Monday, September 26, 2022

NASA's DART Spacecraft Colliding with Asteroid on September 26, 2022

NASA's DART Spacecraft Colliding with Asteroid on September 26, 2022


Looking Back at DART’s Unboxing

Image Description: Technicians prepare to move NASA’s Double Asteroid Redirection Test (DART) spacecraft onto a work stand inside the Astrotech Space Operations Facility at Vandenberg Space Force Base in California following its arrival at the facility on Oct. 4, 2021.

DART was launched on Nov. 23, 2021, aboard a SpaceX Falcon 9 rocket from Vandenberg. The spacecraft will intentionally smash into the moonlet Didymos on Sept. 26, 2022, to see if this method of asteroid deflection—known as the kinetic impactor technique—would be a viable way to protect our planet if an asteroid on a collision course with Earth were discovered in the future.


Image Credit: United States Space Force (USSF) 30th Space Wing/Aaron Taubm

Release Date: September 26, 2022


#NASA #Space #Astronomy #Science #DART #Spacecraft #SpaceX #USSF #Asteroids #Earth #PlanetaryDefense #Test #SolarSystem #JHUAPL #UnitedStates #STEM #Education

Hurricane Ian Flyover | International Space Station

Hurricane Ian Flyover | International Space Station

The International Space Station passed approximately 260 statute miles overhead Hurricane Ian at approximately 3 p.m. EDT Monday, Sept. 26, 2022. External cameras on the orbiting laboratory captured views of the storm as it gained strength south of Cuba while moving toward the north-northwest. The storm is expected to intensify before approaching the west coast of Florida on Wednesday into Thursday. 

NASA managers met Monday morning and made the decision to roll the Artemis I Space Launch System rocket and Orion spacecraft back to the Vehicle Assembly Building after additional data gathered overnight did not show improving expected conditions for the Kennedy Space Center area. The decision allows time for employees to address the needs of their families and protect the integrated rocket and spacecraft system.


Credit: NASA's Johnson Space Center (JSC)

Duration: 11 minute

Release Date: September 26, 2022


#NASA #Space #ISS #Earth #Planet #Atmosphere #Weather #HurricaneIan #Hurricane #Meteorology #CaribbeanSea #AtlanticOcean #Cuba #Artemis #ArtemisI #Astronauts #Photography #Art #Science #HumanSpaceflight #Expedition67 #Florida #UnitedStates #International #STEM #Education #HD #Video

Jupiter's Closest Approach to Earth in 59 Years! | NASA

Jupiter's Closest Approach to Earth in 59 Years! | NASA


Stargazers can expect excellent views of Jupiter the entire night of Monday, Sept. 26, 2022, when the giant planet reaches opposition. From the viewpoint of Earth’s surface, opposition happens when an astronomical object rises in the east as the Sun sets in the west, placing the object and the Sun on opposite sides of Earth.

Jupiter’s opposition occurs every 13 months, making the planet appear larger and brighter than any other time of the year. But that’s not all. Jupiter will also make its closest approach to Earth since 1963—almost six decades ago! This happens because Earth and Jupiter do not orbit the Sun in perfect circles—meaning the planets will pass each other at different distances throughout the year. Jupiter’s closest approach to Earth rarely coincides with opposition, which means this year’s views will be extraordinary. At its closest approach, Jupiter will be approximately 367 million miles in distance from Earth, about the same distance it was in 1963. The massive planet is approximately 600 million miles away from Earth at its farthest point.

“With good binoculars, the banding (at least the central band) and three or four of the Galilean satellites (moons) should be visible,” said Adam Kobelski, a research astrophysicist at NASA’s Marshall Space Flight Center in Huntsville, Alabama. “It’s important to remember that Galileo observed these moons with 17th century optics. One of the key needs will be a stable mount for whatever system you use.”

Kobelski recommends a larger telescope to see Jupiter’s Great Red Spot and bands in more detail; a 4 inch-or-larger telescope and some filters in the green to blue range would enhance the visibility of these features.

