Friday, November 08, 2024

The Veil Nebula | Filaments of The Cygnus Loop: Image 5 | WIYN Telescope

The Veil Nebula | Filaments of The Cygnus Loop: Image 5 | WIYN Telescope



This image was obtained with the wide-field view of the Mosaic camera on the WIYN 0.9-meter telescope at Kitt Peak, Arizona. It shows NGC 6960—faint filaments that are part of a large supernova remnant (SNR) called the Cygnus Loop. These are the remains of a star that exploded 5,000 to 10,000 years ago. The original supernova would have been bright enough to be seen clearly from Earth with the naked eye. The star—that was 20 times the mass of the Sun—lived fast and died young, ending its life in a cataclysmic release of energy. The distance to it is estimated at about 1,500 light years. The bright star near the center of the image, known as 52 Cygnus, is not associated with the supernova.

The Cygnus Loop (radio source W78, or Sharpless 103), located in the constellation Cygnus, is an emission nebula measuring nearly 3° across. Arcs of the loop, known collectively as the Veil Nebula or Cirrus Nebula, emit in the visible electromagnetic range. Radio, infrared, and X-ray images reveal the complete loop. The Cygnus Loop extends over three times the size of the full moon in the night sky, and is tucked next to one of the “swan’s wings” in the constellation of Cygnus.

The color image was generated by combining data from narrowband filters; data from H-alpha was assigned a red color, [OIII] is blue, and [SII] is green. North is to the left and east is down.

The WIYN Consortium, led by the University of Wisconsin-Madison and Indiana University, are operational responsible for the historic 0.9-meter (36-inch) WIYN Telescope at the National Science Foundation's Kitt Peak National Observatory (KPNO).


Image Credit: T.A. Rector (University of Alaska Anchorage) and WIYN/NOIRLab/NSF/AURA
Release Date: June 30, 2020


#NASA #Astronomy #Space #Science #Stars #SupernovaRemnant #SNR #Nebulae #Nebula #VeilNebula #CygnusLoop #W78 #Sharpless103 #IC1340 #NGC6960 #EmissionNebula #52Cygnus #Cygnus #Constellation #MilkyWayGalaxy #Universe #WIYNTelescope #KPNO #Arizona #NSF #AURA #UnitedStates #STEM #Education

The Veil Nebula | Filaments of The Cygnus Loop: Image 4 | WIYN Telescope

The Veil Nebula | Filaments of The Cygnus Loop: Image 4 | WIYN Telescope

This image was obtained with the wide-field view of the Mosaic camera on the WIYN 0.9-meter telescope at Kitt Peak, Arizona. It shows NGC 6992—faint filaments that are part of a large supernova remnant (SNR) called the Cygnus Loop. These are the remains of a star that exploded 5000 to 10,000 years ago. The original supernova would have been bright enough to be seen clearly from Earth with the naked eye. The star—that was 20 times the mass of the Sun—lived fast and died young, ending its life in a cataclysmic release of energy. The distance to it is estimated at about 1,500 light years.

The Cygnus Loop (radio source W78, or Sharpless 103), located in the constellation Cygnus, is an emission nebula measuring nearly 3° across. Arcs of the loop, known collectively as the Veil Nebula or Cirrus Nebula, emit in the visible electromagnetic range. Radio, infrared, and X-ray images reveal the complete loop. The Cygnus Loop extends over three times the size of the full moon in the night sky, and is tucked next to one of the “swan’s wings” in the constellation of Cygnus.

The image was generated with observations in the Oxygen [OIII] (blue), Sulphur [S II] (green) and Hydrogen-Alpha (orange) filters. In this image, North is right, East is up.

The WIYN Consortium, led by the University of Wisconsin-Madison and Indiana University, are operational responsible for the historic 0.9-meter (36-inch) WIYN Telescope at the National Science Foundation's Kitt Peak National Observatory (KPNO).


Image Credit: T.A. Rector (University of Alaska Anchorage) and WIYN/NOIRLab/NSF/AURA
Release Date: June 30, 2020


#NASA #Astronomy #Space #Science #Stars #SupernovaRemnant #SNR #Nebulae #Nebula #VeilNebula #CygnusLoop #W78 #Sharpless103 #IC1340 #NGC6992 #EmissionNebula #Cygnus #Constellation #MilkyWayGalaxy #Universe #WIYNTelescope #KPNO #Arizona #NSF #AURA #UnitedStates #STEM #Education

The Veil Nebula | Filaments of The Cygnus Loop: Image 3 | WIYN Telescope

The Veil Nebula | Filaments of The Cygnus Loop: Image 3 | WIYN Telescope


This image was obtained with the wide-field view of the Mosaic camera on the WIYN 0.9-meter telescope at Kitt Peak, Arizona. It shows faint filaments that are part of a large supernova remnant (SNR) called the Cygnus Loop. These are the remains of a star that exploded 5000 to 10,000 years ago. The original supernova would have been bright enough to be seen clearly from Earth with the naked eye. The star—that was 20 times the mass of the Sun—lived fast and died young, ending its life in a cataclysmic release of energy. The distance to it is estimated at about 1,500 light years.

