Wednesday, May 20, 2026

The Firefox Nebula in Cassiopeia | Mayall Telescope

The Firefox Nebula in Cassiopeia | Mayall Telescope


This image shows off the impressive imaging capabilities of the new charge-coupled device (CCD) detectors in the Mosaic 1.1 camera on the Mayall 4-meter telescope at Kitt Peak National Observatory in Arizona. The image is of Sharpless 2-188 (Sh2-188), nicknamed the Firefox Nebula, an unusual planetary nebula located in the constellation Cassiopeia. The expanding gas from the planetary nebula is colliding with ambient gas in the interstellar medium. The nebula is nearly circular in shape but is much brighter to the southeast (lower left) because the central star is moving rapidly in that direction. Faint wisps of gas can also be seen in the opposite direction. 

Distance from Earth: ~715 light years

The image was generated with deep observations in the Hydrogen alpha filter (red) and the Oxygen [OIII] filter (cyan). In this image, North is up and East is to the left.


Credit: T.A. Rector/University of Alaska Anchorage, H. Schweiker/WIYN and NOIRLab/NSF/AURA
Release Date: June 30, 2020


#NASA #Astronomy #Space #Science #Nebulae #Sh2188 #Simeis22 #FirefoxNebula #CassiopeiaConstellation #Cosmos #Universe #MayallTelescope #KPNO #Arizona #NSF #AURA #UnitedStates #STEM #Education

Tuesday, May 19, 2026

NASA Psyche Mission Mars Flyby Highlights | JPL

NASA Psyche Mission Mars Flyby Highlights | JPL

Mars - Psyche Spacecraft Imager A - May 15, 2026
This view of the Martian surface shows streaks that have formed due to wind blowing over impact craters in the Syrtis Major region. The wind streaks extend to about 30 miles (50 kilometers) long, and the large craters near center-bottom of the scene average around 30 miles in diameter.




This view extends from the south polar cap northwards to the Valles Marineris canyon system and beyond.

NASA Psyche Mission emblem 

NASA’s Psyche spacecraft performed a successful flyby of Mars on May 15, 2026. This provided the mission team with a valuable practice run before the spacecraft's arrival at the mysterious asteroid Psyche in 2029. The Psyche spacecraft came within 2,864 miles (4,609 kilometers) of the planet’s surface. The flyby delivered a gravity assist from Mars generating a critical boost in speed and adjusting the spacecraft’s orbital plane without using any onboard propellant, sending it on its way toward the metal-rich asteroid Psyche.

The spacecraft is now headed directly toward the asteroid, located in the main asteroid belt between Mars and Jupiter. After the Mars flyby, the flight team analyzed radio signals between the spacecraft and NASA’s Deep Space Network (DSN), the agency’s global system for communicating with interplanetary spacecraft, to confirm that Psyche was on the correct trajectory.

“Although we were confident in our calculations and flight plan, monitoring the DSN’s Doppler signal in real time during the flyby was still exciting,” said Don Han, Psyche’s navigation lead at NASA’s Jet Propulsion Laboratory in Southern California. “We’ve confirmed that Mars gave the spacecraft a 1,000 mile‑per‑hour boost and shifted its orbital plane by about 1 degree relative to the Sun. We are now on course for arrival at the asteroid Psyche in summer 2029.”

In the days running up to and during close approach, all of Psyche’s instruments were powered up for calibration efforts, including its imagers, magnetometers, and gamma-ray and neutron spectrometer. As a bonus, Psyche captured Mars images from a rare perspective.

Because Psyche approached Mars from a high phase angle, the planet appeared as a thin crescent in the days running up to the close approach, lit by sunlight reflecting off its surface. In observations from the spacecraft’s multispectral imager, the crescent appeared brighter and extended farther around the planet’s disk than anticipated because of the strong scattering of sunlight through the planet’s dusty atmosphere. As Psyche passed from Mars’ nighttime skies to daytime, it took a rapid series of pictures of the surface around the time of closest approach.

“We’ve captured thousands of images of the approach to Mars and of the planet’s surface and atmosphere at close approach. This dataset provides unique and important opportunities for us to calibrate and characterize the performance of the cameras, as well as test the early versions of our image processing tools being developed for use at the asteroid Psyche,” said Jim Bell, the Psyche imager instrument lead at Arizona State University (ASU) in Tempe. “As the spacecraft continues its journey after the flyby, we’ll continue calibration imaging of Mars for the rest of the month as it recedes into the distance.”

Bell also leads the Mastcam-Z imaging investigation on NASA’s Perseverance Mars rover mission team that was among several missions that provided complementary surface and atmospheric imaging, as well as navigation data, during the flyby to help with calibration efforts. Other missions involved include NASA’s Mars Reconnaissance Orbiter, the 2001 Mars Odyssey orbiter, and the Curiosity rover, along with the European Space Agency’s Mars Express and ExoMars Trace Gas Orbiter.