According to Kobelski, an ideal viewing location will be at a high elevation in a dark and dry area.

“The views should be great for a few days before and after Sept. 26,” Kobelski said. “So, take advantage of good weather on either side of this date to take in the sight. Outside of the Moon, it should be one of the (if not the) brightest objects in the night sky.”

Jupiter has 53 named moons, but scientists believe that 79 moons have been detected in total. The four largest moons, Io, Europa, Ganymede, and Callisto, are called the Galilean satellites. They are named after the man who first observed them in 1610, Galileo Galilei. In binoculars or a telescope, the Galilean satellites should appear as bright dots on either side of Jupiter during opposition.

NASA’s Juno spacecraft, which has been orbiting Jupiter for six years, is dedicated to exploring the planet and its moons. Juno began its journey in 2011 and reached Jupiter five years later. Since 2016, the spacecraft has provided incredible images and data about Jupiter’s lively atmosphere, interior structures, internal magnetic field, and magnetosphere.

Scientists believe studying Jupiter can lead to breakthrough discoveries about the formation of the solar system. Juno’s mission was recently extended until 2025 or until the end of the spacecraft’s life. Learn more about Juno: 

https://go.nasa.gov/3r9WsOL

The next major project for Jupiter exploration is the Europa Clipper. This spacecraft will explore Jupiter’s iconic moon, Europa, which is known for its icy shell and vast ocean that lies beneath its surface. NASA scientists aim to find whether Europa has conditions able to sustain life.  Europa Clipper’s targeted launch is currently scheduled for no earlier than October 2024.


Credit: National Aeronautics and Space Administration (NASA)

Release Date: Sept. 16, 2022


#NASA #ESA #Space #Astronomy #Science #Hubble #Jupiter #Planet #Earth #SolarSystem #Skywatching #SpaceTelescope #GSFC #STScI #Juno #Spacecraft #UnitedStates #Europe #STEM #Education

How Will We Know if NASA’s DART Mission Changed an Asteroid’s Orbit?

How Will We Know if NASA’s DART Mission Changed an Asteroid’s Orbit?

NASA’s Double Asteroid Redirection Test, also known as DART, is humanity’s first attempt to change the motion of a non-hazardous asteroid in space by intentionally crashing a spacecraft into it. After impact, ground-based observatories across the globe will turn their eyes to the skies to determine if this planetary defense test was successful. In this video, NASA visits Lowell Observatory to learn more about how astronomers have been tracking this double asteroid over the course of many years, and how they will document the orbital change post-impact.

DART is a spacecraft designed to impact an asteroid as a test of technology. DART’s target asteroid is NOT a threat to Earth. This asteroid system is a perfect testing ground to see if intentionally crashing a spacecraft into an asteroid is an effective way to change its course, should a hazardous asteroid be discovered in the future.


For more on DART, visit https://nasa.gov/dart

https://dart.jhuapl.edu/


Credit: National Aeronautics and Space Administration (NASA)

Duration: 4 minutes

Release Date: September 6, 2022

#NASA #Space #Astronomy #Science #DART #Spacecraft #Asteroids #Earth #PlanetaryDefense #Test #SolarSystem #JHUAPL #LowellObservatory #UnitedStates #STEM #Education #HD #Video

Todays' Asteroid Test | Defending the Planet: NASA’s DART Mission

Todays' Asteroid Test | Defending the Planet: NASA’s DART Mission

Launched in November 2021, NASA's Double Asteroid Redirection Test (DART) will be the world’s first mission to test planetary defense techniques, demonstrating one mitigation method of asteroid deflection, called kinetic impact. DART will impact the small asteroid moonlet Dimorphos, which orbits a larger companion, Didymos, in a binary asteroid system to change its orbital period. Although neither asteroid poses a threat to Earth, the collision with Dimorphos enables researchers to demonstrate the deflection technique along with several new technologies, and collect important data to enhance our modeling and predictive capabilities for asteroid deflection. Those enhancements will help us better prepare should an asteroid ever be discovered as a threat to Earth.

