Monday, June 12, 2023

Earth Satellites: The International Space Station & The Moon

Earth Satellites: The International Space Station & The Moon

What’s that near the Moon? It is the International Space Station (ISS). Although the ISS may appear to be physically near the Moon, it is not—it is physically closer to the Earth. In low Earth orbit and circulating around our big blue marble about every 90 minutes, the ISS was captured photographically as it crossed nearly in front of the Moon. The Moon, itself in a month-long orbit around the Earth, shows a crescent phase as only a curving sliver of its Sun-illuminated half is visible from the Earth. The featured image was taken in late March 2023 from Shanghai, China and shows not only details of Earth's largest human-made satellite, but details of the cratered and barren surface of Earth's largest natural satellite. Over the next few years, humanity is planning to send more people and machines to the Moon than ever before.


Image Credit & Copyright: Tianyao Yang

Image Date: March 2023

Capture Location: Shanghai, China

Release Date: June 12, 2023

#NASA #Space #Astronomy #Science #Earth #Satellites #Moon #ISS #Astronauts #HumanSpaceflight #Astrophotography #TianyaoYang #Astrophotographer #CitizenScience #Shanghai #上海 #China #中国 #STEM #Education #APoD

A Dishevelled Irregular Galaxy in Pegasus: NGC 7292 | Hubble

A Dishevelled Irregular Galaxy in Pegasus: NGC 7292 | Hubble


The galaxy NGC 7292 billows across this image from the NASA/European Space Agency  Hubble Space Telescope, accompanied by a handful of bright stars and the indistinct smudges of extremely distant galaxies in the background. It lies around 44 million light-years from Earth in the constellation Pegasus.

This slightly dishevelled galaxy is irregular, meaning that it lacks the distinct spiral arms of galaxies like the Whirlpool Galaxy or the smooth elliptical shape of galaxies like Messier 59. Unusually, its core is stretched out into a distinct bar, a feature seen in many spiral galaxies. Alongside its hazy shape, NGC 7292 is remarkably faint. As a result, astronomers classify NGC 7292 as a low surface brightness galaxy, barely distinguishable against the backdrop of the night sky. Such galaxies are typically dominated by gas and dark matter rather than stars.

Image Description: A galaxy fills up most of the frame from the right. It is fuzzy and diffuse, but made up of numerous tiny stars. In the core, the stars merge into a glowing bar shape. The gas and stars in the galaxy vary between warm and cool colors. They are spread over a large area, the colors mixing like clouds. The glow of the galaxy fades into a black background, with a few stars and small, distant galaxies.

Astronomers directed Hubble to inspect NGC 7292 during an observational campaign studying the aftermath of Type II supernovae. These colossal explosions happen when a massive star collapses and then violently rebounds in a catastrophic explosion that tears the star apart. Astronomers hope to learn more about the diversity of Type II supernovae they have observed by scrutinising the aftermath and remaining nearby stars of a large sample of historical Type II supernovae.

NGC 7292’s supernova was observed in 1964 and accordingly given the identifier SN 1964H. Studying the stellar neighbourhood of SN 1964H helps astronomers estimate the initial mass of the star that went supernova, and could uncover surviving stellar companions that once shared a system with the star that would become SN 1964H.


Credit: European Space Agency (ESA)/Hubble & NASA, C. Kilpatrick

Release Date: June 12, 2023


#NASA #ESA #Astronomy #Hubble #Space #Science #Galaxies #Galaxy #NGC7292 #Supernova #SN1964H #Pegasus #Constellation #Cosmos #Universe #HST #SpaceTelescope #GSFC #STScI #UnitedStates #Europe #STEM #Education

Sunday, June 11, 2023

The Clown-faced Nebula: NGC 2392 | Hubble Space Telescope

The Clown-faced Nebula: NGC 2392 | Hubble Space Telescope

The Clown-faced Nebula (NGC 2392) or Caldwell 39, is a bipolar double-shell planetary nebula (PN). It was discovered by astronomer William Herschel in 1787. It is surrounded by gas that composed the outer layers of a Sun-like star. The visible inner filaments are ejected by a strong wind of particles from the central star. The outer disk contains unusual, light-year-long filaments.