Because of its immense size, the Veil Nebula contains several individually named objects, including NGC 6992 and IC 1340 on the left side as well as NGC 6960 and Pickering's Triangle on the right. To create this image, nine separate images were taken and stitched together. The full-resolution image is over 600 megapixels in size. It covers an area of the sky that is about 45 times that of the full moon. 

The Cygnus Loop (radio source W78, or Sharpless 103), located in the constellation Cygnus, is an emission nebula measuring nearly 3° across. Arcs of the loop, known collectively as the Veil Nebula or Cirrus Nebula, emit in the visible electromagnetic range. Radio, infrared, and X-ray images reveal the complete loop. The Cygnus Loop extends over three times the size of the full moon in the night sky, and is tucked next to one of the “swan’s wings” in the constellation of Cygnus.

The image was generated with observations in the Oxygen [OIII] (blue), Sulphur [S II] (green) and Hydrogen-Alpha (orange) filters. In this image, North is up, East is left. Please note that the full resolution version of this image is extremely large at more than 24,000 pixels on a side, and the file size of the TIFF is 1.65 Gigabytes. 

The WIYN Consortium, led by the University of Wisconsin-Madison and Indiana University, are operational responsible for the historic 0.9-meter (36-inch) WIYN Telescope at the National Science Foundation's Kitt Peak National Observatory (KPNO).


Image Credit: T.A. Rector (University of Alaska Anchorage) and WIYN/NOIRLab/NSF/AURA
Release Date: Dec. 18, 2012


#NASA #Astronomy #Space #Science #Stars #SupernovaRemnant #SNR #Nebulae #Nebula #VeilNebula #CygnusLoop #W78 #Sharpless103 #IC1340 #EmissionNebula #Cygnus #Constellation #MilkyWayGalaxy #Universe #WIYNTelescope #KPNO #Arizona #NSF #AURA #UnitedStates #STEM #Education

The Veil Nebula | FiIaments of The Cygnus Loop: Image 2 | Mayall Telescope

The Veil Nebula | Filaments of The Cygnus Loop: Image 2 | Mayall Telescope

These faint filaments (IC 1340) are part of a large supernova remnant (SNR) called the Cygnus Loop, located about 1,500 light-years from Earth. Astronomers estimate the supernova explosion that produced the Veil Nebula occurred between 5,000 to 10,000 years ago. The filaments are the remains of a star that exploded 5,000 to 10,000 years ago. The original supernova would have been bright enough to be seen clearly from Earth with the naked eye. The star—that was 20 times the mass of the Sun—lived fast and died young, ending its life in a cataclysmic release of energy.

The Cygnus Loop (radio source W78, or Sharpless 103), located in the constellation Cygnus, is an emission nebula measuring nearly 3° across. Arcs of the loop, known collectively as the Veil Nebula or Cirrus Nebula, emit in the visible electromagnetic range. Radio, infrared, and X-ray images reveal the complete loop. The Cygnus Loop extends over three times the size of the full moon in the night sky, and is tucked next to one of the “swan’s wings” in the constellation of Cygnus.

This image was obtained with the wide-field view of the Mosaic camera on the 4-meter Mayall telescope at Kitt Peak National Observatory. 

The image was generated with observations in the Oxygen [OIII] (blue), Sulphur [S II] (green) and Hydrogen-Alpha (orange) filters. In this image, North is left, East is down.

The Nicholas U. Mayall Telescope is a four-meter (158 inches) reflector telescope in Arizona named after the American observational astronomer of the same name. The telescope saw first light on February 27, 1973, and was the second-largest in the world at that time.

