Friday, September 23, 2022

A 3D Panning on Massive Star Cluster NGC 3603 (Artist's Impression) | Hubble

A 3D Panning on Massive Star Cluster NGC 3603 (Artist's Impression) | Hubble

A pan on NGC 3603 (artist's impression).

Distance: 20,000 light years


Credit: European Space Agency (ESA) /Hubble (M. Kornmesser & L. L. Christensen)

Duration: 38 seconds

Release Date: February 17, 2016


#NASA #ESA #Astronomy #Space #Hubble #Stars #NGC3603 #StarCluster #Carina #Constellation #Cosmos #Universe #SpaceTelescope #GSFC #STScI #UnitedStates #Europe #STEM #Education #Art #Visualization #HD #Video

Zooming in on Massive Compact Star Cluster in NGC 3603 | Hubble

Zooming in on Massive Compact Star Cluster in NGC 3603 | Hubble

Starting from the magnificent vista of the southern Milky Way we gradually zoom in on the huge star formation region NGC 3603 ending with an extreme close-up of the core of the central star cluster taken with the Wide Field Planetary Camera 2 (WFPC2) camera on the NASA/ESA Hubble Space Telescope.

Credit: NASA, ESA and Wolfgang Brandner (MPIA), Boyke Rochau (MPIA) and Andrea Stolte (University of Cologne)

Acknowledgement: Robert Gendler, Martin Pugh, Astromania de Yave

Duration: 1 minute

Release Date: February 17, 2016


#NASA #ESA #Astronomy #Space #Hubble #Stars #NGC3603 #StarCluster #Carina #Constellation #Cosmos #Universe #SpaceTelescope #GSFC #STScI #UnitedStates #Europe #STEM #Education #HD #Video

Extreme Star Cluster NGC 3603 Bursts into Life | Hubble

Extreme Star Cluster NGC 3603 Bursts into Life | Hubble

The star-forming region NGC 3603 contains one of the most impressive massive young star clusters in the Milky Way. Bathed in gas and dust the cluster formed in a huge rush of star formation thought to have occurred around a million years ago. The hot blue stars at the core are responsible for carving out a huge cavity in the gas seen to the right of the star cluster in NGC 3603's center.


Credit: NASA, European Space Agency and the Hubble Heritage (STScI/AURA)-ESA/Hubble Collaboration

Release Date: October 2, 2007


#NASA #ESA #Astronomy #Space #Hubble #Stars #NGC3603 #StarCluster #Carina #Constellation #Cosmos #Universe #SpaceTelescope #GSFC #STScI #UnitedStates #Europe #STEM #Education

Pan of Massive Star Cluster NGC 346 | Hubble

Pan of Massive Star Cluster NGC 346 | Hubble

Astronomers have been bemused to find young stars spiralling into the center of a massive cluster of stars in the Small Magellanic Cloud, a satellite galaxy of the Milky Way. The outer arm of the spiral in this huge, oddly shaped stellar nursery—called NGC 346—may be feeding star formation in a river-like motion of gas and stars. The massive star cluster NGC 346, located in the Small Magellanic Cloud, has long intrigued astronomers with its unusual shape. Only 150 light-years in diameter, NGC 346 boasts the mass of 50,000 Suns. Its intriguing shape and rapid star formation rate has puzzled astronomers.


Credit: NASA, European Space Agency (ESA), N. Bartmann   

Release Date: September 8, 2022


#NASA #ESA #Hubble #Astronomy #Space #Science #Stars #StarCluster #NGC346 #SmallMagellanicCloud #SMC #Galaxy #Cosmos #Universe #SpaceTelescope #STScI #GSFC #UnitedStates #Europe #STEM #Education #HD #Video

NASA's Space to Ground: Flying Turtles | Week of Sept. 23, 2022

NASA's Space to Ground: Flying Turtles | Week of Sept. 23, 2022

NASA's Space to Ground is your weekly update on what's happening aboard the International Space Station. Ten people are now living aboard the International Space Station with the arrival of three new crewmates inside a Soyuz crew ship on Wednesday. The new crew members from NASA and Roscosmos will spend the next several days getting up to speed with living and working in space.