NASA’s Double Asteroid Redirection Test (DART), the world’s first mission to test technology for defending Earth against potential asteroid or comet hazards, will impact its target asteroid—which poses no threat to Earth—on Monday evening, Sept. 26, 2022.

5:30 p.m. EDT (21:30 UTC):  Live feed from the DART spacecraft as it approaches asteroid Didymos: https://www.nasa.gov/multimedia/nasatv/index.html#media

6 p.m. EDT (22:00 UTC): Live broadcast coverage of the DART mission as the spacecraft attempts to deflect an asteroid from its path (impact targeted for 7:14 p.m. EDT)

https://www.nasa.gov/multimedia/nasatv/index.html#public


The Johns Hopkins Applied Physics Laboratory manages the DART mission for NASA's Planetary Defense Coordination Office as a project of the agency’s Planetary Missions Program Office. 

For more information about DART, visit:

https://dart.jhuapl.edu/

https://www.nasa.gov/dartmission


Credit: Johns Hopkins University Applied Physics Laboratory (JHUAPL)

Duration: 2 minutes, 48 seconds 

Release Date: November 23, 2021


#NASA #Space #Astronomy #Science #DART #Spacecraft #Asteroids #Earth #PlanetaryDefense #Test #SolarSystem #JHUAPL #UnitedStates #STEM #Education #HD #Video

Behind the Spacecraft: NASA's DART—The Double Asteroid Redirection Test Today

Behind the Spacecraft: NASA's DART—The Double Asteroid Redirection Test Today

NASA is crashing a spacecraft into an asteroid . . . on purpose! Our DART mission is a first-of-its-kind planetary defense test to change the motion of an asteroid in space so that we could use this technique if an asteroid were ever discovered to be a threat to Earth. 

Follow DART: www.nasa.gov/DART

The DART mission is a test of a technique that could be used to mitigate the threat of an asteroid on a collision course with Earth should one be discovered in the future. DART’s target is not a threat to Earth. While no known asteroid larger than 140 meters in size has a significant chance to hit Earth for the next 100 years, only about 40 percent of those asteroids have been found as of October 2021.

NASA’s Double Asteroid Redirection Test (DART), the world’s first mission to test technology for defending Earth against potential asteroid or comet hazards, will impact its target asteroid—which poses no threat to Earth—on Monday evening, Sept. 26, 2022.

5:30 p.m. EDT (21:30 UTC):  Live feed from the DART spacecraft as it approaches asteroid Didymos: https://www.nasa.gov/multimedia/nasatv/index.html#media

6 p.m. EDT (22:00 UTC): Live broadcast coverage of the DART mission as the spacecraft attempts to deflect an asteroid from its path (impact targeted for 7:14 p.m. EDT)

https://www.nasa.gov/multimedia/nasatv/index.html#public

This test will show a spacecraft can autonomously navigate to a target asteroid and intentionally collide with it to change the asteroid’s motion in a way that can be measured using ground-based telescopes. DART will provide important data to help better prepare for an asteroid that might pose an impact hazard to Earth, should one ever be discovered.


Credits: NASA

Producer/Editor: Jessica Wilde

Producer: Scott Bednar

Videographers: James Lucas and Seth Robinson

Duration: 2 minutes, 29 seconds

Release Date: October 24, 2021


#NASA #Space #Astronomy #Science #DART #Spacecraft #Asteroids #Earth #PlanetaryDefense #Test #SolarSystem #JHUAPL #UnitedStates #STEM #Education #HD #Video

A Close-up Look at The Antennae Galaxies | Hubble

A Close-up Look at The Antennae Galaxies | Hubble

The Antennae Galaxies—also known as NGC 4038 and NGC 4039—are locked in a deadly embrace. Once normal, sedate spiral galaxies like the Milky Way, the pair have spent the past few hundred million years sparring with one another. This clash is so violent that stars have been ripped from their host galaxies to form a streaming arc between the two. In wide-field images of the pair the reason for their name becomes clear—far-flung stars and streamers of gas stretch out into space, creating long tidal tails reminiscent of antennae.