In addition to the imager, early calibration measurements made by Psyche’s magnetometers may have detected Mars’ bow shock as the spacecraft passed the planet. The gamma-ray and neutron spectrometer team was also quickly gathering data to calibrate the instrument by comparing their measurements with the large pool of existing Mars data.

With Mars in the rearview mirror, the spacecraft will soon resume using its solar-electric propulsion system to reach the main asteroid belt. When it arrives in August 2029, it will insert itself into orbit around the asteroid Psyche. It is thought to be the partial core of a planetesimal, a building block of an early planet. Through a series of circular orbits that go lower and then higher in altitude around Psyche, about 173 miles (280 kilometers) across at its widest point, the spacecraft will map the asteroid and gather science data.

If the asteroid proves to be the metallic core of an ancient planetesimal, it could offer a one-of-a-kind window into the interior of rocky planets like Earth.

“We’ve been anticipating the Mars flyby for years, but now it’s complete. We can thank the Red Planet for giving our spacecraft a critical gravitational slingshot farther into the solar system,” said Lindy Elkins-Tanton, principal investigator for Psyche at the University of California, Berkeley. “Onward to the asteroid Psyche!”

The Psyche mission is led by Arizona State University (ASU). A division of Caltech in Pasadena, JPL is responsible for the mission’s overall management, system engineering, integration and test, and mission operations. Intuitive Machines in Palo Alto, California, provided the high-power solar electric propulsion spacecraft chassis. The operations of the imager instrument are led by ASU, collaborating with Malin Space Science Systems in San Diego on the design, fabrication, and testing of the cameras.

Psyche is the 14th mission selected as part of NASA’s Discovery Program, managed by the agency’s Marshall Space Flight Center in Huntsville, Alabama. NASA’s Launch Services Program, based at NASA’s Kennedy Space Center in Florida, managed the launch service.

For more information about NASA’s Psyche mission, visit:

Credit: NASA/JPL-Caltech/ASU
Image Dates: May 15-16, 2026

#NASA #Space #Astronomy #Science #PsycheAsteroid #16Psyche #Asteroids #PsycheMission #PsycheSpacecraft #Planets #Mars #MarsFlyby #Jupiter #AsteroidBelt #SolarSystem #SpaceExploration #JPL #Caltech #ASU #UnitedStates #STEM #Education

China and Europe Just Launched a Historic Joint Solar Science Mission

China and Europe Just Launched a Historic Joint Solar Science Mission

The SMILE space mission has successfully launched on a mission to better understand space weather and how the Earth is protected from the Sun. This marks the first time the European Space Agency (ESA) and the Chinese Academy of Sciences have jointly designed, operated, and launched a mission. CGTN’s Wu Lei spoke to some of the Chinese scientists involved.

The European Space Agency-China SMILE satellite launched aboard a Vega-C rocket from Europe’s Spaceport in French Guiana. The rocket lifted off on at 04:52 BST / 05:52 CEST (00:52 local time) on May 19, 2026.

SMILE will use four science instruments to study how Earth responds to the solar wind from the Sun. In doing so, SMILE will improve our understanding of solar storms, geomagnetic storms and the science of space weather.

The European Space Agency (ESA) is 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 contributes to a second science instrument (the ultraviolet imager, UVI) and the mission operations once SMILE is in orbit.

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


Credit: European Space Agency (ESA)
Duration: 2 minutes
Release Date: May 19, 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

NASA CRS-34 Cargo Dragon Spacecraft Arrival | International Space Station

NASA CRS-34 Cargo Dragon Spacecraft Arrival | International Space Station

A SpaceX Dragon cargo spacecraft with its nose cone open to reveal its docking mechanism, approaches the International Space Station




NASA astronaut and Expedition 74 flight engineer Jack Hathaway is pictured inside the vestibule between the SpaceX Dragon cargo spacecraft and the International Space Station’s forward port on the Harmony module. Moments later, Hathaway would open the Dragon’s hatch and begin unloading nearly 6,500 pounds of food, supplies, and equipment for the Expedition 74 crew. 
International Space Station configuration as of May 17, 2026: Six spaceships are parked at the space station including the SpaceX CRS-34 Dragon, the SpaceX Crew-12 Dragon, Northrop Grumman’s Cygnus XL, the Soyuz MS-28 crew ship, and the Progress 94 and 95 resupply ships

Expedition 74 emblem

At 6:37 a.m. EDT on May 17, 2026, the SpaceX Dragon spacecraft docked to the forward port of the International Space Station’s Harmony module, carrying nearly 6,500 pounds of food, supplies, and equipment for the Expedition 74 crew. This is the 34th SpaceX commercial resupply services mission to the space station for NASA.