Learn more about the Mayall Telescope: 

https://noirlab.edu/science/programs/kpno/telescopes/nicholas-mayall-4m-telescope


Credit: T.A. Rector (University of Alaska Anchorage) and H. Schweiker (WIYN and NOIRLab/NSF/AURA)
Release Date: June 30, 2020


#NASA #Astronomy #Space #Science #Stars #SupernovaRemnant #SNR #Nebulae #Nebula #VeilNebula #CygnusLoop #W78 #Sharpless103 #IC1340 #EmissionNebula #Cygnus #Constellation #MilkyWayGalaxy #Universe #MayallTelescope #KPNO #Arizona #NSF #AURA #UnitedStates #STEM #Education

The Veil Nebula | FiIaments of The Cygnus Loop: Image 1 | Mayall Telescope

The Veil Nebula | FiIaments of The Cygnus Loop: Image 1 | Mayall Telescope

These are faint filaments that are part of a large supernova remnant (SNR) called the Cygnus Loop. It is located about 1,500 light-years from Earth. These filaments are the remains of a star that exploded 5,000 to 10,000 years ago. The original supernova would have been bright enough to be seen clearly from Earth with the naked eye. The star—that was 20 times the mass of the Sun—lived fast and died young, ending its life in a cataclysmic release of energy.


The Cygnus Loop (radio source W78, or Sharpless 103), located in the constellation Cygnus, is an emission nebula measuring nearly 3° across. Arcs of the loop, known collectively as the Veil Nebula or Cirrus Nebula, emit in the visible electromagnetic range. Radio, infrared, and X-ray images reveal the complete loop. The Cygnus Loop extends over three times the size of the full moon in the night sky, and is tucked next to one of the “swan’s wings” in the constellation of Cygnus.

This image was obtained with the wide-field view of the Mosaic camera on the 4-meter Mayall telescope at Kitt Peak National Observatory. 

The image was generated with observations in the Oxygen [OIII] (blue), Sulphur [S II] (green) and Hydrogen-Alpha (orange) filters. In this image, North is down, East is right.

The Nicholas U. Mayall Telescope is a four-meter (158 inches) reflector telescope in Arizona named after the American observational astronomer of the same name. The telescope saw first light on February 27, 1973, and was the second-largest in the world at that time.

Learn more about the Mayall Telescope: 

https://noirlab.edu/science/programs/kpno/telescopes/nicholas-mayall-4m-telescope


Credit: T.A. Rector (University of Alaska Anchorage) and H. Schweiker (WIYN and NOIRLab/NSF/AURA)
Release Date: June 30, 2020


#NASA #Astronomy #Space #Science #Stars #Nebulae #Nebula #VeilNebula #CygnusLoop #W78 #Sharpless103 #Cygnus #Constellation #MilkyWayGalaxy #Universe #MayallTelescope #KPNO #KittPeakNationalObservatory #Arizona #NSF #AURA #UnitedStates #STEM #Education

Spot Comet Tsuchinshan-ATLAS over Italian Village of Vitorchiano

Spot Comet Tsuchinshan-ATLAS over Italian Village of Vitorchiano

Featured here is a photo of Comet Tsuchinshan-ATLAS as observed on the morning of September 30, 2024, over the Borgo sospeso of Vitorchiano. The waning crescent Moon is at upper left. Because of its weekly hyperbolic orbit, it is not known if Tsuchinshan-ATLAS will be ejected from our solar system and never be seen again. In late September, near perihelion (September 27), it became a naked eye object for the first time. Note that its closest approach to the Earth occurred on October 12, 2024.

Image Details: HDR of 5 shots with times from 1/25 of a second to 5 seconds exposure; 640 ISO; Nikon Z9 camera; Nikon Z70-200/2.8S lens; f/3.5; 100 mm focal length; taken at 06:20 local time.

C/2023 A3 (Tsuchinshan–ATLAS) is a comet from the solar system's Oort cloud discovered by the Purple Mountain Observatory east of Nanjing, China, on January 9, 2023, and independently found by the automated Asteroid Terrestrial-impact Last Alert System (ATLAS) in South Africa on February 22, 2023. ATLAS is funded by NASA's planetary defense office, and developed and operated by the University of Hawaii's Institute for Astronomy. C/2023 A3 passed perihelion (closest approach to the Sun) at a distance of 0.39 AU (58 million km; 36 million miles) on September 27, 2024.

The Oort cloud is theorized to be a vast cloud of icy planetesimals surrounding the Sun at distances ranging from 2,000 to 200,000 AU (0.03 to 3.2 light-years). The concept of such a cloud was proposed in 1950 by the Dutch astronomer Jan Oort, in whose honor the idea was named. Oort proposed that the bodies in this cloud replenish and keep constant the number of long-period comets entering the inner Solar System—where they are eventually consumed and destroyed during close approaches to the Sun.


