NASA Psyche Mission Mars Flyby Highlights | JPL
Image Dates: May 15-16, 2026
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NASA Psyche Mission Mars Flyby Highlights | JPL
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.
NASA CRS-34 Cargo Dragon Spacecraft Arrival | International Space Station
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
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.
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.
Europe-China SMILE Solar Science Mission Launch in South America
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.
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.
Europe-China SMILE Solar Science Mission Launch in South America
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.
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.
Moon & Planet Venus Conjunction: NASA Headquarters in Washington, D.C.
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/
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
#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
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.
#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
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.
Aurora Australis Streams above Indian Ocean | International Space Station
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
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.
Close-up: Star Cluster NGC 6380 in Scorpius | Hubble Space Telescope
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.