Wednesday, May 20, 2026

NASA's Artemis II Moon Crew Visits the U.S. Capitol

NASA's Artemis II Moon Crew Visits the U.S. Capitol

On May 12, 2026, NASA astronauts Christina Koch, Reid Wiseman, and Victor Glover, and Canadian Space Agency (CSA) astronaut Jeremy Hansen visited Capitol Hill in Washington, D.C., where they met U.S. senators and representatives and spoke about their historic mission around the Moon.

NASA's Artemis II Mission took Wiseman, Glover, Koch, and Hansen on a nearly 10-day journey around the Moon and back to Earth.

The Orion spacecraft successfully splashed down on Friday, April 10, 2026, in the Pacific Ocean following its journey around the Moon.

The first crewed test flight of NASA’s Artemis Program lifted off from Launch Pad 39B at the agency’s Kennedy Space Center in Florida on April 1, 2026, carrying the first astronauts to travel to the Moon in more than half a century. 

The crew completed a record-setting lunar flyby, taking them 252,756 miles at their farthest distance from Earth and 4,067 miles above the lunar surface at their closest approach. 

Under Artemis, NASA will send astronauts on increasingly difficult missions to explore more of the Moon for scientific discovery, economic benefits, and to build on our foundation for the first crewed missions to Mars.

Learn more about NASA's Artemis II Mission:
https://www.nasa.gov/mission/artemis-ii/


Credit: NASA
Duration: 1 minute
Release Date: May 20, 2026


#NASA #Space #Science #Earth #Moon #ArtemisProgram #ArtemisII #OrionSpacecraft #Astronauts #ReidWiseman #VictorGlover #ChristinaKoch #JeremyHansen #CSA #Canada #HumanSpaceflight #SolarSystem #SpaceExploration #WashingtonDC #USCapitol #UnitedStates #STEM #Education #HD #Video

Wide-field view: The Pleiades Star Cluster | Australian Astronomical Observatory

Wide-field view: The Pleiades Star Cluster | Australian Astronomical Observatory

The Pleiades are one of the finest and nearest examples of a reflection nebula associated with a cluster of young stars. The cluster itself is a group of many hundreds of stars about 400 light years away in the direction of the northern constellation of Taurus. A handful of the brightest stars cluster together in space and have been recognized as a group since ancient times. However, even the brightest of the Pleiades stars (Alcyone, apparent visual mag +2.9) is relatively faint and would be inconspicuous (and nameless) if it were not a member of the cluster The faintest named star is Asterope, (V = +5.8), close to the threshold of naked eye visibility. All the visible stars of the Pleiades are in reality much more luminous than the Sun.

The nebulosity seen here is light reflected from the particles in a cloud of cold gas and dust this cluster has drifted into. It appears blue because these tiny motes of interstellar dust scatter blue light more efficiently than the longer wavelengths of red light, and it is streaky because of the distribution of dust particles in space. Care has been taken to ensure that the colors visible here are realistic.

In western literature and legend, the stars bear the names of the Seven Sisters, the daughters of Atlas and Pleone. They were also half-sisters to the goddesses of the nearby Hyades stars. The delicate beauty of the stars identified them as a group of women in many cultures, from Australian Aborigine to Native American. To the Japanese they are 'Subaru', a conglomerate or collection (i.e. cluster), while Chinese legends refer to a swarm of bees. Maori and Pacific Islands people often called the Pleiades 'Matariki', the star cluster that heralds the start of the Maori New Year.

Photograph made from plates taken in 1983 October (G) and December (B, R). Image width is about 3.5 degrees.


Image Credit: David Malin
Copyright: Australian Astronomical Observatory
Release Date: April 15,
2000

#NASA #Space #Astronomy #Science #Nebulae #ReflectionaNebulae #Stars #StarClusters #ThePleiades #SevenSisters #Messier45 #M45 #OpenStarCluster #BrownDwarfStars #TaurusConstellation #Cosmos #Universe #Astronomers #DavidMalin #AustralianAstronomicalObservatory #Australia #STEM #Education

The Pleiades Star Cluster in Taurus | Australian Astronomical Observatory

The Pleiades Star Cluster in Taurus | Australian Astronomical Observatory

The Pleiades are one of the finest and nearest examples of a reflection nebula associated with a cluster of young stars. The cluster itself is a group of many hundreds of stars about 400 light years away in the direction of the northern constellation of Taurus. A handful of the brightest stars cluster together in space and have been recognized as a group since ancient times. However, even the brightest of the Pleiades stars (Alcyone, apparent visual mag +2.9) is relatively faint and would be inconspicuous (and nameless) if it were not a member of the cluster The faintest named star is Asterope, (V = +5.8), close to the threshold of naked eye visibility. All the visible stars of the Pleiades are in reality much more luminous than the Sun.