In addition to cargo for the crew aboard the space station, Dragon is delivering several new experiments, including a project  to determine how well Earth-based simulators mimic microgravity conditions, a bone scaffold made from wood that could produce new treatments for fragile bone conditions like osteoporosis, and equipment to help researchers evaluate how red blood cells and the spleen change in space. The Dragon spacecraft also will carry a new instrument to study charged particles around the Earth that can impact power grids and satellites, an investigation that could provide a fundamental understanding of how planets form, and an  instrument designed to take highly accurate measurements of sunlight reflected by Earth and the Moon.



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 Credits: NASA/Jessica Meir/Chris Williams, ESA/Sophie Adenot
Date: May 17, 2026


#NASA #Space #Science #ISS #Earth #CRS34Mission #SpaceX #CargoDragonSpacecraft #Astronauts #Cosmonauts #Russia #Roscosmos #ESA #Europe #HumanSpaceflight #InternationalCooperation #Expedition74 #SpaceLaboratory #MicrogravityExperiments #Florida #UnitedStates #STEM #Education

FU Orionis Star System in Orion (infrared) | NASA's Spitzer Space Telescope

FU Orionis Star System in Orion (infrared) | NASA's Spitzer Space Telescope


FU Orionis is a variable and binary star system in the constellation of Orion that in 1937 rose in apparent visual magnitude from 16.5 to 9.6, and has since been around magnitude 9. The name FU Orionis is a variable star designation in the Argelander system, assigned sequentially as new variables are discovered. FU Orionis is about 1,360 light years distant and is associated with the molecular cloud Barnard 35. The star itself is the brightest one in the image, glowing yellow given this particular processing and filter set, just to the lower left of center.

For a long time this variable was considered unique, but in 1970 a similar star, V1057 Cygni, was discovered, and a number of additional examples have been discovered since then. These stars represent the FU Orionis class of variable stars, GCVS type FU, often nicknamed FUors. These stars are pre–main sequence stars displaying extreme changes in magnitude and spectral type.

Also, visible here is Barnard 35, a dark nebula located in the constellation of Orion. It is a dense interstellar cloud of dust and gas that obscures the light from background stars, appearing as a prominent dark nebula against the brighter nebular regions of the Lambda Orionis Ring (also known as Sh 2-264). Discovered by astronomer E. E. Barnard in the early 20th century, Barnard 35 is part of the larger Orion molecular cloud complex and is associated with active star formation triggered by nearby massive stars.

The Spitzer Space Telescope, formerly the Space Infrared Telescope Facility (SIRTF), was an infrared space telescope that was active between 2003 and 2020. Spitzer was the third space telescope dedicated to infrared astronomy, following IRAS (1983) and ISO (1995–1998). It was the first spacecraft to use an Earth-trailing orbit, later used by the Kepler planet-finder.


The Jet Propulsion Laboratory (JPL) managed the Spitzer Space Telescope mission for NASA’s Science Mission Directorate in Washington until the mission was retired in January 2020. Science operations were conducted at the Spitzer Science Center at Caltech. Spacecraft operations were based at Lockheed Martin Space in Littleton, Colorado. Data are archived at the Infrared Science Archive operated by IPAC at Caltech. Caltech manages JPL for NASA.

For more information about Spitzer, visit:
https://www.nasa.gov/spitzer


Credit: Spitzer Space Telescope/NASA/JPL
Release Date: Feb. 7, 2020


#NASA #Astronomy #Space #Science #Stars #VariableStars #BinaryStarSystems #Nebulae #DarkNebulae #Barnard35 #FUOrionis #OrionConstellation #Cosmos #Universe #NASASpitzer #SpitzerSpaceTelescope #SST #InfraredAstronomy #JPL #Caltech #UnitedStates #STEM #Education

FU Orionis Star System in Orion | Hubble Space Telescope

FU Orionis Star System in Orion | Hubble Space Telescope

FU Orionis is a variable and binary star system in the constellation of Orion that in 1937 rose in apparent visual magnitude from 16.5 to 9.6, and has since been around magnitude 9. The name FU Orionis is a variable star designation in the Argelander system, assigned sequentially as new variables are discovered. FU Orionis is about 1,360 light years distant and is associated with the molecular cloud Barnard 35. The star itself is the brightest one in the image, glowing yellow given this particular processing and filter set, just to the lower left of center.