NGC 2392 lies about 6,500 light-years away, and is visible with a small telescope in the constellation of Gemini.

At the center of NGC 2392, there is an O-type star with a spectral type of O(H)6f.


Credit: NASA, European Space Agency (ESA), Andrew Fruchter (STScI), and the ERO team (STScI + ST-ECF)

Release Date: Jan. 24, 2000


#NASA #ESA #Astronomy #Space #Science #Hubble #Nebulae #Nebula #NGC2392 #ClownFacedNebula #PlanetaryNebula #Star #Gemini #Constellation #MilkyWayGalaxy #Cosmos #Universe #SpaceTelescope #GSFC #STScI #UnitedStates #Europe #STEM #Education

Earth View (1969) | NASA Apollo 12 Moon Mission

Earth View (1969) | NASA Apollo 12 Moon Mission

Apollo 12 Hasselblad image of the Earth's limb from film magazine 51/R - Orbital Image#AS12-51-7587

Some of the most breathtaking views of Earth taken from space are those that capture our planet’s limb. When viewed from the side, the Earth looks like a flat circle, and the atmosphere appears like a halo around it. This edge of the atmosphere is known as the limb.

Apollo 12 (November 14–24, 1969) was the sixth crewed flight in the United States Apollo program and the second to land on the Moon. It was launched on November 14, 1969, by NASA from the Kennedy Space Center, Florida. Commander Charles "Pete" Conrad and Lunar Module Pilot Alan L. Bean performed just over one day and seven hours of lunar surface activity while Command Module Pilot Richard F. Gordon remained in lunar orbit.


Image Credit: NASA's Johnson Space Center (JSC)/Project Apollo Archive

Processing: Kevin Gill

Kevin's Twitter Page: https://twitter.com/kevinmgill

Image Date: November 1969


#NASA #Space #Astronomy #Science #Planet #Earth #Atmosphere #Limb #Moon #ApolloProgram #Apollo12 #Astronauts #PeteConrad #AlanBean #RichardGordon #HumanSpaceflight #SolarSystem #SpaceExploration #History #Photography #HasselbladImage #STEM #Education

Saturn's Moon Titan: Thick Atmosphere with Rivers, Lakes & Seas | NASA Cassini

Saturn's Moon Titan: Thick Atmosphere with Rivers, Lakes & Seas | NASA Cassini

Titan at Saturn - May 2011
Titan at Saturn - May 2012
Titan & Dione at Saturn - May 2011
Titan & Dione at Saturn - May 2011
Tethys, Enceladus & Titan at Saturn - Oct. 2007
Saturn & Titan - May 2015

Saturn’s largest moon Titan is an extraordinary and exceptional world. Among our solar system’s more than 150 known moons, Titan is the only one with a substantial atmosphere. And of all the places in the solar system, Titan is the only place besides Earth known to have liquids in the form of rivers, lakes and seas on its surface.

Titan is larger than the planet Mercury and is the second largest moon in our solar system. Jupiter's moon Ganymede is just a little bit larger (by about 2 percent). Titan’s atmosphere is made mostly of nitrogen, like Earth’s, but with a surface pressure 50 percent higher than Earth’s. Titan has clouds, rain, rivers, lakes and seas of liquid hydrocarbons like methane and ethane. The largest seas are hundreds of feet deep and hundreds of miles wide. Beneath Titan’s thick crust of water ice is more liquid—an ocean primarily of water rather than methane. Titan’s subsurface water could be a place to harbor life as we know it, while its surface lakes and seas of liquid hydrocarbons could conceivably harbor life that uses different chemistry than we are used to—that is, life as we do not yet know it. 

The Cassini spacecraft ended its mission on Sept. 15, 2017. Cassini's end involved a series of close Saturn passes, approaching within the rings, then an entry into Saturn's atmosphere to destroy the spacecraft. This method was chosen because it is necessary to ensure protection and prevent biological contamination to any of the moons of Saturn thought to offer potential habitability.

For more information about the Cassini-Huygens mission visit: https://saturn.jpl.nasa.gov and www.nasa.gov/cassini

The Cassini-Huygens mission was a cooperative project of NASA, the European Space Agency and the Italian Space Agency. The Jet Propulsion Laboratory, a division of the California Institute of Technology in Pasadena, California, managed the mission for NASA's Science Mission Directorate, Washington, D.C. 