Image Credit: Marco Meniero
Location: Borgo sospeso of Vitorchiano (Vt), Italy
Coordinates: 42.4704, 12.1742
Marco's Website: https://www.meniero.it
Caption Credits: Marco Meniero; Jim Foster
Image Date: Sept. 30, 2024
Release Date: Nov. 8, 2024


#NASA #Space #Astronomy #Science #SolarSystem #Planet #Earth #Moon #Italy #Italia #Europe #CentralEurope #Comets #CometTsuchinshanATLAS #C2023A3 #OortCloud #SolarSystem #Astrophotography #MarcoMeniero #Astrophotographer #China #中国 #SouthAfrica #STEM #Education #EPoD

Stephan's Quintet: A Multi-Wavelength Exploration | Space Telescope Science Institute

Stephan's Quintet: A Multi-Wavelength Exploration | Space Telescope Science Institute

This visualization explores the galaxy group Stephan's Quintet by using observations in visible, infrared, and X-ray light. The sequence contrasts images from NASA's Hubble Space Telescope, Spitzer Space Telescope, Webb Space Telescope, and Chandra X-ray Observatory to provide insights across the electromagnetic spectrum.

Exploring the grouping in three dimensions, the video showcases the galaxy distances, diverse shapes, and the interactions between them. In particular, the stretched and distorted galactic features, along with a ridge of high-energy emission, provide evidence of a high-speed collision occurring within the group.

Multi-wavelength views enable contrasting and complimentary studies of this complex compact group.


Video Credit: Space Telescope Science Institute (STScI)

Visualization: Frank Summers (STScI), Alyssa Pagan (STScI), Joseph DePasquale (STScI), Leah Hustak (STScI), Joseph Olmsted (STScI), Greg Bacon (STScI); Narration: Frank Summers (STScI); Audio: Danielle Kirshenblat (STScI); Producer: NASA's Universe of Learning

Duration: 5 minutes

Release Date: Nov. 8, 2024


#NASA #ESA #Astronomy #Space #Science #Hubble #Galaxies #NGC7319 #NGC7320 #NGC7320C #NGC7318A #NGC7318B #NGC7317 #StephansQuintet #HicksonCompactGroup92 #Pegasus #Constellation #Universe #JWST #HST #NASASpitzer #NASAChandra #SpaceTelescopes #GSFC #STScI #UnitedStates #Europe #CSA #Canada #STEM #Education #HD #Video

NASA's Space to Ground: Location, Location, Location | Week of Nov. 8, 2024

NASA's Space to Ground: Location, Location, Location | Week of Nov. 8, 2024

NASA's Space to Ground is your weekly update on what's happening aboard the International Space Station. The SpaceX Dragon Freedom spacecraft, with Expedition 72 crew members NASA astronauts Nick Hague, Suni Williams, and Butch Wilmore, as well as Roscosmos cosmonaut Aleksandr Gorbunov, autonomously redocked with the space-facing port of the station’s Harmony module on November 3, 2024.

The port relocation freed up Harmony’s forward-facing port for the 31st SpaceX commercial resupply services mission to the International Space Station. This was the fifth port relocation of a Dragon spacecraft with crew aboard following previous moves during the Crew-1, Crew-2, Crew-6, and Crew-8 missions.

Expedition 72 Updates:

https://blogs.nasa.gov/spacestation/

Expedition 72 Crew

Station Commander: Suni Williams

Roscosmos (Russia): Alexey Ovchinin, Ivan Vagner, Aleksandr Gorbunov

NASA: Butch Wilmore, Don Pettit, Nick Hague

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.

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)


Video Credit: NASA's Johnson Space Center (JSC)
Duration: 3 minutes, 10 seconds 
Release Date: Nov. 8, 2024


#NASA #Space #Science #ISS #Earth #SpaceX #CRS31 #CargoDragonSpacecraft #SpaceXCrew9 #CrewDragonSpacecraft #CrewDragonFreedom #Astronauts #Cosmonauts #Russia #Россия #Roscosmos #Роскосмос #InternationalCooperation #LongDurationMissions #HumanSpaceflight #SpaceLaboratory #UnitedStates #Expedition72 #STEM #Education #HD #Video

Thursday, November 07, 2024

Hurricane Rafael after Crossing Cuba | NOAA GOES 16 Weather Satellite

Hurricane Rafael after Crossing Cuba | NOAA GOES 16 Weather Satellite



The latest major storm in 2024’s active hurricane season brought heavy rain and storm surge to Cuba as it moved into the Gulf of Mexico. Hurricane Rafael made landfall in the western Cuban province of Artemisa as a Category 3 storm on the afternoon of November 6, 2024. The hurricane approached the island from the south, having skirted past Jamaica the previous day as a tropical storm. Approaching Cuba, it traversed warm waters and encountered light to moderate vertical wind shear—environmental conditions that helped the storm to strengthen into a major hurricane.

