View allAll Photos Tagged helixnebula
This infrared image from NASA's Spitzer Space Telescope shows the Helix nebula, a cosmic starlet often photographed by amateur astronomers for its vivid colors and eerie resemblance to a giant eye.
The nebula, located about 700 light-years away in the constellation Aquarius, belongs to a class of objects called planetary nebulae. Discovered in the 18th century, these cosmic butterflies were named for their resemblance to gas-giant planets.
Planetary nebulae are actually the remains of stars that once looked a lot like our sun.
When sun-like stars die, they puff out their outer gaseous layers. These layers are heated by the hot core of the dead star, called a white dwarf, and shine with infrared and visible-light colors. Our own sun will blossom into a planetary nebula when it dies in about five billion years.
In Spitzer's infrared view of the Helix nebula, the eye looks more like that of a green monster's. Infrared light from the outer gaseous layers is represented in blues and greens. The white dwarf is visible as a tiny white dot in the center of the picture. The red color in the middle of the eye denotes the final layers of gas blown out when the star died.
The brighter red circle in the very center is the glow of a dusty disk circling the white dwarf (the disk itself is too small to be resolved). This dust, discovered by Spitzer's infrared heat-seeking vision, was most likely kicked up by comets that survived the death of their star. Before the star died, its comets and possibly planets would have orbited the star in an orderly fashion. But when the star blew off its outer layers, the icy bodies and outer planets would have been tossed about and into each other, resulting in an ongoing cosmic dust storm. Any inner planets in the system would have burned up or been swallowed as their dying star expanded.
The Helix nebula is one of only a few dead-star systems in which evidence for comet survivors has been found.
This image is made up of data from Spitzer's infrared array camera and multiband imaging photometer. Blue shows infrared light of 3.6 to 4.5 microns; green shows infrared light of 5.8 to 8 microns; and red shows infrared light of 24 microns.
This comparison shows a new view of the Helix Nebula acquired with the VISTA telescope in infrared light (left) and the more familiar view in visible light from the MPG/ESO 2.2-metre telescope (right). The infrared vision of VISTA reveals strands of cold nebular gas that are mostly obscured in visible light images of the Helix.
First target from Okie-Tex this past week. I was able to image 2 targets per night over multiple nights. Had some PC problems and slight breezes affects my system so had some issues with tracking hence it took 3 nights for this target. 27 x 5min subs. DSLR is not cooled which I think would have helped this set. Even though the nights were cool, colder is better. Stacked in Nebulosity. First time to process primarily in Photoshop.
Orion 190mm Mak-Newt
iEQ45
Canon 60D (modified)
Orion 80mm short tube w/ SSAG
This infrared image from NASA's Spitzer Space Telescope shows the Helix nebula, a cosmic starlet often photographed by amateur astronomers for its vivid colors and eerie resemblance to a giant eye.
The nebula, located about 700 light-years away in the constellation Aquarius, belongs to a class of objects called planetary nebulae. Discovered in the 18th century, these cosmic butterflies were named for their resemblance to gas-giant planets.
Planetary nebulae are actually the remains of stars that once looked a lot like our sun.
When sun-like stars die, they puff out their outer gaseous layers. These layers are heated by the hot core of the dead star, called a white dwarf, and shine with infrared and visible-light colors. Our own sun will blossom into a planetary nebula when it dies in about five billion years.
In Spitzer's infrared view of the Helix nebula, the eye looks more like that of a green monster's. Infrared light from the outer gaseous layers is represented in blues and greens. The white dwarf is visible as a tiny white dot in the center of the picture. The red color in the middle of the eye denotes the final layers of gas blown out when the star died.
The brighter red circle in the very center is the glow of a dusty disk circling the white dwarf (the disk itself is too small to be resolved). This dust, discovered by Spitzer's infrared heat-seeking vision, was most likely kicked up by comets that survived the death of their star. Before the star died, its comets and possibly planets would have orbited the star in an orderly fashion. But when the star blew off its outer layers, the icy bodies and outer planets would have been tossed about and into each other, resulting in an ongoing cosmic dust storm. Any inner planets in the system would have burned up or been swallowed as their dying star expanded.
The Helix nebula is one of only a few dead-star systems in which evidence for comet survivors has been found.
This image is made up of data from Spitzer's infrared array camera and multiband imaging photometer. Blue shows infrared light of 3.6 to 4.5 microns; green shows infrared light of 5.8 to 8 microns; and red shows infrared light of 24 microns.