For a long time this variable was considered unique, but in 1970 a similar star, V1057 Cygni, was discovered, and a number of additional examples have been discovered since then. These stars represent the FU Orionis class of variable stars, GCVS type FU, often nicknamed FUors. These stars are pre–main sequence stars displaying extreme changes in magnitude and spectral type.

Also, visible here is Barnard 35, a dark nebula located in the constellation of Orion. It is a dense interstellar cloud of dust and gas that obscures the light from background stars, appearing as a prominent dark nebula against the brighter nebular regions of the Lambda Orionis Ring (also known as Sh 2-264). Discovered by astronomer E. E. Barnard in the early 20th century, Barnard 35 is part of the larger Orion molecular cloud complex and is associated with active star formation triggered by nearby massive stars.


Image Credit: NASA, ESA, Space Telescope Science Institute (STScI)
Processing: Judy Schmidt
Date: May 18, 2026

#NASA #ESA #Hubble #Astronomy #Space #Science #Stars #VariableStars #BinaryStarSystems #FUOrionis #Nebulae #DarkNebulae #Barnard35 #OrionConstellation #Cosmos #Universe #HST #HubbleSpaceTelescope #GSFC #STScI #JudySchmidt #UnitedStates #Europe #STEM #Education 

Europe-China SMILE Solar Science Mission Launch in South America

Europe-China SMILE Solar Science Mission Launch in South America










The European Space Agency-China SMILE satellite launched aboard a Vega-C rocket from Europe’s Spaceport in French Guiana. The rocket lifted off on at 04:52 BST / 05:52 CEST (00:52 local time) on May 19, 2026.

The Solar wind Magnetosphere Ionosphere Link Explorer (SMILE) launched on Vega-C flight VV29. At 35 meters (115 feet) tall, a Vega-C weighs 210 tonnes on the launch pad and the rocket used three solid-propellant-powered stages to take SMILE to orbit before the fourth liquid-propellant stage took over for a precise drop-off around Earth. SMILE is a joint mission between the European Space Agency (ESA) and the Chinese Academy of Sciences (CAS).

SMILE will use four science instruments to study how Earth responds to the solar wind from the Sun. In doing so, SMILE will improve our understanding of solar storms, geomagnetic storms and the science of space weather.

Kourou is a commune in French Guiana, an overseas region and department of France in South America. 

The Vega-C program is led by the European Space Agency (ESA), working with Avio as prime contractor and design authority.

The European Space Agency (ESA) is 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 contributes to a second science instrument (the ultraviolet imager, UVI) and the mission operations once SMILE is in orbit.

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


Credit: European Space Agency (ESA)
Dates: May 18-19, 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

Europe-China SMILE Solar Science Mission Launch in South America

Europe-China SMILE Solar Science Mission Launch in South America


The European Space Agency-China SMILE satellite launched aboard a Vega-C rocket from Europe’s Spaceport in French Guiana. The rocket lifted off on at 04:52 BST / 05:52 CEST (00:52 local time) on May 19, 2026.

The Solar wind Magnetosphere Ionosphere Link Explorer (SMILE) launched on Vega-C flight VV29. At 35 meters (115 feet) tall, a Vega-C weighs 210 tonnes on the launch pad and the rocket used three solid-propellant-powered stages to take SMILE to orbit before the fourth liquid-propellant stage took over for a precise drop-off around Earth. SMILE is a joint mission between the European Space Agency (ESA) and the Chinese Academy of Sciences (CAS).

SMILE will use four science instruments to study how Earth responds to the solar wind from the Sun. In doing so, SMILE will improve our understanding of solar storms, geomagnetic storms and the science of space weather.

Kourou is a commune in French Guiana, an overseas region and department of France in South America. 

The Vega-C program is led by the European Space Agency (ESA), working with Avio as prime contractor and design authority.

The European Space Agency (ESA) is 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 contributes to a second science instrument (the ultraviolet imager, UVI) and the mission operations once SMILE is in orbit.

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


Credit: European Space Agency (ESA)
Duration: 4 minutes
Release Date: May 19, 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

Moon & Planet Venus Conjunction: NASA Headquarters in Washington, D.C.

Moon & Planet Venus Conjunction: NASA Headquarters in Washington, D.C.





The Moon and planet Venus are seen in conjunction, Monday, May 18, 2026, from the Mary W. Jackson NASA Headquarters Building in Washington, District of Columbia. In astronomy, a conjunction refers to an event where two or more celestial bodies appear to meet or pass each other in the sky. A conjunction is an apparent phenomenon caused by an observer's perspective. However, the two objects involved are not actually close to one another in space.