Rafael’s sustained wind speeds peaked at 115 miles (185 kilometers) per hour prior to landfall, reported the National Hurricane Center (NHC). It weakened slightly upon encountering land, downgrading to a Category 2 storm as it moved across Cuba and tracked northwest into the Gulf of Mexico.

According to news reports, the Cuban government announced the hurricane had knocked out power across the entire island before landfall. Several airports suspended flights. Western Cuba was expected to receive 4 to 8 inches (100 to 200 millimeters) of rainfall from the storm system, according to the NHC, with several inches also forecast for the Cayman Islands and Florida Keys. The NHC also warned of strong storm surge that could raise water as much as 14 feet (about 4 meters) above normal levels along Cuba’s southern coast.

As of the morning of November 7, forecasters expected Rafael to move slowly to the west and remain a hurricane for several days, though it could weaken as it encounters a dry airmass in the southern Gulf of Mexico. The longer-term forecast remained uncertain.

Consistent with National Weather Service predictions, it has been an active year for hurricanes in the North Atlantic. Rafael is the 17th named storm and 11th hurricane of the 2024 season, which runs from June 1 to November 30. These numbers exceed the average seasonal totals of 14 named storms and seven hurricanes.

GOES-16 is the first of the GOES-R series of Geostationary Operational Environmental Satellites (GOES) operated by NASA and the National Oceanic and Atmospheric Administration (NOAA). GOES-16 serves as the operational geostationary weather satellite in the GOES East position at 75.2°W, providing a view centered on the Americas. GOES-16 provides high spatial and temporal resolution imagery of the Earth through 16 spectral bands at visible and infrared wavelengths using its Advanced Baseline Imager (ABI). GOES-16 was launched from Cape Canaveral in November 2016 aboard a United Launch Alliance (ULA) Atlas V rocket.


Image Credit: National Oceanic and Atmospheric Administration (NOAA)
NASA Article Credit: Lindsey Doermann
Release Date: Nov. 7, 2024


#NASA #NOAA #Space #Satellites #GOES16 #GOESEast #Science #Planet #Earth #Atmosphere #Meteorology #Weather #Oceans #AtlanticOcean #GulfOfMexico #Cuba #HurricaneRafael #SeaTemperatures #ClimateChange #GlobalHeating #Environment #CIRA #UnitedStates #STEM #Education #Timelapse #Animation #GIF

Ancient Impact Crater & 'Eye' of Quebec in Canada | Landsat 8 Satellite | USGS

Ancient Impact Crater & 'Eye' of Quebec in Canada | Landsat 8 Satellite | USGS

A large, round lake in Quebec, Canada, highlights the geography of an ancient impact crater. In the late Triassic Period, a 3 mile wide meteorite struck northern Pangea at over 30,000 miles per hour. The resulting crater is now 214 million years old, but the dramatic circular lake visible in 2024 Landsat imagery is a surprisingly recent feature.

It was the completion of the Daniel-Johnson Dam in 1968 that united two river systems, creating the Manicouagan Reservoir, or the Eye of Quebec. A declassified 1964 satellite image from the CIA’s Project Argon shows two crescent-shaped lakes originally outlining the impact zone. By 1972, the reservoir’s new water level had been established, as revealed by Landsat 1, with more or less the same shoreline it has today.

The Landsat program conceived of in the 1960s, has been running longer than any remote sensing program. The idea was simple: position a satellite in a nearly polar orbit fixed to the solar angle so that each daytime pass would cross the equator at roughly the same local time.

Data representing bands of the spectrum are captured and processed into grayscale recordings that can be combined to create natural looking views like this or false color views like this. Nine Landsat satellites have been launched in partnership with NASA since 1972.

The USGS EROS Center archive contains a wealth of satellite and digitized film imagery available at no cost to communities and scientists studying land change around the world: 

https://www.usgs.gov/centers/eros/science/usgs-eros-archive-products-overview

Official Quebec Tourism Website:

https://www.bonjourquebec.com/en

Côte-Nord: 

https://www.bonjourquebec.com/en/where-to-go/regions-of-quebec/cote-nord

Station Uapishka S.E.N.C.: 

https://www.bonjourquebec.com/en/listing/accommodation/station-uapishka-s-e-n-c/0a5a


Video Credit: United States Geological Survey (USGS)
Duration: 1 minute, 22 seconds
Release Date: Nov. 7, 2024

#NASA #USGS #Space #Planet #Earth #Geology #Meteorite #Pangea #ImpactCrater #Crater #ManicouaganReservoir #EyeOfQuebec #Quebec #Canada #Satellites #Landsat #Landsat8 #RemoteSensing #EarthObservation #EROS #SouthDakota #GSFC #UnitedStates #International #History #STEM #Education #HD #Video

Close-up: The 'Phantoms' of Star Gamma Cassiopeia—Nebulae IC 59 & IC 63

Close-up: The 'Phantoms' of Star Gamma Cassiopeia—Nebulae IC 59 & IC 63

These brightly outlined flowing shapes look ghostly on a cosmic scale. A telescopic view toward the constellation Cassiopeia, the colorful skyscape features the swept-back, comet-shaped clouds IC 59 (left) and IC 63. About 600 light-years distant, the clouds are not actually ghosts. They are slowly disappearing though, under the influence of energetic radiation from hot, luminous star gamma Cas. 

