Friday, August 05, 2022

NASA Previews Artemis I Moon Mission

NASA Previews Artemis I Moon Mission

Mission experts for NASA's Artemis I mission around the Moon reviewed the details and mission timeline—from pre-launch to splashdown—of the four-to-six-week flight test that will demonstrate the capabilities of the Space Launch System (SLS) Moon rocket and Orion capsule. 

Briefing participants:

• Debbie Korth, Orion program deputy manager, NASA Johnson

• Rick LaBrode, lead Artemis I flight director, NASA Johnson

• Judd Frieling, Artemis I ascent/entry flight director, NASA Johnson

• Melissa Jones, Artemis I recovery director, NASA Kennedy

• Reid Wiseman, chief astronaut, NASA Johnson

• Philippe Deloo, Orion European Service Module program manager, ESA (European Space Agency)

Currently targeted to launch no earlier than Monday, Aug. 29, 2022, the SLS rocket will send the uncrewed Orion spacecraft around the Moon and back to Earth to check out spacecraft systems before crew fly aboard on Artemis II. The Artemis I mission is one more step toward taking the next giant leap: sending the first astronauts to Mars.


More info on this historic mission: https://nasa.gov/specials/artemis-i


Credit: National Aeronautics and Space Administration (NASA)

Duration: 1 hour, 33 minutes

Release Date: August 5, 2022


#NASA #ESA #Space #Moon #MSFC #Artemis #ArtemisI #Orion #Spacecraft #SLS #NASASLS #SpaceLaunchSystem #Rocket #DeepSpace #Astronauts #Mars #MoonToMars #JourneyToMars #Science #Engineering #Technology #Exploration #SolarSystem #UnitedStates #Europe #STEM #Education #HD #Video

NASA’s Curiosity Rover Turns 10: Here’s What It’s Learned

NASA’s Curiosity Rover Turns 10: Here’s What It’s Learned 

Mars News Report Aug. 5, 2022: NASA’s Curiosity Mars rover set out to answer a big question when it landed on the Red Planet 10 years ago: Could Mars have supported ancient life? Scientists have discovered the answer is yes and have been working to learn more about the planet’s past habitable environment.

In this Mars Report, Curiosity Deputy Project Scientist Abigail Fraeman provides an update on the rover’s capabilities a decade after landing in Gale Crater. Now, Curiosity is heading to an area that may help answer how long ancient life could have persisted on the Red Planet as Mars went through significant changes in the climate.

Some of the images in this video include color enhancement that exaggerate small changes in color from place to place in the Martian scene. This makes it easier for the science team to use their everyday experience to interpret the landscape. For instance, the sky on Mars would not actually look blue to a human explorer on the Red Planet, but pinkish.

For more information on NASA's Mars missions, visit mars.nasa.gov


Credit: NASA/JPL-Caltech/ASU/MSSS/JHU-APL

Duration: 3 minutes, 41 seconds

Release Date: August 5, 2022


#NASA #Space #Astronomy #Science #Mars #RedPlanet #Planet #Astrobiology #Geology #Environment #Climate #TenthAnniversary #MountSharp #GaleCrater #Curiosity #Rover #MSL #Robotics #Technology #JPL #California #UnitedStates #JourneyToMars #STEM #Education #HD #Video

Crab Nebula: Multiwavelength Structure of a Pulsar Wind Nebula | Hubble & More

Crab Nebula: Multiwavelength Structure of a Pulsar Wind Nebula | Hubble & More

This visualization features a three-dimensional multiwavelength representation of the Crab Nebula, a pulsar wind nebula that is the remains of an exploded star. This video is based on images from NASA’s three Great Observatories: the Chandra X-ray Observatory and the Hubble and Spitzer Space Telescopes.

The video begins by showing the Crab Nebula in context, pinpointing the location of the observed supernova in the constellation Taurus. This view zooms in to present the Hubble, Spitzer, and Chandra images of the Crab Nebula, each highlighting one of the nested structures in the system.

The video then begins a slow buildup of the three-dimensional X-ray structure, showing the pulsar and disk of energized material, and adding jets of particles firing off from opposite sides of the energetic dynamo.

Appearing next is a rotating infrared view of a glowing cloud of emission, called synchrotron radiation, enveloping the pulsar system. This distinctive form of radiation occurs when streams of charged particles spiral around the pulsar’s magnetic field lines.