The nebulosity seen here is light reflected from the particles in a cloud of cold gas and dust this cluster has drifted into. It appears blue because these tiny motes of interstellar dust scatter blue light more efficiently than the longer wavelengths of red light, and it is streaky because of the distribution of dust particles in space. Care has been taken to ensure that the colors visible here are realistic.

In western literature and legend, the stars bear the names of the Seven Sisters, the daughters of Atlas and Pleone. They were also half-sisters to the goddesses of the nearby Hyades stars. The delicate beauty of the stars identified them as a group of women in many cultures, from Australian Aborigine to Native American. To the Japanese they are 'Subaru', a conglomerate or collection (i.e. cluster), while Chinese legends refer to a swarm of bees. Maori and Pacific Islands people often called the Pleiades 'Matariki', the star cluster that heralds the start of the Maori New Year.

Photograph made from plates taken in October 1983 (G) and December (B, R). Image width is about 100 arc min.


Image Credit: David Malin
Copyright: Australian Astronomical Observatory
Date: Aug. 17, 1984

#NASA #Space #Astronomy #Science #Nebulae #ReflectionaNebulae #Stars #StarClusters #ThePleiades #SevenSisters #Messier45 #M45 #OpenStarCluster #BrownDwarfStars #TaurusConstellation #Cosmos #Universe #Astronomers #DavidMalin #AustralianAstronomicalObservatory #Australia #STEM #Education

Distant Irregular Galaxy NGC 2719 & Companion in Lynx | Hubble Space Telescope

Distant Irregular Galaxy NGC 2719 & Companion in Lynx | Hubble Space Telescope

NGC 2719 is a Magellanic irregular galaxy in the constellation of Lynx. A Magellanic spiral galaxy has only one spiral arm. The long galaxy is NGC 2719 and the smaller one is NGC 2719A. NGC 2719 was discovered by German-British astronomer William Herschel on March 28, 1786. Together with the galaxy NGC 2719A (also known as PGC 2528A), NGC 2719 is listed in Halton Arp's Atlas of Peculiar Galaxies as Arp 202. The galaxy pair is also listed as Holm 105 in Erik Holmberg's A Study of Double and Multiple Galaxies Together with Inquiries into some General Metagalactic Problems, published in 1937.

Distance from Earth: ~159 million light-years

Image Processor Judy Schmidt: "They're an interacting pair, and the smaller one seems to have a rather long string of stars trailing it, visible at the lower right edge of the image. The stream itself is difficult to see, but does connect. Luckily, the stream just made it onto the detector. You can see a tiny sliver of a blank spot at the lower right corner."


Image Credit: NASA, ESA, Space Telescope Science Institute (STScI)
Processing: Judy Schmidt
Release Date: Sept. 15, 2025

#NASA #ESA #Hubble #Astronomy #Space #Science #Galaxies #InteractingGalaxies #NGC2719 #Arp202 #NGC2719A #PGC2528A #Holm105 #LynxConstellation #Cosmos #Universe #HST #HubbleSpaceTelescope #GSFC #STScI #JudySchmidt #UnitedStates #Europe #STEM #Education

STEMonstrations: Distribution of Mass | International Space Station

STEMonstrations: Distribution of Mass | International Space Station

Have you ever kicked a soccer ball and wondered why it curves, spins, or sometimes wobbles? 

NASA astronaut Jessica Meir aboard the International Space Station explains the science hidden inside every ball. Engineers carefully design soccer balls so they fly smoothly whether they are being kicked in your backyard or in the World Cup.

We are engaging students in NASA’s exciting missions, broad range of careers, and unique opportunities. Join us as we apply science, technology, engineering, and mathematics to explore space, improve aeronautics, examine Earth, and strive to land the next humans on the Moon with the Artemis Program.