Gamma Cas is physically located only 3 to 4 light-years from the nebulae and lies just above the right edge of the frame. Slightly closer to gamma Cas, IC 63 is dominated by red H-alpha light emitted as hydrogen atoms ionized by the hot star's ultraviolet radiation recombine with electrons. Farther from the star, IC 59 shows less H-alpha emission but more of the characteristic blue tint of dust reflected star light. The field of view spans over 1 degree or 10 light-years at the estimated distance of the interstellar apparitions.


Image Credit & Copyright: Christophe Vergnes, Hervé Laur

Christophe's website: https://www.astrobin.com/users/Chris.V/

Release Date: Oct. 26, 2024


#NASA #Space #Astronomy #Science #Star #GammaCassiopeiae #GammaCas #Nebulas #Nebulae #IC59 #IC63 #Cassiopeia #MilkyWayGalaxy #Cosmos #Universe #Astrophotographers #ChristopheVergnes #HervéLaur #Astrophotography #STEM #Education #APoD

Wide Field View of Star Gamma Cassiopeia with Nebulae IC 59 & IC 63

Wide Field View of Star Gamma Cassiopeia with Nebulae IC 59 & IC 63

The bright bluish star shown here is Gamma Cassiopeiae. It is currently evaporating two nearby clouds of gas—nebulae IC 59 and IC 63. The leading edges of these clouds glow strongly in the intense bath of radiation from this hot star. Hints of bluish light behind the front lines of these nebulae show a bit of scattered light. Astronomically speaking, these clouds do not have much more time and will soon be blown away into the interstellar medium.

This image was taken as part of Advanced Observing Program (AOP) program at Kitt Peak Visitor Center.


Credit: KPNO/NOIRLab/NSF/AURA/Tom Bash and John Fox/Adam Block

Release Date: June 6, 2014


#NASA #Space #Astronomy #Science #Star #GammaCassiopeiae #GammaCas #Nebulae #Nebula #IC59 #IC63 #Cassiopeia #Constellation #MilkyWayGalaxy #Cosmos #Universe #KPNO #KittPeak #Tucson #Arizona #NOIRLab #AURA #NSF #UnitedStates #STEM #Education

The 'Ghosts' of Star Gamma Cassiopeia: Nebulae IC 59 & IC 63

The 'Ghosts' of Star Gamma CassiopeiaNebulae IC 59 & IC 63

Gamma Cassiopeiae shines high in northern autumn evening skies. It is the brightest spiky star in this telescopic field of view toward the constellation Cassiopeia. Gamma Cas shares the ethereal-looking scene with ghostly interstellar clouds of gas and dust, IC 59 and IC 63. About 600 light-years distant, the clouds are not actually ghosts. They are slowly disappearing though, eroding under the influence of energetic radiation from hot and luminous gamma Cas. Gamma Cas is physically located only 3 to 4 light-years from the nebulae. Slightly closer to gamma Cas, IC 63 is dominated by red H-alpha light emitted as hydrogen atoms ionized by the star's ultraviolet radiation recombine with electrons. Farther from the star, IC 59 shows proportionally less H-alpha emission but more of the characteristic blue tint of dust reflected star light. The cosmic stage spans over 1 degree or 10 light-years at the estimated distance of gamma Cas and friends.

Astrophotographer Markus Horn: "The area around the well-known 'Ghost of Cassiopeia' had been on my agenda for a while, and this year I was finally able to make it happen. Once again, I wanted to use my fast f/2 optics and a 400mm focal length to capture not only RGB data but also as much H-alpha signal as possible across the entire region. My goal was to show how deeply IC 63 and IC 59 are embedded within the H-alpha clouds. For this, I gathered 9.5 hours of RGB and 6.75 hours of H-alpha data."

"To ensure that the beautiful reflection nebulae of IC 63 and IC 59 weren’t completely overwhelmed by the narrowband data, I combined the H-alpha data in this area with the RGB data using continuum substraction. Finally, I invested a few more hours in finding a good balance between the RGB and narrowband components for the final image."