Mary Jackson (born Winston; April 9, 1921–February 11, 2005) was an American mathematician and aerospace engineer at the National Advisory Committee for Aeronautics (NACA) that in 1958 was succeeded by the National Aeronautics and Space Administration (NASA). She worked at Langley Research Center in Hampton, Virginia, for most of her career. She started as a computer at the segregated West Area Computing division in 1951. "Human computers," were responsible for complex mathematical calculations and data processing. In 1958, after taking engineering classes, she became NASA's first black female engineer. African-American women computers played a vital role in advancing NASA projects, including the first American astronaut to orbit Earth in 1962. 

Mary Winston Jackson successfully overcame the barriers of segregation and gender bias to become a professional aerospace engineer and leader in ensuring equal opportunities for future generations.
Learn more about Mary W. Jackson:

Image Credit: NASA/Bill Ingalls
Date: May 18, 2026

#NASA #Astronomy #Space #Science #Skywatching #SolarSystem #Earth #Moon #Planets #Venus #Conjunction #History #MaryWJackson #AfricanAmericans #Women #Engineers #Computers #WashingtonDC #UnitedStates #NorthernHemisphere #Astrophotography #STEM #Education

Monday, May 18, 2026

NASA F-15 Aircraft Test Model Wing for Commercial Aviation Fuel Savings

NASA F-15 Aircraft Test Model Wing for Commercial Aviation Fuel Savings

NASA’s Crossflow Attenuated Natural Laminar Flow (CATNLF) project aims to lower fuel costs for future commercial aircraft by testing a scale-model wing designed to improve laminar flow. The project flew the scale-model wing on the bottom of a NASA F-15 research aircraft during a series of flight tests at NASA’s Armstrong Flight Research Center in Edwards, California. 

Learn more: https://www.nasa.gov/image-article/nasa-completes-first-flight-of-laminar-flow-scaled-wing-design/


Video Credits: NASA Armstrong Flight Research Center and NASA Langley Research Center
Duration: 6 minutes, 45 seconds
Release Date: May 18, 2026

#NASA #Aerospace #CommercialAviation #Aircraft #NASAF15 #NASAF15D #NASAF15Eagle #Science #Physics #Engineering #CivilianResearch #AeronauticalResearch #WingDesign #CATNLFProject #FlightTests #Boeing #McDonnellDouglas #NASAArmstrong #Edwards #California #NASALangley #Virginia #UnitedStates #STEM #Education #HD #Video

Spiral Galaxies NGC 3166 & NGC 3169 in Sextans | Mayall Telescope

Spiral Galaxies NGC 3166 & NGC 3169 in Sextans | Mayall Telescope

This image was obtained with the wide-field view of the Mosaic camera on the Mayall 4-meter telescope at Kitt Peak National Observatory. NGC 3166 (lower right) and NGC 3169 (upper left) are two spiral galaxies trapped in a death spiral. As these two galaxies begin to merge, they are starting to be pulled apart. The faint wisps surrounding NGC 3169 are its outer spiral arms being pulled off. Eventually these two galaxies will merge to form a single galaxy. NGC 3165, the small galaxy below NGC 3166, is also a member of this group. 

Distance from Earth: ~70 million light-years away

The image was generated with observations in the B (blue), V (green), I (orange) and Hydrogen-Alpha (red) filters. This image is rotated clockwise 30 degrees from north is up, east is to the left.

The Nicholas U. Mayall Telescope is a four-meter (158 inches) reflector telescope in Arizona named after the American observational astronomer of the same name. The telescope saw first light on February 27, 1973, and was the second-largest in the world at that time.

Learn more about the Mayall Telescope: 
https://noirlab.edu/science/programs/kpno/telescopes/nicholas-mayall-4m-telescope


Credit:T.A. Rector (University of Alaska Anchorage) and H. Schweiker (WIYN and NOIRLab/NSF/AURA)
Image Credit: June 30, 2020


#NASA #Astronomy #Space #Science #Galaxies #NGC3166 #NGC3169 #InteractingGalaxies #SextansConstellation #Cosmos #Universe #MayallTelescope #KPNO #Arizona #NSF #AURA #UnitedStates #STEM #Education

Antares & The Rho Ophiuchi Dark Cloud | Australian Astronomical Observatory

Antares & The Rho Ophiuchi Dark Cloud | Australian Astronomical Observatory

The dusty region between Ophiuchus and Scorpius contains examples of the most colorful and spectacular nebulae ever photographed. The upper part of the picture is filled with the bluish glow of light from hot stars reflected by a huge, cool cloud of dust and gas where such stars are born. This dust is also seen as a dark nebula, a molecular cloud, hiding the light of background stars, especially on middle left (east) of the picture.