This image of the Antennae Galaxies shows obvious signs of chaos. Clouds of gas are seen in bright pink and red, surrounding the bright flashes of blue star-forming regions—some of which are partially obscured by dark patches of dust. The rate of star formation is so high that the Antennae Galaxies are said to be in a state of starburst, a period in which all of the gas within the galaxies is being used to form stars. This cannot last forever and neither can the separate galaxies; eventually the nuclei will coalesce, and the galaxies will begin their retirement together as one large elliptical galaxy.


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

Duration: 46 seconds

Release Date: February 16, 2016


#NASA #ESA #Astronomy #Space #Hubble #Antennae #Galaxies #AntennaeGalaxies #NGC4038 #NGC4039 #Corvus #Constellation #MilkyWay #Galaxy #Cosmos #Universe #SpaceTelescope #GSFC #STScI #UnitedStates #Europe #STEM #Education #SD #Video

Zooming in on The Tail of The Antennae Galaxies | Hubble

Zooming in on The Tail of The Antennae Galaxies | Hubble

This video shows the constellation of Corvus, the Crow, and a zoom into the tidal tail of the Antennae Galaxies.


Credit: NASA, European Space Agency (ESA), R. Gendler and A. Fujii

Duration: 58 seconds

Release Date: February 17, 2016


#NASA #Astronomy #Space #Antennae #Galaxies #AntennaeGalaxies #NGC4038 #NGC4039 #Corvus #Constellation #MilkyWay #Galaxy #Cosmos #Universe #NOAO #Telescope #UnitedStates #STEM #Education #HD #Video

Stars in the Tail of The Antennae Galaxies | Hubble

Stars in the Tail of The Antennae Galaxies | Hubble


This Hubble Advanced Camera for Surveys (ACS) image shows a portion of the southern tidal tail of the Antennae galaxies. The main visible component consists of young blue stars recently formed out of the gas accumulating along the spine of the tail, and many red background galaxies can also be seen. The region is also filled by thousands of faint red stars, just visible when zooming on the image.

Distance: 45 million light years

The Antennae Galaxies are among the closest known merging galaxies. The two galaxies, also known as NGC 4038 and NGC 4039, started to interact a few hundred million years ago, creating one of the most impressive sights in the night sky. They are considered by scientists as the archetypal merging galaxy system and are used as a standard with which to validate theories about galaxy evolution.

By measuring the colors and brightnesses of red giant stars in the system, the scientists found that the Antennae Galaxies are much closer than previously thought: 45 million light-years instead of the previous best estimate of 65 million light-years. These red stars cannot be brighter than a certain threshold, and it is this luminosity threshold that was used to derive the new distance of the Antennae.


Credit: NASA, ESA & Ivo Saviane (European Southern Observatory)

Release Date: May 9, 2008


#NASA #Astronomy #Space #Antennae #Galaxies #AntennaeGalaxies #NGC4038 #NGC4039 #Corvus #Constellation #MilkyWay #Galaxy #Cosmos #Universe #NOAO #Telescope #UnitedStates #STEM #Education

A Stately Spiral Galaxy in Hydra: NGC 5495 | Hubble

A Stately Spiral Galaxy in Hydra: NGC 5495 | Hubble


The stately sweeping spiral arms of the spiral galaxy NGC 5495 are revealed by the NASA/European Space Agency Hubble Space Telescope’s Wide Field Camera 3 in this image. NGC 5495, which lies around 300 million light-years from Earth in the constellation Hydra, is a Seyfert galaxy, a type of galaxy with a particularly bright central region. These luminous cores—known to astronomers as active galactic nuclei—are dominated by the light emitted by dust and gas falling into a supermassive black hole.