Image Details:
Celestron RASA 8 f/2
Celestron Motorfocus
EQ6-R Pro
ZWO ASI 2600 MC Pro (Gain 100, Offset 18, -10°)
RGB: 576 × 60″ (9h 36′)
TS 2600 MP (Gain 100, Offset 200, -10°)
Baader H-Alpha Highspeed 3.5nm: 202 × 120″ (6h 44')
Total: 16h 20'
Bortle 5 (19.50 SQM)
N.I.N.A., Guiding: ASI 120MM & PHD2
Astropixelprocessor, Photoshop, Pixinsight

Image Credit: Markus Horn
Release Date: Nov. 7, 2024

#NASA #Space #Astronomy #Science #Star #GammaCassiopeiae #GammaCas #Nebulae #Nebula #IC59 #IC63 #Cassiopeia #MilkyWayGalaxy #Cosmos #Universe #Astrophotographer #MarkusHorn #Astrophotography #STEM #Education

Star Trail Photography: Sunset to Sunrise | International Space Station

Star Trail Photography: Sunset to Sunrise | International Space Station

NASA astronaut Don Pettit: "This 30-minute time exposure through orbital night with our new 15mm wide-angle lens was able to capture sunset (on the left) all the way to sunrise (on the right). I have never been able to capture this before but our new fast (14mm f1.4 and 15mm T1.8) wide-angle lenses are opening up observations previously not possible. Visible are circular star trails above the earth limb created not from Earth rotation but from our orbital motion (pitch axis of ISS), cities streaking by (again due to orbital motion), lightning flashes, aurora, atmospheric airglow (both strong green and fainter red). Stay tuned for more of these."

Image details: Nikon Z9, Arri-Zeiss 15mm T1.8 master prime lens, 30 seconds at T1.8 for individual exposures assembled with Photoshop into a composite equivalent to a 30-minute exposure, ISO 200, adjusted for levels, contrast, color, and spot removal. With our current 8-year-old laptops, I cannot perform dark frame subtraction followed by robust denoise operations (would take about 30 hours run time for a single composition where cosmic rays would probably require a re-boot in the process), so clean, finished photographs will have to wait until I return to Earth."

Expedition 72 Updates:

https://blogs.nasa.gov/spacestation/

Expedition 72 Crew

Station Commander: Suni Williams

Roscosmos (Russia): Alexey Ovchinin, Ivan Vagner, Aleksandr Gorbunov

NASA: Butch Wilmore, Don Pettit, Nick Hague

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 Date: NASA's Johnson Space Center (JSC)

Release Date: Nov. 7, 2024


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Aurora Dome over Labrador

Aurora Dome over Labrador


Astrophotographer Adam Woodworth: "During the intense aurora on October 10, 2024, my buddy Steve Sheppard and I experienced the most amazing display of aurora that either of us had ever seen. For most of the night the aurora was clearly visible in the sky but still faint enough that you could barely make out some green color with the naked eye. But at one point the sky exploded with bright colors and we were under a horizon to horizon 360 degree dome of aurora for a few minutes. It was so bright it lit up the ground, and we could clearly see color all across the sky . . ."

Image Details: Nikon Z 6 with Sigma 14mm f/1.8 lens @ f/1.8, ISO 1250, 2 seconds for all exposures in this panorama

Labrador is a geographic region within the Canadian province of Newfoundland and Labrador.

On Earth, auroras are mainly created by particles originally emitted by the Sun in the form of solar wind. When this stream of electrically charged particles gets close to our planet, it interacts with the magnetic field, which acts as a gigantic shield. While it protects Earth’s environment from solar wind particles, it can also trap a small fraction of them. Particles trapped within the magnetosphere—the region of space surrounding Earth in which charged particles are affected by its magnetic field—can be energized and then follow the magnetic field lines down to the magnetic poles. There, they interact with oxygen and nitrogen atoms in the upper layers of the atmosphere, creating the flickering, colorful lights visible in the polar regions here on Earth.

Earth auroras have different names depending on which pole they occur at. Aurora Borealis, or the northern lights, is the name given to auroras around the north pole and Aurora Australis, or the southern lights, is the name given for auroras around the south pole.