The visible-light outer shell of the Crab Nebula appears next. Looking like a cage around the entire system, this shell of glowing gas consists of tentacle-shaped filaments of ionized oxygen. The tsunami of particles unleashed by the pulsar is pushing on this expanding debris cloud like an animal rattling its cage.

The X-ray, infrared, and visible-light models are combined at the end of the video to reveal both a rotating three-dimensional multiwavelength view and the corresponding two-dimensional multiwavelength image of the Crab Nebula.


Credit: NASA, ESA, F. Summers, J. Olmsted, L. Hustak, J. DePasquale, G. Bacon (STScI), N. Wolk (CfA|H&S/CXC), R. Hurt (Caltech/IPAC)

Duration: 3 minutes, 43 seconds

Release Date: January 5, 2020


#NASA #ESA #Astronomy #Space #Hubble #Star #NeutronStar #Nebula #SupernovaRemnant #CrabNebula #NGC1952 #Taurus #Constellation #Cosmos #Universe #SpaceTelescope #Chandra #Spitzer #SpaceTelescope #GSFC #STScI #UnitedStates #Europe #STEM #Education #Visualization #HD #Video

The Crab Nebula: Multiwavelength View | Hubble

The Crab Nebula: Multiwavelength View | Hubble

Astronomers have produced a highly detailed image of the Crab Nebula, by combining data from telescopes spanning nearly the entire breadth of the electromagnetic spectrum, from radio waves seen by the Karl G. Jansky Very Large Array (VLA) to the powerful X-ray glow as seen by the orbiting Chandra X-ray Observatory. And, in between that range of wavelengths, the Hubble Space Telescope's crisp visible-light view, and the infrared perspective of the Spitzer Space Telescope.

The Crab Nebula, the result of a bright supernova explosion seen by Chinese and other astronomers in the year 1054, is 6,500 light-years from Earth. At its center is a super-dense neutron star, rotating once every 33 milliseconds, shooting out rotating lighthouse-like beams of radio waves and light — a pulsar (the bright dot at image center). The nebula's intricate shape is caused by a complex interplay of the pulsar, a fast-moving wind of particles coming from the pulsar, and material originally ejected by the supernova explosion and by the star itself before the explosion.

This image combines data from five different telescopes: the VLA (radio) in red; Spitzer Space Telescope (infrared) in yellow; Hubble Space Telescope (visible) in green; XMM-Newton (ultraviolet) in blue; and Chandra X-ray Observatory (X-ray) in purple.

The new VLA, Hubble, and Chandra observations all were made at nearly the same time in November 2012. A team of scientists led by Gloria Dubner of the Institute of Astronomy and Physics (IAFE), the National Council of Scientific Research (CONICET), and the University of Buenos Aires in Argentina then made a thorough analysis of the newly revealed details in a quest to gain new insights into the complex physics of the object. They are reporting their findings in the Astrophysical Journal.

"Comparing these new images, made at different wavelengths, is providing us with a wealth of new detail about the Crab Nebula. Though the Crab has been studied extensively for years, we still have much to learn about it," Dubner said.

The Hubble Space Telescope is a project of international cooperation between NASA and ESA (European Space Agency). NASA’s Goddard Space Flight Center in Greenbelt, Maryland, manages the telescope. The Space Telescope Science Institute (STScI) in Baltimore conducts Hubble science operations. STScI is operated for NASA by the Association of Universities for Research in Astronomy, Inc., in Washington, D.C.

NASA’s Marshall Space Flight Center in Huntsville, Alabama, manages the Chandra program for NASA’s Science Mission Directorate in Washington, D.C. The Smithsonian Astrophysical Observatory in Cambridge, Massachusetts, controls Chandra’s science and flight operations.

NASA’s Jet Propulsion Laboratory, Pasadena, California, manages the Spitzer Space Telescope for NASA’s Science Mission Directorate, Washington, D.C. Science operations are conducted at the Spitzer Science Center at Caltech in Pasadena, California. Spacecraft operations are based at Lockheed Martin Space Systems Company, Littleton, Colorado. Data are archived at the Infrared Science Archive housed at the Infrared Processing and Analysis Center at Caltech. Caltech manages JPL for NASA.

The National Radio Astronomy Observatory (NRAO) is a facility of the National Science Foundation, operated under cooperative agreement by Associated Universities, Inc.