New flight engineers Frank Rubio from NASA and Dmitri Petelin from Roscosmos are beginning their first space mission with veteran cosmonaut Sergey Prokopyev, who is on his second space station mission. The trio blasted off at 9:54 a.m. EDT on Wednesday, September 21, 2022, to the orbiting lab inside the Soyuz MS-22 spacecraft from Kazakhstan. The threesome docked to the Rassvet module less than three-and-a-half hours later. They waited a couple of more hours after leak and pressure checks before opening the spacecraft hatch and entering the station to begin lab familiarization activities ahead of a six-month mission.

Late next week, three cosmonauts who have been residing on the space station since March 18, will end their mission and return to Earth. Commander Oleg Artemyev and Flight Engineers Denis Matveev and Sergey Korsakov will board the Soyuz MS-21 crew ship, undock from the Prichal module, reenter Earth’s atmosphere, and parachute to a landing in Kazakhstan.

European Space Agency (ESA) astronaut Samantha Cristoforetti will take over as station commander from Artemyev before he departs during the traditional Change of Command ceremony next week. The leadership change will be seen live on NASA TV, the agency’s app, and its website at 9:35 a.m. on Sept. 28.


Credit: NASA's Johnson Space Center (JSC)

Duration: 3 minutes

Release Date: September 23, 2022


#NASA #Space #ISS #Earth #Science #Roscomos #Роскосмос #SoyuzMS22 #Spacecraft #Cosmonauts #SergeyProkopyev #DmitriPetelin #Astronaut #FrankRubio #HumanSpaceflight #Expedition68 #Russia #Россия #Europe #Italia #Italy #Canada #Japan #日本 #JSC #UnitedStates #STEM #Education #HD #Video

Thursday, September 22, 2022

Star Cluster in The Large Magellanic Cloud | Hubble

Star Cluster in The Large Magellanic Cloud | Hubble


This image shows an open cluster known as NGC 2164, which was first discovered in 1826 by a Scottish astronomer named James Dunlop. NGC 2164 is located within one of the Milky Way galaxy's closest neighbors—the satellite galaxy known as the Large Magellanic Cloud. The Large Magellanic cloud is a relatively small galaxy that lies about 160,000 light-years from Earth. It is considered a satellite galaxy because it is gravitationally bound to the Milky Way. In fact, the Large Magellanic Cloud is on a very slow collision course with the Milky Way—it is predicted that they will collide 2.4 billion years from now.

The Large Magellanic Cloud only contains about one hundredth as much mass as the Milky Way, but it still contains billions of stars. The open cluster NGC 2164 is in good company in the Large Magellanic Cloud—the satellite galaxy is home to roughly 700 open clusters, alongside about 60 globular clusters. This image of NGC 2164 was taken by the NASA/European Space Agency Hubble Space Telescope’s Wide Field Camera 3 (WFC3), which has previously imaged many other open clusters, including NGC 330 and Messier 11.


Credit: European Space Agency (ESA)/Hubble & NASA, J. Kalirai, A. Milone

Release Date: August 23, 2021


#NASA #ESA #Astronomy #Space #Science #Hubble #Stars #OpenStarCluster #StarCluster #NGC2164 #Dorado #Constellation #LMC #Galaxy #Cosmos #Universe #SpaceTelescope #STScI #GSFC #UnitedStates #Europe #Astronomer #JamesDunlop #History #STEM #Education

Capturing the Spectacular Outflow from Spiral Galaxy Markarian 817 | Hubble

Capturing the Spectacular Outflow from Spiral Galaxy Markarian 817 | Hubble

Rings of brilliant blue stars encircle the bright, active core of this spiral galaxy, whose monster black hole is blasting material into space at over 14 million kilometers per hour. Viewed nearly face-on, the galaxy, called Markarian 817, shows intense star-forming regions and dark bands of interstellar dust along its spiral arms.

Distance: 450 million light years

Observations by the new Cosmic Origins Spectrograph (COS) aboard the NASA/European Space Agency Hubble Space Telescope captured the powerful outflow of material from this galaxy.