This image is drawn from a series of observations captured by astronomers studying supermassive black holes lurking in the hearts of other galaxies. Studying the central regions of galaxies can be challenging: as well as the light created by matter falling into supermassive black holes, areas of star formation and the light from existing stars all contribute to the brightness of galactic cores. Hubble’s crystal-clear vision helped astronomers disentangle the various sources of light at the core of NGC 5495, allowing them to precisely weigh its supermassive black hole.

As well as NGC 5495, two stellar interlopers are visible in this image. One is just outside the center of NGC 5495, and the other is very prominent alongside the galaxy. While they share the same location on the sky, these objects are much closer to home than NGC 5495: they are stars from our own Milky Way. The bright stars are surrounded by criss-cross diffraction spikes, optical artefacts created by the internal structure of Hubble interacting with starlight.


Credit: European Space Agency (ESA)/Hubble & NASA, J. Greene

Acknowledgement: R. Colombari

Release Date: September 26, 2022


#NASA #ESA #Astronomy #Space #Galaxy #SeyfertGalaxy #NGC5495 #Hubble #Hydra #Constellation #Cosmos #Universe #SpaceTelescope #GSFC #STScI #UnitedStates #Europe #STEM #Education

Sunday, September 25, 2022

The Antennae Galaxies: Wide-field View

The Antennae Galaxies: Wide-field View

This photo of the Antennae galaxies was taken with one of the National Optical Astronomy Observatory (NOAO) telescopes from the ground.

This image is a color composite made from exposures from the Digitized Sky Survey 2 (DSS2). The field of view is 2.8 x 2.8 degrees.


Credit: European Space Agency (ESA)/Hubble and Digitized Sky Survey 2

Acknowledgements: Davide De Martin (ESA/Hubble)


#NASA #Astronomy #Space #Antennae #Galaxies #AntennaeGalaxies #NGC4038 #NGC4039 #Corvus #Constellation #MilkyWay #Galaxy #Cosmos #Universe #NOAO #Telescope #UnitedStates #STEM #Education

The Antennae Galaxies: Ground-based View

The Antennae Galaxies: Ground-based View

This photo of the Antennae galaxies was taken with one of the National Optical Astronomy Observatory (NOAO) telescopes from the ground.


Credit: NOAO/AURA/NSF, B. Twardy, B. Twardy, and A. Block (NOAO)

Release Date: October 17, 2006


#NASA #Astronomy #Space #Antennae #Galaxies #AntennaeGalaxies #NGC4038 #NGC4039 #Corvus #Constellation #MilkyWay #Galaxy #Cosmos #Universe #NOAO #Telescope #UnitedStates #STEM #Education

The Antennae Galaxies (Optical, X-ray & Infrared) | Hubble, Chandra & Spitzer

The Antennae Galaxies (Optical, X-ray & Infrared) | Hubble, Chandra & Spitzer

This is a beautiful image of two colliding galaxies by NASA's Great Observatories. The Antennae galaxies, located about 62 million light-years from Earth, are shown in this composite image from the Chandra X-ray Observatory (blue), the Hubble Space Telescope (gold and brown), and the Spitzer Space Telescope (red). The Antennae galaxies take their name from the long antenna-like "arms," seen in wide-angle views of the system. These features were produced by tidal forces generated in the collision.

The collision, which began more than 100 million years ago and is still occurring, has triggered the formation of millions of stars in clouds of dusts and gas in the galaxies. The most massive of these young stars have already sped through their evolution in a few million years and exploded as supernovae.

The X-ray image from Chandra shows huge clouds of hot, interstellar gas that have been injected with rich deposits of elements from supernova explosions. This enriched gas, which includes elements such as oxygen, iron, magnesium, and silicon, will be incorporated into new generations of stars and planets. The bright, point-like sources in the image are produced by material falling onto black holes and neutron stars that are remnants of the massive stars. Some of these black holes may have masses that are almost one hundred times that of the Sun.