Credits: NASA, European Space Agency, G. Dubner (IAFE, CONICET-University of Buenos Aires) et al.; A. Loll et al.; T. Temim et al.; F. Seward et al.; VLA/NRAO/AUI/NSF; Chandra/CXC; Spitzer/JPL-Caltech; XMM-Newton/ESA; and Hubble/STScI

Release Date: May 10, 2017


#NASA #ESA #Astronomy #Space #Hubble #Nebula #CrabNebula #NGC1952 #Taurus #Constellation #Cosmos #Universe #Chandra #Spitzer #VLA #XMMNewton #SpaceTelescope #GSFC #STScI #UnitedStates #Europe #STEM #Education

Zoom into The Crab Nebula: Detailed View | Hubble

Zoom into The Crab Nebula: Detailed View | Hubble

This video zooms in on a detailed Crab Nebula image—one of the largest ever taken with Hubble's WFPC2 camera. It was assembled from 24 individual exposures taken with the NASA/European Space Agency Hubble Space Telescope and was the highest resolution image of the entire Crab Nebula ever made in 2005.

Distance: 6,500 light years


Credit: NASA, European Space Agency, and G. Bacon of the Space Telescope Science Institute (STScI)

Release Date: December 31, 2014

Duration: 30 seconds


#NASA #ESA #Astronomy #Space #Hubble #Star #NeutronStar #Nebula #SupernovaRemnant #CrabNebula #NGC1952 #Taurus #Constellation #Cosmos #Universe #SpaceTelescope #GSFC #STScI #UnitedStates #Europe #STEM #Education #HD #Video


The Crab Nebula: Detailed View | Hubble

The Crab Nebula: Detailed View | Hubble


This Hubble image provides a highly detailed view of the entire Crab Nebula. The Crab is among the most interesting and well studied objects in astronomy. The Crab is among the most interesting and well studied objects in astronomy.

This image is one of the largest ever taken with Hubble's WFPC2 camera. It was assembled from 24 individual exposures taken with the NASA/European Space Agency Hubble Space Telescope and was the highest resolution image of the entire Crab Nebula ever made in 2005.


Credit: NASA, European Space Agency and Allison Loll/Jeff Hester (Arizona State University) Acknowledgement: Davide De Martin (ESA/Hubble)

Release Date: December 1, 2005


#NASA #ESA #Astronomy #Space #Hubble #Star #NeutronStar #Nebula #CrabNebula #NGC1952 #Taurus #Constellation #Cosmos #Universe #SpaceTelescope #GSFC #STScI #UnitedStates #Europe #STEM #Education

Zooming in on The Crab Nebula | Hubble

Zooming in on The Crab Nebula | Hubble

This video zooms into part of the sky in the constellation of Taurus (The Bull) ending on the inner parts of the famous Crab Nebula, a supernova remnant.

Distance: 6,500 light years


Credit: European Space Agency/Hubble, Digitized Sky Survey, Nick Risinger

Music: Johan Monell

Release Date: July 7, 2016


#NASA #ESA #Astronomy #Space #Hubble #Star #NeutronStar #Nebula #SupernovaRemnant #CrabNebula #NGC1952 #Taurus #Constellation #Cosmos #Universe #SpaceTelescope #GSFC #STScI #UnitedStates #Europe #STEM #Education #HD #Video

Moving Heart of The Crab Nebula | Hubble

Moving Heart of The Crab Nebula | Hubble


While many other images of the famous Crab Nebula have focused on the filaments in the outer part of the nebula, this image shows the very heart of the Crab Nebula including the central neutron star—it is the rightmost of the two bright stars near the center of this image.

The rapid motion of the material nearest to the central star is revealed by the subtle rainbow of colors in this time-lapse image, the rainbow effect being due to the movement of material over the time between one image and another.


Credit: European Space Agency/Hubble & NASA

Acknowledgement: Mahdi Zamani

Release Date: July 7, 2016


#NASA #ESA #Astronomy #Space #Hubble #Star #NeutronStar #Nebula #CrabNebula #NGC1952 #Taurus #Constellation #Cosmos #Universe #SpaceTelescope #GSFC #STScI #UnitedStates #Europe #STEM #Education

NASA's Space to Ground: The Gateway Connection | Week of August 5, 2022

NASA's Space to Ground: The Gateway Connection Week of August 5, 2022

NASA's Space to Ground is your weekly update on what's happening aboard the International Space Station. 