Dominating the lower half of this cosmic landscape is the over-exposed image of the red supergiant star Antares, a star that it is steadily shedding material from its distended surface as it nears the end of its life. These tiny, smoke-like solid particles reflect Antares' light and hide it in a nebula of its own making. Antares and its nebula are about 600 light years away. Partly surrounding Sigma Scorpii (735 light years distant) at the right of the picture is a red emission nebula, completing the most comprehensive collection of nebular types ever seen in one photograph. There is also two globular clusters, one of the nearest to the sun, M4 (NGC 6121, 4500 light years away) at lower center right and NGC 6144, 28,000 light years away and much fainter, buried behind Antares' haze

Like all the images on these pages, this picture was made from three black and white glass negatives. Care has been taken to ensure that the colors are realistic.

Photograph made from plates taken in June 1979 (G,R), and July 1979 (B). Image width is about 3.5 degrees.


Image Credit: David Malin
Copyright: Australian Astronomical Observatory
Date: Aug. 15, 1979

#NASA #Space #Astronomy #Science #Nebulae #EmissionNebulae #Stars #StarClusters #GlobularClusters #Antares #NGC6144 #M4 #StellarNurseries #RhoOphiuchi #CloudComplex #SigmaScorpii #OphiuchusConstellation #Cosmos #Universe #Astronomers #DavidMalin #AustralianAstronomicalObservatory #Australia #STEM #Education

Planet Mars Images: May 15-17, 2026 | NASA's Curiosity & Perseverance Rovers

Planet Mars Images: May 15-17, 2026 | NASA's Curiosity & Perseverance Rovers

Mars 2020 - sol 1862
Mars 2020 - sol 1862
Mars 2020 - sol 1862
Mars 2020 - sol 1859
Mars 2020 - sol 1861
MSL - sol 4896
MSL - sol 4897
Mars 2020 - sol 1862

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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 15-17, 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 #STEM #Education

China Long March-8 Rocket Launches New Satellites for Spacesail Constellation

China Long March-8 Rocket Launches New Satellites for Spacesail Constellation

China launched a Long March-8 carrier rocket on May 17, 2026, in Hainan, sending a new satellite group into space. The rocket lifted off at 22:42 (Beijing Time) from the Hainan commercial spacecraft launch site. The satellite group, the ninth batch that will constitute the Spacesail (Qianfan) Constellation, entered the preset orbit successfully.

Qianfan is China's first giant low-orbit commercial satellite constellation to enter the formal networking phase. It will build a satellite Internet system that provides high-speed, real-time, secure, and reliable integrated solutions and services connecting space, air, ground and sea, independently constructed and operated by China. The project launched its first batch of satellites in August 2024 and aims to have a full operational network of more than 15,000 low-Earth orbit satellites in place by 2030. Qianfan is designed to support China's Belt and Road Initiative, providing secure digital links for Chinese businesses and infrastructure projects across the globe.

The Long March-8 rocket that carried out this mission is a member of the Long March 8 family. Together with the Long March-8A carrier rocket, the two models feature the payload capacity of 5 tonnes and 7 tonnes to sun-synchronous orbit, respectively. This underscores China's upgraded launch capabilities for deploying satellites into medium and low Earth orbits.

This year, the Long March 8 rockets will enter a high-density launch schedule, continuing to support the development of China's low-Earth orbit satellite Internet constellation and the high-quality development of the country's commercial space sector. 


Video Credit: CCTV
Duration: 24 seconds 
Release Date: May 18, 2026

#NASA #Space #Science #Earth #Satellites #SpaceSailConstellation #QianfanConstellation #千帆星座 #China #中国 #CNSA #中国国家航天局 #Rockets #LongMarch8Rockets #长征八号运载火箭  #MediumLiftRockets #CASC #SpaceTechnology #CommercialSpace #CommercialSpaceflight #Spaceports #Wenchang #Hainan #STEM #Education #HD #Video

Sunday, May 17, 2026

Aurora Australis Streams above Indian Ocean | International Space Station

Aurora Australis Streams above Indian Ocean | International Space Station


The aurora australis streams serenely above the Indian Ocean southwest of Perth, Australia, in this photograph taken at approximately 10:20 p.m. local time from the International Space Station as it orbited 268 miles above the Earth.

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.


Credit: ESA/Sophie Adenot
Date: May 7, 2026


#NASA #Space #Science #Astronomy #ISS #Earth #IndianOcean #Aurora #AuroraAustralis #Astronauts #Cosmonauts #Russia #Россия #Roscosmos #Роскосмос #HumanSpaceflight #InternationalCooperation #Expedition74 #SpaceLaboratory #MicrogravityExperiments #JSC #UnitedStates #ESA #Europe #STEM #Education

Star Cluster Westerlund 2 in Carina | Webb Telescope+Chandra X-ray Observatory

Star Cluster Westerlund 2 in Carina | Webb Telescope+Chandra X-ray Observatory

This image of Westerlund 2 features Chandra X-ray Observatory data (pink) and James Webb infrared data (red, orange, green, cyan, and blue). Scores of gleaming stars ringed in neon pink stretch across the frame, highlighting a cluster where stars are between one and three million years old. Brick-orange dust clouds along the bottom edge illustrate the raw materials of this active stellar nursery.