Image Credits: NASA/JPL-Caltech/Space Science Institute

Processing: Kevin M. Gill

Image Dates: 2007-2015


#NASA #Astronomy #Science #Space #Planet #Saturn #Moons #Titan #Dione #Enceladus #Tethys #Astrobiology #Atmosphere #Hydrocarbons #LiquidMethane #Water #H2O #Rivers #Lakes #Seas #Chemistry #SolarSystem #SpaceExploration #CassiniSpacecraft #CassiniMission #JPL #SSI #UnitedStates #History #STEM #Education

Planet Jupiter's Underground Ocean Moon Ganymede Close-up | NASA Juno Mission

Planet Jupiter's Underground Ocean Moon Ganymede Close-up | NASA Juno Mission







Jupiter’s moon Ganymede is proving to be a fascinating world. Not only is it the largest moon in our solar system, bigger than the planet Mercury and the dwarf planet Pluto, but NASA’s Hubble Space Telescope has found the best evidence yet for an underground saltwater ocean on Ganymede. The ocean is thought to have more water than all the water on Earth's surface. Ganymede’s ocean is estimated to be 60 miles (100 kilometers) thick—10 times deeper than Earth's ocean—and is thought to be buried under a 95-mile- (150-kilometer-) thick crust of mostly ice. Identifying liquid water is crucial in the search for habitable worlds beyond Earth and in the search for life as we know it. Ganymede is also the only moon in the Solar System to have a magnetosphere. 

The European Space Agency's JUICE Mission will arrive at Ganymede in 2031 to conduct investigations. 
Learn more about Europe's JUICE Mission: https://bit.ly/JuiceESAScience

NASA’s Jet Propulsion Laboratory, a division of Caltech in Pasadena, California, manages the Juno mission for the principal investigator, Scott J. Bolton, of the Southwest Research Institute in San Antonio. Juno is part of NASA’s New Frontiers Program, which is managed at NASA’s Marshall Space Flight Center in Huntsville, Alabama, for the agency’s Science Mission Directorate in Washington. Lockheed Martin Space in Denver built and operates the spacecraft.

More information about Juno:
https://www.nasa.gov/juno
and
https://www.missionjuno.swri.edu

Credit: NASA's Jet Propulsion Laboratory (JPL)/Caltech/Southwest Research Institute (SwRI)
Processing: Andrea Luck
Andrea's Twitter Page: https://twitter.com/andrluck
Release Dates: Jan. 1-2, 2022 

#NASA #Astronomy #Space #Science #Jupiter #Planet #Ganymede #Moon #Ocean #Astrobiology #Biosignatures #Habitability #Radiation #JunoMission #JunoSpacecraft #SolarSystem #SpaceExploration #JPL #Caltech #California #UnitedStates #CitizenScience #AndreaLuck #STEM #Education

Hubble’s Inside The Image: Eta Carinae—Great Eruption of a Massive Star

Hubble’s Inside The Image: Eta CarinaeGreat Eruption of a Massive Star

The Hubble Space Telescope has taken over 1.5 million observations over the years. One of them is the breathtaking image of Eta Carinae. Eta Carinae was the site of a giant outburst about 150 years ago, when it became one of the brightest stars in the southern sky. Though the star released as much visible light as a supernova explosion, it survived the outburst. Somehow, the explosion produced two polar lobes and a large thin equatorial disk, all moving outward at about 1.5 million miles per hour.

In this video, Dr. Keith Noll explains this breathtaking image and explains how important Hubble is to exploring the mysteries of the universe.


Credit: NASA's Goddard Space Flight Center (GSFC)

Producer & Director: James Leigh

Editor: Lucy Lund

Director of Photography: James Ball

Additional Editing & Photography: Matthew Duncan

Executive Producers: James Leigh & Matthew Duncan

Production & Post: Origin Films 

Duration: 2 minutes, 54 seconds

Release Date: June 10, 2023


#NASA #Space #Astronomy #Science #Hubble #Star #EtaCarinae #AGCarinae #Carina #Constellation #Astrophysics #Astronomer #KeithNoll #Physics #Cosmos #Universe #Telescope #GSFC #STScI #UnitedStates #ESA #Europe #STEM #Education #HD #Video

Saturday, June 10, 2023

Wide-field View: Star Cluster NGC 6520 & Dark Cloud Barnard 86 | ESO

Wide-field View: Star Cluster NGC 6520 & Dark Cloud Barnard 86 | ESO

This wide-field view shows the very rich star fields of the Large Sagittarius Star Cloud and the cluster NGC 6520 and the neighboring dark cloud Barnard 86. It was created from images from the Digitized Sky Survey 2.