NASA STEM resources: https://www.nasa.gov/learning-resources/

Science, Technology, Engineering, Math (STEM) Education


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.


Video Credit: NASA's Johnson Space Center
Duration: 3 minutes, 21 seconds
Release Date: May 19, 2026


#NASA #Space #Science #ISS #Earth #Soccer #Mass #Motion #Physics #Astronauts #Cosmonauts #Russia #Roscosmos #ESA #Europe #HumanSpaceflight #InternationalCooperation #Expedition74 #SpaceLaboratory #MicrogravityExperiments #Florida #UnitedStates #STEM #Education #HD #Video

A Supercharged Supernova Discovered | NASA’s Fermi Gamma-ray Space Telescope

A Supercharged Supernova Discovered | NASA’s Fermi Gamma-ray Space Telescope

Gamma rays detected by NASA’s Fermi Gamma-ray Space Telescope gave scientists a look under the hood of a rare supernova that produced much more light than normal. 

The Fermi Gamma-ray Space Telescope (FGST), formerly called the Gamma-ray Large Area Space Telescope (GLAST), is a space observatory being used to perform gamma-ray astronomy observations from low Earth orbit. Its main instrument is the Large Area Telescope (LAT). This is being used to perform an all-sky survey studying astrophysical and cosmological phenomena, such as active galactic nuclei, pulsars, other high-energy sources and dark matter. Another instrument aboard Fermi, the Gamma-ray Burst Monitor (GBM), is being utilized to study gamma-ray bursts and solar flares.

Fermi, named for high-energy physics pioneer Enrico Fermi, was launched in 2008. The mission is a joint venture of NASA, the United States Department of Energy, and government agencies in France, Germany, Italy, Japan, and Sweden. It is the most sensitive gamma-ray telescope on orbit, succeeding INTEGRAL. The project is a recognized CERN experiment (RE7).


Credit: NASA's Goddard Space Flight Center/Scientific Visualization Studio
Sophia Roberts (eMITS): Lead Producer
Francis Reddy (University of Maryland College Park): Lead Writer
Jonathan North (eMITS): Lead Animator
Elizabeth Hays (NASA/GSFC): Scientist
Fabio Acero (University of Saclay): Scientist
Duration: 1 minute, 46 seconds
Release Date: May 20, 2026

#NASA #Astronomy #Space #Science #Stars #NeutronStars #Magnetars #Supernovae #GammaRays #Astrophysics #Fermi #FGST #SpaceTelescopes #Cosmos #Universe #GSFC #DOE #UnitedStates #Europe #Japan #STEM #Education #HD #Video

SpaceX Starship and Super Heavy Version 3 Moved to Launchpad at Starbase Texas

SpaceX Starship and Super Heavy Version 3 Moved to Launchpad at Starbase Texas








Starship and Super Heavy V3 have been moved to the pad at Starbase Texas for final testing and preparations for launch. "These vehicles are the first of many—made possible by the tireless effort of SpaceX engineers and technicians—and are designed to enable the core revolutionary capabilities of Starship."

As of October 13, 2025, the SpaceX Starship has been "launched 11 times with 6 successes and 5 failures." SpaceX has developed Starship with the intention of lowering launch costs using economies of scale. It aims to achieve this by reusing both rocket stages, increasing payload mass to orbit, increasing launch frequency, creating a mass-manufacturing pipeline and adapting it to a wide range of space missions.

NASA plans to use a lunar lander version of Starship for landing astronauts on the Moon during the Artemis IV mission through the Human Landing System (HLS) program.

Learn more about Starship:

Download the Free Starship User Guide (PDF):

Credit: Space Exploration Technologies Corporation (SpaceX)
Release Date: May 19, 2026

#NASA #SpaceX #Space #Earth #Mars #Moon #MoonToMars #ArtemisProgram #ArtemisIII #ArtemisIV #Starship #StarshipV3 #StarshipFlight12 #ReusableSpacecraft #SuperHeavy #SuperHeavyV3 #ElonMusk #Engineering #SpaceTechnology #HumanSpaceflight #CommercialSpace #SpaceExploration #StarbaseTexas #Texas #UnitedStates #STEM #Education

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

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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