Learn more:
The Colors of the Aurora (National Park Service)
https://www.nps.gov/articles/-articles-aps-v8-i1-c9.htm


Image Credit & Copyright: Adam Woodworth
Adam's website: https://www.adamwoodworth.com
Image Date: Oct. 10, 2024
Release Date: Nov. 6, 2024

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NASA X-59 Research Aircraft Fires Up its Engine for First Time

NASA X-59 Research Aircraft Fires Up its Engine for First Time

NASA’s X-59 quiet supersonic research aircraft sits in its run stall at Lockheed Martin’s Skunk Works facility in Palmdale, California, firing up its engine for the first time. These engine-run tests start at low power and allow the X-59 team to verify the aircraft’s systems are working together while powered by its own engine. 
Direct view of the front of the X-59 aircraft, mostly in the shade of a run stall. Flaps on both wings are activated, moving downward. Team members wear protective ear guards and look at the aircraft from both sides. NASA’s 100-foot-long X-59 sits in the run stall with the engine and the rest of the back of the aircraft sitting outside the run stall’s open bay door at Lockheed Martin’s Skunk Works facility in Palmdale, California, prior to its first engine run. Engine runs are part of a series of integrated ground tests needed to ensure safe flight and successful achievement of mission goals.
View of an aircraft cockpit inside a run stall. The canopy atop the cockpit is open. Inside, a pilot looks at his instruments as he wears a helmet and oxygen mask. The white, gold, and blue paint scheme of the NASA aircraft is prominent. Lockheed Martin test pilot Dan Canin sits in the cockpit of NASA’s X-59 quiet supersonic research aircraft in a run stall at Lockheed Martin’s Skunk Works facility in Palmdale, California prior to its first engine run.

NASA’s Quesst mission marked a major milestone with the start of tests on the engine that will power the quiet supersonic X-59 experimental aircraft.

These engine-run tests started on Oct. 30, 2024. They allow the X-59 team to verify the aircraft’s systems are working together while powered by its own engine. In previous tests, the X-59 used external sources for power. The engine-run tests set the stage for the next phase of the experimental aircraft’s progress toward flight.

The X-59 team is conducting the engine-run tests in phases. In this first phase, the engine rotated at a relatively low speed without ignition to check for leaks and ensure all systems are communicating properly. The team then fueled the aircraft and began testing the engine at low power, with the goal of verifying that it and other aircraft systems operate without anomalies or leaks while on engine power.

“The first phase of the engine tests was really a warmup to make sure that everything looked good prior to running the engine,” said Jay Brandon, NASA’s X-59 chief engineer. “Then we moved to the actual first engine start. That took the engine out of the preservation mode that it had been in since installation on the aircraft. It was the first check to see that it was operating properly and that all the systems it impacted—hydraulics, electrical system, environmental control systems, etc.—seemed to be working.”

The X-59 will generate a quieter thump rather than a loud boom while flying faster than the speed of sound. The aircraft is the centerpiece of NASA’s Quesst mission. It will gather data on how people perceive these thumps, providing regulators with information that could help lift current bans on commercial supersonic flight over land.

The engine, a modified F414-GE-100, packs 22,000 pounds of thrust. This will enable the X-59 to achieve the desired cruising speed of Mach 1.4 (925 miles per hour) at an altitude of approximately 55,000 feet. It sits in a nontraditional spot–atop the aircraft—to aid in making the X-59 quieter.

Engine runs are part of a series of integrated ground tests needed to ensure safe flight and successful achievement of mission goals. Because of the challenges involved with reaching this critical phase of testing, the X-59’s first flight is now expected in early 2025. The team will continue progressing through critical ground tests and address any technical issues discovered with this one-of-a-kind, experimental aircraft. The X-59 team will have a more specific first flight date as these tests are successfully completed.

The testing is taking place at Lockheed Martin’s Skunk Works facility in Palmdale, California. During later phases, the team will test the aircraft at high power with rapid throttle changes, followed by simulating the conditions of an actual flight.

“The success of these runs will be the start of the culmination of the last eight years of my career,” said Paul Dees, NASA’s deputy propulsion lead for the X-59. “This isn’t the end of the excitement but a small steppingstone to the beginning. It’s like the first note of a symphony, where years of teamwork behind the scenes are now being put to the test to prove our efforts have been effective, and the notes will continue to play a harmonious song to flight.”

After the engine runs, the X-59 team will move to aluminum bird testing, where data will be fed to the aircraft under both normal and failure conditions. The team will then proceed with a series of taxi tests, where the aircraft will be put in motion on the ground. These tests will be followed by final preparations for first flight.

The X-59's goal is to help change existing national and international aviation rules that ban commercial supersonic flight over land.

Learn more here:

https://www.nasa.gov/mission/quesst/

https://www.nasa.gov/flightlog

X-59 Free Maker Bundle (STEM Education):

https://www.nasa.gov/sites/default/files/atoms/files/x-59-maker-bundle-v8.pdf


Image Credit: NASA/Carla Thomas
Article Credit: NASA Langley
Release Date: Nov. 6, 2024


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