Distance: 6,000 light years


Credit: European Southern Observatory (ESO)/Digitized Sky Survey 2

Acknowledgement: Davide De Martin

Release Date: Feb. 13, 2013


#NASA #ESO #Astronomy #Space #Science #Stars #StarCluster #NGC6520 #Nebulae #StarFormation #DarkCloud #Barnard86 #BokGlobule #Sagittarius #Constellation #MilkyWayGalaxy #Cosmos #Universe #Telescope #LaSillaObservatory #Chile #SouthAmerica #Europe #STEM #Education

Zooming into Star Cluster NGC 6520 & Dark Cloud Barnard 86 | ESO

Zooming into Star Cluster NGC 6520 & Dark Cloud Barnard 86 | ESO

This video sequence starts with a view of the spectacular Milky Way. As we zoom in towards the center we see a huge cloud of faint stars, this is the Large Sagittarius Star Cloud. On top of this cloud there is a much smaller dark feature called Barnard 86 and in the final view from the MPG/ESO 2.2-meter telescope at the European Southern Observatory's La Silla Observatory in Chile we see not only the gecko-shaped dark cloud but also its neighboring star cluster NGC 6520.

Credit: European Southern Observatory (ESO)/Digitized Sky Survey 2/Nick Risinger

Release Date: Feb. 14, 2013


#NASA #ESO #Astronomy #Space #Science #Stars #StarCluster #NGC6520 #Nebulae #StarFormation #DarkCloud #Barnard86 #BokGlobule #Sagittarius #Constellation #MilkyWayGalaxy #Cosmos #Universe #Telescope #LaSillaObservatory #Chile #SouthAmerica #Europe #STEM #Education #HD #Video

Infrared/visible-light Crossfade: Star Cluster NGC 6520 & Dark Cloud Barnard 86

Infrared/visible-light Crossfade: Star Cluster NGC 6520 & Dark Cloud Barnard 86

This sequence compares views of the region around the dark cloud Barnard 86 in infrared and visible light. The infrared view comes from the VISTA survey telescope and the visible light view is a new image from the MPG/ESO 2.2-meter telescope at the European Southern Observatory's La Silla Observatory in Chile. In the infrared, the cloud is more transparent and less prominent and the bright star cluster NGC 6520 becomes almost invisible.


Credit: European Southern Observatory (ESO)

Duration: 56 seconds

Release Date: Feb. 14, 2013


#NASA #ESO #Astronomy #Space #Science #Stars #StarCluster #NGC6520 #Nebulae #StarFormation #DarkCloud #Barnard86 #BokGlobule #Sagittarius #Constellation #MilkyWayGalaxy #Cosmos #Universe #VSTTelescope #VisibleLight #InfraredLight #LaSillaObservatory #Chile #SouthAmerica #Europe #STEM #Education #HD #Video

Panning across Star Cluster NGC 6520 & Dark Cloud Barnard 86 | ESO

Panning across Star Cluster NGC 6520 & Dark Cloud Barnard 86 | ESO

This pan video takes a close look at a new image from the Wide Field Imager on the MPG/ESO 2.2-meter telescope at the European Southern Observatory's La Silla Observatory in Chile, showing the bright star cluster NGC 6520 and its neighbor, the strangely shaped dark cloud Barnard 86. This cosmic pair is set against millions of glowing stars from the brightest part of the Milky Way—a region so dense with stars that barely any dark sky is seen across the picture.