The COS spectrum of Markarian 817 highlights the outflow's dynamic nature. A gas cloud containing hydrogen that was detected in Hubble data taken in 1997 does not appear in the COS observation because the cloud has apparently been driven out by an outflow of material from the galaxy.

This discharge is being powered by a huge disc of matter encircling the supermassive black hole, which is 40 million times more massive than our Sun. The disc is driving the material out of the galaxy through powerful winds, produced by streams of charged particles. Some of the outflow rains back onto the galaxy. The rest settles into the intergalactic gas.

Astronomers want to know how much of the outflow lands in the galaxy and how much escapes into intergalactic space. To achieve this, they need high-quality spectroscopic observations to detect the signatures of the outflowing material, which includes carbon, nitrogen and oxygen. This will allow them to determine the composition, location and dynamics of the winds that distribute the material.

Markarian 817 is 430 million light-years away in the northern constellation of Draco. COS observed the galaxy on August 4, 2009, using its far-ultraviolet detector to distinguish the outflow from the galaxy’s core. NASA astronauts installed COS during Servicing Mission 4 in May 2009 to upgrade and repair the Hubble.

The Hubble image was taken with the Wide Field Camera 3 on August 2, 2009. The composite image was made by using filters that isolate light from the blue, green and infrared portions of the spectrum, as well as emission from glowing hydrogen.

The Hubble observations are part of the Hubble Servicing Mission 4 Early Release Observations.


Credit: NASA, European Space Agency (ESA) and the Hubble SM4 ERO Team

Release Date: September 9, 2009


#NASA #ESA #Astronomy #Space #Science #Hubble #Galaxy #Spiral #Markarian817 #BlackHole #Outflow #Draco #Constellation #LMC #Galaxy #Cosmos #Universe #SpaceTelescope #STScI #GSFC #UnitedStates #Europe #STEM #Education

Probing a Super-giant Shell of Gas and Stars: LH 72 | Hubble

Probing a Super-giant Shell of Gas and Stars: LH 72 | Hubble


In one of the largest known star formation regions in the Large Magellanic Cloud (LMC), a small satellite galaxy of the Milky Way, lie young and bright stellar groupings known as OB associations. One of these associations, called LH 72, was captured in this dramatic NASA/European Space Agency Hubble Space Telescope image. It consists of a few high-mass, young stars embedded in a beautiful and dense nebula of hydrogen gas.

Distance: 170,000 light years

Much of the star formation in the LMC occurs in super-giant shells. These regions of interstellar gas are thought to have formed due to strong stellar winds and supernova explosions that cleared away much of the material around the stars creating wind-blown shells. The swept-up gas eventually cools down and fragments into smaller clouds that dot the edges of these regions and eventually collapse to form new stars.

The biggest of these shells, home to LH 72, is designated LMC4. With a diameter of about 6,000 light-years, it is the largest in the Local Group of galaxies that is home to both the Milky Way and LMC. Studying gas-embedded young associations of stars like LH 72 is a way of probing the super-giant shells to understand how they formed and evolved.

This image was taken with Hubble’s Wide Field Planetary Camera 2 using five different filters in ultraviolet, visible and infrared light. The field of view is approximately 1.8 by 1.8 arcminutes.


Credit: European Space Agency (ESA)/Hubble, NASA and D. A. Gouliermis

Release Date: November 21, 2011


#NASA #ESA #Astronomy #Space #Science #Hubble #Stars #StarFormation #OBAssociations #Nebula #LH72 #LMC4 #Dorado #Constellation #LMC #Galaxy #Cosmos #Universe #SpaceTelescope #STScI #GSFC #UnitedStates #Europe #STEM #Education

Space Shuttle Endeavour Gets a Piggyback Ride | NASA's Johnson Space Center

Space Shuttle Endeavour Gets a Piggyback Ride | NASA's Johnson Space Center


10-Year Anniversary: Our Shuttle Carrier Aircraft ferries the Space Shuttle Endeavour over the Johnson Space Center in Houston in this Sept. 20, 2012, image. Endeavour’s end destination was the California Science Center, where it sits on display. The shuttle Endeavour brought the first parts of the International Space Station to space and completed 25 missions.

