly in the Pacific Airshow, Oct. 2-4, 2026. NASA is hosting an exhibit for the air show featuring Artemis, the X‑59, SkyFall, a lunar globe, and an Apollo 15 Moon rock, with pilots and research experts available throughout the weekend.

Learn more: 

Image Credit: NASA/Jim Ross
Dates: Oct. 1-2, 2026

#NASA #Aerospace #TestPilots #Aircraft #NASAF15 #NASAF15Eagle #NASAFA18 #NASAFA18Hornet #Science #Physics #Engineering #CivilianResearch #AeronauticalResearch #FlightTests #Boeing #McDonnellDouglas #NASAArmstrong #Edwards #Airshows #PacificAirshow #Huntington #California #UnitedStates #STEM #Education