Distance: 6,000 light years


Credit: European Southern Observatory (ESO)

Duration: 36 seconds

Release Date: Feb. 14, 2013


#NASA #ESO #Astronomy #Space #Science #Stars #StarCluster #NGC6520 #Nebulae #StarFormation #DarkCloud #Barnard86 #BokGlobule #Sagittarius #Constellation #MilkyWayGalaxy #Cosmos #Universe #Telescope #LaSillaObservatory #Chile #SouthAmerica #Europe #STEM #Education #HD #Video

Bright Star Cluster NGC 6520 & Strangely Shaped Dark Cloud Barnard 86 | ESO

Bright Star Cluster NGC 6520 & Strangely Shaped Dark Cloud Barnard 86 | ESO

This image from the Wide Field Imager on the MPG/ESO 2.2-meter telescope at the European Southern Observatory’s La Silla Observatory in Chile, shows the bright star cluster NGC 6520 and its neighbor, the strangely shaped dark cloud Barnard 86. This cosmic pair is set against millions of glowing stars from the brightest part of the Milky Way—a region so dense with stars that barely any dark sky is seen across the picture.

Distance: 6,000 light years


Credit: European Southern Observatory (ESO)

Release Date: Feb. 13 2013


#NASA #ESO #Astronomy #Space #Science #Stars #StarCluster #NGC6520 #Nebulae #StarFormation #DarkCloud #Barnard86 #BokGlobule #Sagittarius #Constellation #MilkyWayGalaxy #Cosmos #Universe #Telescope #LaSillaObservatory #Chile #SouthAmerica #Europe #STEM #Education

International Students Visit World's Largest Single-dish Radio Telescope in China

International Students Visit World's Largest Single-dish Radio Telescope in China

"I didn't expect the telescope can be so gigantic." Forty international students recently visited China's five-hundred-meter Aperture Spherical Radio Telescope (FAST), the world's largest single-dish radio telescope, constructed in 2016. Fast radio bursts, or FRBs, are one of the greatest mysteries of our universe. FAST has already reported the largest set of FRB events ever detected in history. For example, between August and October 2019, the Five-Hundred-Meter Aperture Spherical Radio Telescope (FAST) in southwestern China recorded a total of 1,652 such brief and bright outbursts from a single repeating FRB source in a dwarf galaxy three billion light years away. 

“The study is very thorough, with a level of details and sensitivity we’ve never had before,” says astrophysicist Emily Petroff from the University of Amsterdam in the Netherlands and McGill University in Canada

Coming from deep space, these fast radio bursts can flash and fade in a matter of milliseconds, yet in each instance can release as much energy as the sun does in a year. They pop up all across the sky multiple times a day, but most appear to be one-off events and are thus hard to catch. First discovered in 2007, FRBs have challenged and tantalized scientists seeking to uncover their obscure origins and to use them as unique tools for probing the depths of intergalactic space.

The primary driving force behind the FAST project was Nan Rendong, a researcher with the Chinese National Astronomical Observatory, part of the Chinese Academy of Sciences. He held the positions of chief scientist and chief engineer of the project. He died September 15, 2017, in Boston due to lung cancer.

Learn more about FAST in China: 


Credit: New China TV

Acknowledgements: Scientific American Magazine

Duration: 1 minute, 20 seconds

Release Date: June 10, 2023


#NASA #Space #Astronomy #Science #Pulsars #FRB #FastRadioBursts #RadioTelescope #FAST #五百米口径球面射电望远镜 #Tianyan #Guizhou #China #NanRendong #CNAO #Scientist #Engineer #Researcher #CAS #STEM #Education #Students #History #HD #Video

El astronauta Frank Rubio habla con el Museo Nacional del Latino Estadounidense

El astronauta Frank Rubio habla con el Museo Nacional del Latino Estadounidense

En un evento en directo desde la Estación Espacial Internacional, el astronauta Frank Rubio conversó con el Museo Nacional del Latino Estadounidense el 18 de mayo de 2023.  Rubio respondió preguntas de estudiantes e hizo algunas demostraciones de movimiento en microgravedad. La conexión, que se llevó a cabo en inglés, lleva subtítulos en español en este video. 