NASA's Gateway Program: 

https://www.nasa.gov/gateway

Learn more about the important research being operated on Station:

https://www.nasa.gov/iss-science 

For more information about STEM on Station:

https://www.nasa.gov/stemonstation

Science, Technology, Engineering, Math (STEM)


Credit: NASA's Johnson Space Center (JSC)

Release Date: August 5, 2022

Duration: 10 minutes, 16 seconds


#NASA #Space #Earth #ISS #Aretmis #Moon #Gateway #SpaceXCrew5 #SpaceX #Astronauts #Research #Laboratory #Science #Technology #HumanSpaceflight #Europe #Russia #Россия #Japan #日本 #Canada #UnitedStates #Expedition67 #STEM #Education #HD #Video

Thursday, August 04, 2022

Panning across The Skull & Crossbones Nebula | ESO

Panning across The Skull & Crossbones Nebula | ESO

This pan video explores a vivid active star forming region—NGC 2467, otherwise known as the Skull and Crossbones Nebula. This image of dust, gas and bright young stars, gravitationally bound into the form of a grinning skull, was captured with the FORS instrument on the European Southern Observatory’s Very Large Telescope (VLT). Whilst ESO’s telescopes are usually used for the collection of science data, their immense resolving power makes them ideal for capturing images such as this—which are beautiful for their own sake.

Distance: 4,500 light years


Credit: European Southern Observatory (ESO)

Duration: 25 seconds

Release Date: November 7, 2018


#NASA #ESO #Astronomy #Space #Stars #Nebula #SkullCrossbonesNebula #NGC2467 #Puppis #Constellation #Cosmos #Universe #Telescope #VLT #Chile #Europe #STEM #Education #HD #Video

Zooming in on The Skull & Crossbones Nebula | ESO

Zooming in on The Skull & Crossbones Nebula | ESO

This zoom video starts with a wide view of the Milky Way and ends with a close-up look at a vivid picture of an active star forming region—NGC 2467, otherwise known as the Skull and Crossbones Nebula. This image of dust, gas and bright young stars, gravitationally bound into the form of a grinning skull, was captured with the FORS instrument on the European Southern Observatory’s Very Large Telescope (VLT). Whilst ESO’s telescopes are usually used for the collection of science data, their immense resolving power makes them ideal for capturing images such as this— which are beautiful for their own sake.

Distance: 4,500 light years


Credit:  European Southern Observatory/Digitized Sky Survey 2/N. Risinger

Music: astral electronic

Duration: 50 seconds

Release Date: November 7, 2018


#NASA #ESO #Astronomy #Space #Stars #Nebula #SkullCrossbonesNebula #NGC2467 #Puppis #Constellation #Cosmos #Universe #Telescope #VLT #Chile #Europe #STEM #Education #HD #Video

The Skull & Crossbones Nebula | ESO

The Skull & Crossbones Nebula | ESO


This vivid picture of an active star forming region—NGC 2467, otherwise known as the Skull and Crossbones Nebula—is as sinister as it is beautiful. This image of dust, gas and bright young stars, gravitationally bound into the form of a grinning skull, was captured with the FORS instrument on the European Southern Observatory’s Very Large Telescope (VLT). Whilst ESO’s telescopes are usually used for the collection of science data, their immense resolving power makes them ideal for capturing images such as this—which are beautiful for their own sake.


Credit: European Southern Observatory (ESO)

Release Date: October 24, 2018


#NASA #ESO #Astronomy #Space #Stars #Nebula #SkullCrossbonesNebula #NGC2467 #Puppis #Constellation #Cosmos #Universe #Telescope #VLT #Chile #Europe #STEM #Education

The Skull & Crossbones Nebula | ESO

The Skull & Crossbones Nebula | ESO


Area surrounding the stellar cluster NGC 2467, also known as the Skull & Crossbones Nebula. It is located in the southern constellation of Puppis ("The Stern"). With an age of a few million years at most, it is a very active stellar nursery, where new stars are born continuously from large clouds of dust and gas. The image, looking like a colorful cosmic ghost or a gigantic celestial "skull", contains the open clusters Haffner 18 (center) and Haffner 19 (middle right: it is located inside the smaller pink region—the lower eye of the "skull"), as well as vast areas of ionized gas. The bright star at the center of the largest pink region on the bottom of the image is HD 64315, a massive young star that is helping shaping the structure of the whole nebular region.