On its final flight to the California Science Center 10 years ago, Endeavour was escorted by a combination of F/A-18s and an F-15 from NASA’s Armstrong Flight Research Center in Edwards, California. Those aircraft were flown by NASA Armstrong pilots, while center photographers and videographers documented the orbiter’s final journey.


Image Credit: NASA/Robert Markowitz

Caption Credit: Monika Luabeya

Release Date: September 22, 2022


#NASA #Space #Science #Endeavour #STS #SpaceShuttle #Spacecraft #Boeing747 #Aircraft #Aerospace #Engineering #Technology #HumanSpaceflight #JSC #Houston #Texas #UnitedStates #History #STEM #Education 

Space Shuttle Endeavour’s Last Flight 10 Years Ago | NASA

Space Shuttle Endeavour’s Last Flight 10 Years Ago | NASA Armstrong

People from communities all over California watched the skies in hopes of catching a glimpse of space shuttle Endeavour as it was ferried on the NASA 747 Shuttle Carrier Aircraft to Los Angeles on Sept. 21, 2012.

On its final flight to the California Science Center, Endeavour was escorted by a combination of F/A-18s and an F-15 from NASA’s Armstrong Flight Research Center in Edwards, California. Those aircraft were flown by NASA Armstrong pilots, while center photographers and videographers documented the orbiter’s final journey.

Included on the space shuttle’s flight path were many California landmarks such as the California State Capitol Building, Disneyland, Dodger Stadium, the Getty Center, the Golden Gate Bridge, and the Hollywood sign. Also on the route were the Los Angeles Memorial Coliseum, NASA’s Ames Research Center, NASA’s Jet Propulsion Laboratory in Pasadena, and the Santa Monica Pier.


Credit: NASA's Armstrong Flight Research Center

Duration: 5 minutes

Release Date: September 21, 2022


#NASA #Space #Science #Endeavour #STS #SpaceShuttle #Spacecraft #Boeing747 #Aircraft #Aerospace #Engineering #Technology #HumanSpaceflight #CaliforniaScienceCenter #LosAngeles #AFRC #EdwardsAirForceBase #California #UnitedStates #STEM #Education #History #HD #Video

Pan on the Star-forming Region LH 95 in the Large Magellanic Cloud | Hubble

Pan on the Star-forming Region LH 95 in the Large Magellanic Cloud | Hubble

This video shows a star forming region in the Large Magellanic Cloud (LMC). It reveals a large number of low-mass infant stars coexisting with young massive stars.


Credit: European Space Agency (ESA)/Hubble (M. Kornmesser & L. L. Christensen)

Duration: 28 seconds

Release Date: August 14, 2006


#NASA #ESA #Astronomy #Space #Science #Hubble #Stars #StarFormation #Nebula #LH95 #Dorado #Constellation #LMC #Galaxy #Cosmos #Universe #SpaceTelescope #STScI #GSFC #UnitedStates #Europe #STEM #Education #SD #Video

Zoom on the Star-forming Region LH 95 in the Large Magellanic Cloud | Hubble

Zoom on the Star-forming Region LH 95 in the Large Magellanic Cloud | Hubble

This video shows a star forming region in the Large Magellanic Cloud (LMC). It reveals a large number of low-mass infant stars coexisting with young massive stars.


Credit: European Space Agency (ESA)/Hubble (M. Kornmesser & L. L. Christensen)
Duration: 30 seconds
Release Date: August 14, 2006


#NASA #ESA #Astronomy #Space #Science #Hubble #Stars #StarFormation #Nebula #LH95 #Dorado #Constellation #LMC #Galaxy #Cosmos #Universe #SpaceTelescope #STScI #GSFC #UnitedStates #Europe #STEM #Education #SD #Video

Revisiting Large & Small Stars in Harmonious Coexistence | ESO

Revisiting Large & Small Stars in Harmonious Coexistence | ESO


Part of the Large Magellanic Cloud (LMC) centered on LH 95. This image is a color composite taken by the Digitized Sky Survey (DSS), the field of view is 3.0x2.7 degrees.