Astronaut Frank Rubio’s Official NASA Biography:

https://www.nasa.gov/astronauts/biographies/frank-rubio/biography/


Credit: NASA's Johnson Space Center (JSC)

Duration: 20 minutes

Release Date: June 9, 2023


#NASA #Space #ISS #Earth #Astronauts #FrankRubio #LatinoAmerican #Doctor #Physician #FlightSurgeon #Cosmonauts #Роскосмос #Russia #Россия #UAE #MBRSC #Science #HumanSpaceflight #Expedition69 #JSC #UnitedStates #MicrogravityResearch #Students #ArtemisGeneration #STEM #Education #HD #Video

NASA Crews Spray Foam Insulation on Artemis III Moon Rocket Hardware

NASA Crews Spray Foam Insulation on Artemis III Moon Rocket Hardware

Teams at NASA’s Marshall Space Flight Center in Huntsville, Alabama, have completed applying a spray-on foam insulation to the launch vehicle stage adapter (LVSA) for the Artemis III mission. The LVSA is a cone-shaped piece of hardware that connects the SLS (Space Launch System) rocket’s upper and lower stages and partially encloses the engine of the interim cryogenic propulsion stage. The spray-on foam insulation is a type of thermal protection system that is used to protect the Moon rocket’s hardware from the extreme temperatures, forces, and sounds it will experience during launch and ascent. Unlike other parts of the mega rocket, the thermal protection system for the LVSA is applied entirely by hand using a tool similar to a spray gun. It is the largest piece of SLS hardware to be hand sprayed. Teams started applying the thermal protection system in March 2023.

The LVSA in this video will be used for Artemis III, the mission that will land the first woman and first person of color on the lunar surface. The LVSA is fully manufactured at Marshall by NASA, lead contractor Teledyne Brown Engineering, and the Jacobs Space Exploration Group’s ESSCA contract. 

Learn more about SLS: nasa.gov/sls


Video Credit: NASA's Marshall Space Flight Center (MSFC)

Duration: 1 minute, 25 seconds

Release Date: June 9, 2023


#NASA #Space #Moon #Artemis #ArtemisIII #Rocket #SLS #SpaceLaunchSystem #Boeing #MoonRocket #LVSA #TeledyneBrownEngineering #DeepSpace #MoonToMars #Astronauts #Science #Engineering #Technology #SpaceExploration #SolarSystem #NASAMarshall #MSFC #Hunstville #Alabama #UnitedStates #STEM #Education #HD #Video

Planet Jupiter and Ocean Moon Ganymede | NASA Cassini Mission

Planet Jupiter and Ocean Moon Ganymede | NASA Cassini Mission

Jupiter’s moon Ganymede is proving to be a fascinating world. Not only is it the largest moon in our solar system, bigger than the planet Mercury and the dwarf planet Pluto, but NASA’s Hubble Space Telescope has found the best evidence yet for an underground saltwater ocean on Ganymede. The ocean is thought to have more water than all the water on Earth's surface. Ganymede’s ocean is estimated to be 60 miles (100 kilometers) thick—10 times deeper than Earth's ocean—and is thought to be buried under a 95-mile- (150-kilometer-) thick crust of mostly ice. Identifying liquid water is crucial in the search for habitable worlds beyond Earth and in the search for life as we know it.

The Cassini spacecraft ended its mission on Sept. 15, 2017. Cassini's end involved a series of close Saturn passes, approaching within the rings, then an entry into Saturn's atmosphere to destroy the spacecraft. This method was chosen because it is necessary to ensure protection and prevent biological contamination to any of the moons of Saturn thought to offer potential habitability.

For more information about the Cassini-Huygens mission visit: https://saturn.jpl.nasa.gov and www.nasa.gov/cassini

The Cassini-Huygens mission was a cooperative project of NASA, the European Space Agency and the Italian Space Agency. The Jet Propulsion Laboratory, a division of the California Institute of Technology in Pasadena, California, managed the mission for NASA's Science Mission Directorate, Washington, D.C. 


Image Credit: NASA/JPL-Caltech/SpaceScienceInstitute/AndreaLuck

Andrea Luck on Twitter: https://bit.ly/3Cn9jmo 

Image Date: Jan. 6, 2001


#NASA #Astronomy #Science #Space #Planet #Jupiter #Moon #Ganymede #Astrobiology #OceanWorld #WaterIce #SolarSystem #SpaceExploration #CassiniSpacecraft #CassiniMission #JPL #SSI #UnitedStates #History #STEM #Education