The cluster measures between 6 light-years and 13 light-years across, and is host to examples of our Milky Way galaxy's hottest, brightest, and most massive stars.


Credit: X-ray: NASA/CXC/SAO/Sejong Univ./Hur et al; JWST: ESA/Webb, NASA & CSA, V. Almendros-Abad, M. Guarcello, K. Monsch, and the EWOCS team
Image Processing: NASA/CXC/SAO/L. Frattare and K. Arcand
Release Date: May 15, 2026

#NASA #Space #Astronomy #Science #Stars #StarClusters #Westerlund2 #BrownDwarfs #Nebulae #Carina #Constellations #Astrophysics #Cosmos #Universe #JWST #MIRI #NIRCam #InfraredAstronomy #NASAChandra #XrayAstronomy #SpaceTelescopes #ESA #CSA #GSFC #STScI #CXC #UnitedStates #STEM #Education

Close-up: Star Cluster NGC 6380 in Scorpius | Hubble Space Telescope

Close-up: Star Cluster NGC 6380 in Scorpius | Hubble Space Telescope

This image shows the globular cluster NGC 6380. It lies around 35,000 light-years from Earth in the constellation Scorpio (The Scorpion). The very bright star at the top of the image is HD 159073, only around 4,000 light-years from Earth—making it a much nearer neighbor than NGC 6380. This image was taken with Hubble’s Wide Field Camera 3 (WFC3). As its name suggests, this instrument has a wide field of view, meaning that it can image relatively large areas of the sky in enormous detail.

NGC 6380 is not a particularly exciting name, but it indicates that this cluster is cataloged in the New General Catalog (NGC), originally compiled in 1888. This cluster has, however, been known by many other names. It was originally discovered by James Dunlop in 1826, and he rather immodestly named it Dun 538. Eight years later, in 1834, it was independently rediscovered by John Herschel and he (similarly immodestly) went on to name it H 3688. The cluster was re-rediscovered in 1959 in Paris by Pişmiş, who cataloged it as Tonantzintla 1—and to continue the pattern, also referred to it as Pişmiş 25. In addition to its colorful history of rediscovery, up until the 1950s NGC 6380 was thought to be an open cluster. It was A. D. Thackeray that realized that it was in fact a globular cluster. Nowadays, this cluster is reliably recognized in widely available catalogs as a globular cluster, and referred to simply as NGC 6380. 


Credit: ESA/Hubble & NASA, E. Noyola
Duration: 30 seconds
Date: July 12, 2021

#NASA #ESA #Hubble #Astronomy #Space #Science #Stars #StarClusters #GlobularClusters #NGC6380 #StarHD159073 #ScorpiusConstellation #Cosmos #Universe #HST #HubbleSpaceTelescope #GSFC #STScI #UnitedStates #Europe #STEM #Education #HD #Video

Rediscovered, Renamed, Reclassified: Star Cluster NGC 6380 in Scorpius | Hubble

Rediscovered, Renamed, Reclassified: Star Cluster NGC 6380 in Scorpius | Hubble


This image shows the globular cluster NGC 6380. It lies around 35,000 light-years from Earth in the constellation Scorpio (The Scorpion). The very bright star at the top of the image is HD 159073, only around 4,000 light-years from Earth—making it a much nearer neighbor than NGC 6380. This image was taken with Hubble’s Wide Field Camera 3 (WFC3). As its name suggests, this instrument has a wide field of view, meaning that it can image relatively large areas of the sky in enormous detail.

NGC 6380 is not a particularly exciting name, but it indicates that this cluster is cataloged in the New General Catalog (NGC), originally compiled in 1888. This cluster has, however, been known by many other names. It was originally discovered by James Dunlop in 1826, and he rather immodestly named it Dun 538. Eight years later, in 1834, it was independently rediscovered by John Herschel and he (similarly immodestly) went on to name it H 3688. The cluster was re-rediscovered in 1959 in Paris by Pişmiş, who cataloged it as Tonantzintla 1—and to continue the pattern, also referred to it as Pişmiş 25. In addition to its colorful history of rediscovery, up until the 1950s NGC 6380 was thought to be an open cluster. It was A. D. Thackeray that realized that it was in fact a globular cluster. Nowadays, this cluster is reliably recognized in widely available catalogs as a globular cluster, and referred to simply as NGC 6380. 