Edited European Southern Observatory image of the Helix Nebula. Color/processing variant.
Original caption: ESO's Visible and Infrared Survey Telescope for Astronomy (VISTA) has captured this unusual view of the Helix Nebula (NGC 7293), a planetary nebula located 700 light-years away. The coloured picture was created from images taken through Y, J and K infrared filters. While bringing to light a rich background of stars and galaxies, the telescope's infrared vision also reveals strands of cold nebular gas that are mostly obscured in visible images of the Helix.
This composite image is a view of the colorful Helix Nebula taken with the Advanced Camera for Surveys aboard NASA/ESA Hubble Space Telescope and the Mosaic II Camera on the 4-meter telescope at Cerro Tololo Inter-American Observatory in Chile. The object is so large that both telescopes were needed to capture a complete view. The Helix is a planetary nebula, the glowing gaseous envelope expelled by a dying, sun-like star. The Helix resembles a simple doughnut as seen from Earth. But looks can be deceiving. New evidence suggests that the Helix consists of two gaseous disks nearly perpendicular to each other.
Credit:
NASA, ESA, C.R. O'Dell (Vanderbilt University), and M. Meixner, P. McCullough, and G. Bacon ( Space Telescope Science Institute)
Using layer blending , the clone tool, and appropriated images from the Hubble telescope (tarantula nebula, helix nebula), as well as two images of my boyfriend's eye; I created a portrait of sorts..
Edited Chandra Space Telescope and Hubble Space Telescope image of the Helix Nebula. Color/processing variant.
Image source: www.nasa.gov/mission_pages/chandra/news/nasas-chandra-ope...
Original caption: When a star like the Sun runs out of fuel, it expands and its outer layers puff off, and then the core of the star shrinks. This phase is known as a "planetary nebula," and astronomers expect our Sun will experience this in about 5 billion years. This Helix Nebula images contains infrared data from NASA's Spitzer Space Telescope (green and red), optical light from Hubble (orange and blue), ultraviolet from NASA's Galaxy Evolution Explorer (cyan), and Chandra's X-rays (appearing as white) showing the white dwarf star that formed in the center of the nebula. The image is about four light years across.
These gigantic, tadpole-shaped objects are probably the result of a dying star's last gasps. Dubbed "cometary knots" because their glowing heads and gossamer tails resemble comets, the gaseous objects probably were formed during a star's final stages of life. Hubble astronomer C. Robert O'Dell and graduate student Kerry P. Handron of Rice University in Houston, Texas discovered thousands of these knots with the Hubble Space Telescope while exploring the Helix nebula, the closest planetary nebula to Earth at 450 light-years away in the constellation Aquarius. Although ground-based telescopes have revealed such objects, astronomers have never seen so many of them. The most visible knots all lie along the inner edge of the doomed star's ring, trillions of miles away from the star's nucleus. Although these gaseous knots appear small, they're actually huge. Each gaseous head is at least twice the size of our solar system; each tail stretches for 100 billion miles, about 1,000 times the distance between the Earth and the Sun. Astronomers theorize that the doomed star spews hot, lower-density gas from its surface, which collides with cooler, higher-density gas that had been ejected 10,000 years before. The crash fragments the smooth cloud surrounding the star into smaller, denser finger-like droplets, like dripping paint. This image was taken in August, 1994 with Hubble's Wide Field Planetary Camera 2. The red light depicts nitrogen emission ([NII] 6584A); green, hydrogen (H-alpha, 6563A); and blue, oxygen (5007A).
Takahashi FS102 with ZWO ASI533 MC-Pro.
Optolong L-Enhance filter.
All on an ancient Orion Atlas EQ-G Goto mount. Guided and run with ZWO ASIAir. Post processed in Astro Pixel Processor and Photoshop CS3.
The Helix Nebula, which is composed of gaseous shells and disks puffed out by a dying sunlike star, exhibits complex structure on the smallest visible scales. In this new image from NASA's Spitzer Space Telescope, infrared light at wavelengths of 3.6, 4.5, and 8.0 microns has been colored blue, green, and red (respectively). The color saturation also has been increased to intensify hues. The "cometary knots" show blue-green heads due to excitation of their molecular material from shocks or ultraviolet radiation. The tails of the cometary knots appear redder due to being shielded from the central star's ultraviolet radiation and wind by the heads of the knots.
Edited Chandra Space Telescope and Hubble Space Telescope image of the Helix Nebula. Inverted grayscale variant.