Distance: 170,000 light years


Credit: Davide De Martin (European Space Agency/Hubble), the ESA/ESO/NASA FITS Liberator & Digitized Sky Survey 2

Release Date: August 14, 2006


#NASA #ESA #Astronomy #Space #Science #Hubble #Stars #StarFormation #Nebula #LH95 #Dorado #Constellation #LMC #Galaxy #Cosmos #Universe #SpaceTelescope #STScI #GSFC #UnitedStates #Europe #STEM #Education

Expedition 68 Crew: Launch Day | International Space Station

Expedition 68 Crew: Launch Day | International Space Station








Scenes from Launch Day: Expedition 68 astronaut Frank Rubio of NASA and his crewmates, Sergey Prokopyev and Dmitri Petelin of Roscosmos successfully launched onboard their Soyuz MS-22 spacecraft, Wednesday, Sept. 21, 2022, in Baikonur, Kazakhstan, and safely arrived later at the International Space Station. Their Soyuz spacecraft bore the name of Konstantin Tsiolkovsky, the “father” of cosmonautics. 

Rubio, Prokopyev, and Petelin will spend approximately six months on the orbital complex, returning to Earth in March 2023. 

Astronaut Frank Rubio’s Official NASA Biography:

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

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. The ISS has been the most politically complex space exploration program ever undertaken.

Credit: NASA/Bill Ingalls/Victor Zelentsov

Image Date: Sept. 21, 2022


#NASA #ISS #Earth #Science #Soyuz  #Союз #Rocket #Launch #Roscomos #Роскосмос #СоюзMS22 #SoyuzMS22 #Spacecraft #Cosmonauts #Commander #SergeyProkopyev #DmitriPetelin #Russia #Россия #Astronaut #FrankRubio #UnitedStates #JSC #BaikonurCosmodrome #Kazakhstan #Қазақстан #Human #Spaceflight #Expedition68 #STEM #Education

Center of The Milky Way: Wide-field View | ESO

Center of The Milky Way: Wide-field View | ESO


This visible light wide-field view shows the rich star clouds in the constellation of Sagittarius (the Archer) in the direction of the center of our Milky Way galaxy. The entire image is filled with vast numbers of stars—but far more remain hidden behind clouds of dust and are only revealed in infrared images. This view was created from photographs in red and blue light and form part of the Digitized Sky Survey 2. The field of view is approximately 3.5 degrees x 3.6 degrees.

Distance: 25,000 light years


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

Acknowledgment: Davide De Martin and S. Guisard

Release Date: May 12, 2022


#NASA #ESO #Astronomy #Space #Science #BlackHole #SagittariusA #SagittariusAAsterisk #Sagittarius #Constellation #MilkyWay #Galaxy #Cosmos #Universe #Telescope #Chile #Europe #STEM #Education

Hot Gas Bubble Swirling Around Our Supermassive Black Hole | ESO

Hot Gas Bubble Swirling Around Our Supermassive Black Hole | ESO

ESOcast 256 Light: Using the Atacama Large Millimeter/submillimeter Array (ALMA), astronomers have found a hot bubble of gas that swirls around Sagittarius A*, the black hole at the center of our galaxy, at 30% of the speed of light.


Credit: European Southern Observatory (ESO)

Directed by: Herbert Zodet and Martin Wallner

Editing: Herbert Zodet

Web and technical support: Gurvan Bazin and Raquel Yumi Shida

Written by: Rebecca Forsberg and Rory Harris

Footage and photos: ESO, Event Horizon Telescope (EHT) Collaboration, M. Kornmesser, L. Calçada (Acknowledgment: M. Wielgus), Jordy Davelaar et al./Radboud University/BlackHoleCam, ALMA (ESO/NAOJ/NRAO) and C. Malin

Scientific consultant: Mariya Lyubenova

Release Date: September 22, 2022

Duration: 1 minute, 27 seconds


#NASA #ESO #ALMA #EHT #Astronomy #Space #Science #GasBubble #BlackHole #SagittariusA #SagittariusAAsterisk #MilkyWay #Galaxy #Cosmos #Universe #Telescope #Chile #Europe #Infographics #STEM #Education #HD #Video