Credit: ESA/Hubble & NASA, E. Noyola
Date: July 12, 2021


#NASA #ESA #Hubble #Astronomy #Space #Science #Stars #StarClusters #GlobularClusters #NGC6380 #StarHD159073 #ScorpiusConstellation #Cosmos #Universe #HST #HubbleSpaceTelescope #GSFC #STScI #UnitedStates #Europe #STEM #Education

Expedition 74 Crew Photos: April-May 2026 | International Space Station

Expedition 74 Crew Photos: April-May 2026 | International Space Station

From left, Expedition 74 flight engineers Sophie Adenot of the European Space Agency and Jessica Meir of NASA pose for a portrait inside the International Space Station’s cupola on Mother’s Day. Adenot, who has a son, and Meir, who has a daughter, join hands to form a heart and wear T‑shirts celebrating motherhood.


European Space Agency astronaut and Expedition 74 flight engineer Sophie Adenot speaks to students on the ground using the International Space Station's ham radio. The ARISS, or Amateur Radio on the International Space Station, program gives students around the world the opportunity to talk directly with crew members aboard the orbital outpost, inspiring them to pursue careers in science, technology, engineering, and math.
European Space Agency astronaut and Expedition 74 flight engineer Sophie Adenot works inside the Kibo laboratory module’s Life Science Glovebox, processing blood stem cell samples to learn how to produce larger quantities of clinical‑grade stem cells in space. Results from this biotechnology investigation may lead to improved stem‑cell qualities, potentially enhancing treatments for blood diseases and cancer while also expanding commercial opportunities in space.
NASA astronaut and Expedition 74 flight engineer Jessica Meir works inside the International Space Station's Harmony module conducting a biotechnology investigation to observe how tiny, engineered materials that mimic DNA behave in microgravity. Meir pointed a light-measuring device, called a spectrophotometer, at the DNA-like sample materials housed in small transparent containers to analyze their ability to form stable structures. Doctors on Earth will use the research data to learn how to improve and develop future treatments, or nano-therapies, that target cancer cells more precisely.
NASA astronauts Jack Hathaway and Chris Williams, both Expedition 74 flight engineers prepare the NanoRacks External Platform—carrying three scientific payloads—for installation inside the Kibo laboratory module’s airlock where it will be placed outside in the vacuum of space. The payloads will test ultra‑high‑resolution hyperspectral imagery, measure radio signals passing through Earth’s ionosphere, and help doctors identify space‑sensitive proteins while evaluating mobility and neuromuscular health therapies. 

NASA astronaut and Expedition 74 flight engineer Chris Williams speaks to students on the ground using the International Space Station's ham radio. The ARISS, or Amateur Radio on the International Space Station, program gives students around the world the opportunity to talk directly with crew members aboard the orbital outpost, inspiring them to pursue careers in science, technology, engineering, and math.

NASA astronaut and Expedition 74 flight engineer Jack Hathaway installs the NanoRacks External Platform—carrying three scientific payloads—inside the Kibo laboratory module’s airlock for placement outside in the vacuum of space. The payloads will test ultra‑high‑resolution hyperspectral imagery, measure radio signals passing through Earth’s ionosphere, and help doctors identify space‑sensitive proteins while evaluating mobility and neuromuscular health therapies.

Station Update: At 6:37 a.m. EDT on May 17, 2026, the SpaceX Dragon spacecraft docked to the forward port of the International Space Station’s Harmony module, carrying nearly 6,500 pounds of food, supplies, and equipment for the Expedition 74 crew. This is the 34th SpaceX commercial resupply services mission to the space station for NASA.

In addition to cargo for the crew aboard the space station, Dragon is delivering several new experiments, including a project  to determine how well Earth-based simulators  mimic microgravity conditions, a bone scaffold made from wood that could produce new treatments for fragile bone conditions like osteoporosis, and equipment to help researchers evaluate how red blood cells and the spleen change in space. The Dragon spacecraft also will carry a new instrument to study charged particles around the Earth that can impact power grids and satellites, an investigation that could provide a fundamental understanding of how planets form, and an  instrument designed to take highly accurate measurements of sunlight reflected by Earth and the Moon.

The mission launched at 6:05 p.m. May 15 aboard a SpaceX Falcon 9 rocket from Cape Canaveral in Florida.

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: NASA's Johnson Space Center
Dates: April 18-May 13, 2026


#NASA #Space #Science #Astronomy #ISS #Earth #Astronauts #Cosmonauts #Russia #Россия #Roscosmos #Роскосмос #HumanSpaceflight #InternationalCooperation #Expedition74 #SpaceLaboratory #MicrogravityExperiments #JSC #UnitedStates #ESA #Europe #STEM #Education