Distance: 13,000 light years


Credit: European Southern Observatory (ESO)

Release Date: December 25, 2005


#NASA #ESO #Astronomy #Space #Stars #Nebula #SkullCrossbonesNebula #NGC2467 #StarClusters #Haffner18 #Haffner19 #Star #HD64315 #Puppis #Constellation #Cosmos #Universe #Telescope #Chile #Europe #STEM #Education

Wednesday, August 03, 2022

A Cosmic Concoction | Hubble

A Cosmic Concoction | Hubble


A colorful star-forming region is featured in this stunning new NASA/ESA Hubble Space Telescope image of NGC 2467. Looking like a roiling cauldron of some exotic cosmic brew, huge clouds of gas and dust are sprinkled with bright blue, hot young stars.

Strangely shaped dust clouds, resembling spilled liquids, are silhouetted against a colorful background of glowing. Like the familiar Orion Nebula, NGC 2467 is a huge cloud of gas—mostly hydrogen—that serves as an incubator for new stars.

This picture was created from images taken with the Wide Field Channel of the Advanced Camera for Surveys through three different filters (F550M, F660N and F658N, shown in blue, green and red). These filters were selected to let through different colors of red and yellow light arising from different elements in the gas. The total aggregate exposure time was about 2,000 seconds and the field of view is about 3.5 arcminutes across. These data were taken in 2004.


Credit: NASA, European Space Agency and Orsola De Marco (Macquarie University)

Release Date: July 13, 2010


#NASA #ESA #Astronomy #Space #Hubble #Stars #Nebula #NGC2467 #Puppis #Constellation #Cosmos #Universe #SpaceTelescope #GSFC #STScI #UnitedStates #Europe #STEM #Education

Giant Star Cluster in Scorpius | Hubble

Giant Star Cluster in Scorpius | Hubble

The star cluster Pismis 24 lies in the core of the large emission nebula NGC 6357 that extends one degree on the sky in the direction of the Scorpius constellation. Part of the nebula is ionized by the youngest (bluest) heavy stars in Pismis 24. The intense ultraviolet radiation from the blazing stars heats the gas surrounding the cluster and creates a bubble in NGC 6357. The presence of these surrounding gas clouds makes probing into the region even harder.

One of the top candidates for the title of "Milky Way stellar heavyweight champion" was, until now, Pismis 24-1, a bright young star that lies in the core of the small open star cluster Pismis 24 (the bright stars in the Hubble image) about 8,000 light-years away from Earth. Pismis 24-1 was thought to have an incredibly large mass of 200 to 300 solar masses. New NASA/ESA Hubble measurements of the star, have, however, resolved Pismis 24-1 into two separate stars, and, in doing so, have "halved" its mass to around 100 solar masses.


Credit: NASA, European Space Agency and Jesús Maíz Apellániz (Instituto de Astrofísica de Andalucía, Spain)

Acknowledgement: Davide De Martin (ESA/Hubble)

Release Date: December 11, 2006


#NASA #ESA #Astronomy #Space #Hubble #Stars #StarCluster #Pismis24 #Pismis241 #Nebula #EmissionNebula #NGC6357 #Scorpius #Constellation #Cosmos #Universe #SpaceTelescope #GSFC #STScI #UnitedStates #Europe #STEM #Education

Cosmic Silver Lining | Hubble

Cosmic Silver Lining | Hubble


This image showcases the emission nebula NGC 2313. The bright star V565—surrounded by four prominent diffraction spikes—illuminates a silvery, fan-shaped veil of gas and dust, while the right half of this image is obscured by a dense cloud of dust. Nebulae with similar shapes—a star accompanied by a bright fan of gas—were once referred to as cometary nebulae, though the name is no longer used. 

The language that astronomers use changes as we become better acquainted with the Universe, and astronomical history is littered with now-obsolete phrases to describe objects in the night sky, such as “spiral nebulae” for spiral galaxies or “inferior planets” for Mercury and Venus. 


Credit: European Space Agency/Hubble, R. Sahai

Release Date: May 10, 2021


#NASA #ESA #Astronomy #Space #Hubble #Stars #Star #V565 #EmissionNebula #NGC2313 #Monoceros #Constellation #Cosmos #Universe #SpaceTelescope #GSFC #STScI #UnitedStates #Europe #STEM #Education