Image source: www.nasa.gov/mission_pages/chandra/news/nasas-chandra-ope...
Original caption: When a star like the Sun runs out of fuel, it expands and its outer layers puff off, and then the core of the star shrinks. This phase is known as a "planetary nebula," and astronomers expect our Sun will experience this in about 5 billion years. This Helix Nebula images contains infrared data from NASA's Spitzer Space Telescope (green and red), optical light from Hubble (orange and blue), ultraviolet from NASA's Galaxy Evolution Explorer (cyan), and Chandra's X-rays (appearing as white) showing the white dwarf star that formed in the center of the nebula. The image is about four light years across.
Edited Chandra Space Telescope and Hubble Space Telescope image of the Helix Nebula. Color/processing variant.
Image source: www.nasa.gov/mission_pages/chandra/news/nasas-chandra-ope...
Original caption: When a star like the Sun runs out of fuel, it expands and its outer layers puff off, and then the core of the star shrinks. This phase is known as a "planetary nebula," and astronomers expect our Sun will experience this in about 5 billion years. This Helix Nebula images contains infrared data from NASA's Spitzer Space Telescope (green and red), optical light from Hubble (orange and blue), ultraviolet from NASA's Galaxy Evolution Explorer (cyan), and Chandra's X-rays (appearing as white) showing the white dwarf star that formed in the center of the nebula. The image is about four light years across.
This infrared image from NASA's Spitzer Space Telescope shows the Helix nebula, a cosmic starlet often photographed by amateur astronomers for its vivid colors and eerie resemblance to a giant eye.
The nebula, located about 700 light-years away in the constellation Aquarius, belongs to a class of objects called planetary nebulae. Discovered in the 18th century, these cosmic butterflies were named for their resemblance to gas-giant planets.
Planetary nebulae are actually the remains of stars that once looked a lot like our sun.
When sun-like stars die, they puff out their outer gaseous layers. These layers are heated by the hot core of the dead star, called a white dwarf, and shine with infrared and visible-light colors. Our own sun will blossom into a planetary nebula when it dies in about five billion years.
In Spitzer's infrared view of the Helix nebula, the eye looks more like that of a green monster's. Infrared light from the outer gaseous layers is represented in blues and greens. The white dwarf is visible as a tiny white dot in the center of the picture. The red color in the middle of the eye denotes the final layers of gas blown out when the star died.
The brighter red circle in the very center is the glow of a dusty disk circling the white dwarf (the disk itself is too small to be resolved). This dust, discovered by Spitzer's infrared heat-seeking vision, was most likely kicked up by comets that survived the death of their star. Before the star died, its comets and possibly planets would have orbited the star in an orderly fashion. But when the star blew off its outer layers, the icy bodies and outer planets would have been tossed about and into each other, resulting in an ongoing cosmic dust storm. Any inner planets in the system would have burned up or been swallowed as their dying star expanded.
The Helix nebula is one of only a few dead-star systems in which evidence for comet survivors has been found.
This image is made up of data from Spitzer's infrared array camera and multiband imaging photometer. Blue shows infrared light of 3.6 to 4.5 microns; green shows infrared light of 5.8 to 8 microns; and red shows infrared light of 24 microns.
Credit: NASA/JPL-Caltech/Univ. of Ariz.
Edited Chandra Space Telescope and Hubble Space Telescope image of the Helix Nebula. Color/processing variant.
Image source: www.nasa.gov/mission_pages/chandra/news/nasas-chandra-ope...
Original caption: When a star like the Sun runs out of fuel, it expands and its outer layers puff off, and then the core of the star shrinks. This phase is known as a "planetary nebula," and astronomers expect our Sun will experience this in about 5 billion years. This Helix Nebula images contains infrared data from NASA's Spitzer Space Telescope (green and red), optical light from Hubble (orange and blue), ultraviolet from NASA's Galaxy Evolution Explorer (cyan), and Chandra's X-rays (appearing as white) showing the white dwarf star that formed in the center of the nebula. The image is about four light years across.
A newly expanded image of the Helix nebula lends a festive touch to the fourth anniversary of the launch of NASA's Spitzer Space Telescope. This spectacular object, a dying star unraveling into space, is a favorite of amateur and professional astronomers alike. Spitzer has mapped the expansive outer structure of the six-light-year-wide nebula, and probed the inner region around the central dead star to reveal what appears to be a planetary system that survived the star's chaotic death throes.