The Spitzer data show infrared light from warm dust clouds that have been heated by newborn stars, with the brightest clouds lying in the overlapping region between the two galaxies.

The Hubble data reveal old stars and star-forming regions in gold and white, while filaments of dust appear in brown. Many of the fainter objects in the optical image are clusters containing thousands of stars.

The Chandra image was taken in December 1999. The Spitzer image was taken in December 2003. The Hubble image was taken in July 2004, and February 2005.


Credit: NASA, European Space Agency (ESA), SAO, CXC, JPL-Caltech, and STScI 

Acknowledgment: G. Fabbiano and Z. Wang (Harvard-Smithsonian CfA, USA), and B. Whitmore (STScI)

Release Date: August 5, 2010


#NASA #ESA #Astronomy #Space #Hubble #Spitzer #Chandra #Infrared #Antennae #Galaxies #AntennaeGalaxies #NGC4038 #NGC4039 #Corvus #Constellation #MilkyWay #Galaxy #Cosmos #Universe #SpaceTelescope #GSFC #STScI #JPL #CXC #UnitedStates #Europe #STEM #Education

Zooming Out from The Antennae Galaxies | Hubble

Zooming Out from The Antennae Galaxies | Hubble


Distance: 65 million light years


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

Duration: 22 seconds

Release Date: February 17, 2016


#NASA #ESA #Astronomy #Space #Hubble #Antennae #Galaxies #AntennaeGalaxies #NGC4038 #NGC4039 #Corvus #Constellation #MilkyWay #Galaxy #Cosmos #Universe #SpaceTelescope #GSFC #STScI #UnitedStates #Europe #STEM #Education #HD #Video

Panning on The Antennae Galaxy | Hubble

Panning on The Antennae Galaxy | Hubble  

Panning on the Antennae Galaxy. The stellar fireworks contain brilliant young clusters of tens of thousands of stars. Orange blobs to the left and right of center are the two cores of the original galaxies, criss-crossed by dark filaments of dust seen in silhouette. Brilliant blue star clusters, born in the collision, pepper the galaxies. Pinkish glowing hydrogen gas identify star birth regions glowing under the intense energy from newborn stars.


Credit:ESA/Hubble (Martin Kornmesser)

Duration: 58 seconds

Release Date: October 17, 2006


#NASA #ESA #Astronomy #Space #Hubble #Antennae #Galaxies #AntennaeGalaxies #NGC4038 #NGC4039 #Corvus #Constellation #MilkyWay #Galaxy #Cosmos #Universe #SpaceTelescope #GSFC #STScI #UnitedStates #Europe #STEM #Education #SD #Video

Zooming on The Antennae Galaxy | Hubble

Zooming on The Antennae Galaxy | Hubble

Zooming through the nighttime sky into the constellation Corvus the crow, deeper into the Hubble's Advanced Camera for Surveys image of the Antennae galaxies. The stellar fireworks contain brilliant young clusters of tens of thousands of stars. Orange blobs to the left and right of center are the two cores of the original galaxies, criss-crossed by dark filaments of dust seen in silhouette. 

Brilliant blue star clusters, born in the collision, pepper the galaxies. Pinkish glowing hydrogen gas identify star birth regions glowing under the intense energy from newborn stars.


Credit: Akira Fujii, Digitized Sky Survey 2 and ESA/Hubble (Martin Kornmesser)

Duration: 58 seconds

Release Date: February 16, 2016


#NASA #ESA #Astronomy #Space #Hubble #Antennae #Galaxies #AntennaeGalaxies #NGC4038 #NGC4039 #Corvus #Constellation #MilkyWay #Galaxy #Cosmos #Universe #SpaceTelescope #GSFC #STScI #UnitedStates #Europe #STEM #Education #HD #Video