Edited Chandra Space Telescope and Hubble Space Telescope image of the Helix Nebula. Color/processing variant.
Image source: www.nasa.gov/mission_pages/chandra/news/nasas-chandra-ope...
Original caption: When a star like the Sun runs out of fuel, it expands and its outer layers puff off, and then the core of the star shrinks. This phase is known as a "planetary nebula," and astronomers expect our Sun will experience this in about 5 billion years. This Helix Nebula images contains infrared data from NASA's Spitzer Space Telescope (green and red), optical light from Hubble (orange and blue), ultraviolet from NASA's Galaxy Evolution Explorer (cyan), and Chandra's X-rays (appearing as white) showing the white dwarf star that formed in the center of the nebula. The image is about four light years across.
This composite image is a view of the colorful Helix Nebula taken with the Advanced Camera for Surveys aboard NASA/ESA Hubble Space Telescope and the Mosaic II Camera on the 4-meter telescope at Cerro Tololo Inter-American Observatory in Chile. The object is so large that both telescopes were needed to capture a complete view. The Helix is a planetary nebula, the glowing gaseous envelope expelled by a dying, sun-like star. The Helix resembles a simple doughnut as seen from Earth. But looks can be deceiving. New evidence suggests that the Helix consists of two gaseous disks nearly perpendicular to each other.
The Helix Nebula, NGC 7293, in Aquarius. 22 hours of S2/Ha/O3 imaging with 235-mm SCT and 0.7x reducer.
A newly expanded image of the Helix nebula lends a festive touch to the fourth anniversary of the launch of NASA's Spitzer Space Telescope. This spectacular object, a dying star unraveling into space, is a favorite of amateur and professional astronomers alike. Spitzer has mapped the expansive outer structure of the six-light-year-wide nebula, and probed the inner region around the central dead star to reveal what appears to be a planetary system that survived the star's chaotic death throes.
What should have been a great clear night of imaging was a bit of a let down. This was the best I could retrieve from the data what with the scope slipping focus slightly on the Eagle nebula plus me trying to capture things too low down and into the light polution. I think I also balls-ed up my flat frames as there's a noticeable light gradient in this shot which should be averaged out. Unfortunately, as the weather has been so cloudy for the last 6 weeks, I've missed a whole load of interesting subjects for this year, they're all sinking too low after dark.
20 x 180s Lights
9 Darks
20 Flats
20 Bias
Skywatcher Evo100ED + 0.85 reducer/flattener
Skywatcher HEQ5Pro with EQMOD and PHD2 guiding
Altair Astro 60mm guidescope with GPCAM3 385C
Nikon D5100 astro-mod DSLR @ISO1600
IDAS D2 Light Pollution Suppression Filter
The NASA/ESA Hubble Space Telescope has captured the sharpest view yet of the most famous of all planetary nebulae: the Ring Nebula (M57). In this October 1998 image, the telescope has looked down a barrel of gas cast off by a dying star thousands of years ago. This photo reveals elongated dark clumps of material embedded in the gas at the edge of the nebula; the dying central star floating in a blue haze of hot gas. The nebula is about a light-year in diameter and is located some 2, 000 light-years from Earth in the direction of the constellation Lyra.
E-PL6, "Newton ohne Namen 200/800flat" ISO640 40x4 Minuten bei sehr schlechtem hellen Himmel anhe am Horizont
Unser nächster planetarischer Nebel, ca 670 LJ weit weg und so groß wie der Mond am Himmel erscheint
Uma das nebulosas planetárias mais famosas, se não a mais famosa. Conhecida popularmente como "Olho de Deus", ela é a NGC7293 ou Nebulosa de Helix. Seu formato se assemelha a um olho e ela é relativamente grande no céu. Essa é minha segunda captura desse objeto, já que a primeira ficou estranha, provavelmente por conta do orvalho. Gostei do resultado e vocês? Captura feita em num local Bortle 4, o @Bregildo_Camping e foi utilizado filtro L-Pro.
One of the most famous planetary nebulae. Popularly known as "The eye of god" its the NGC7293 or Helix Nebula. Its shape looks like an eye an its relatively big in the sky. This is my second attempt of this object. The first one looked weird, probably because of the dew and humidity. I really liked it, what about you? Capture made on a Bortle 4 site, the @Bregildo_Camping using a L-Pro filter.
Canon SL2 modified, Sky-Watcher 200p (200/1000mm), ISO 1600. Guiding with Asiair and ASI290mc in an adapted finderscope 50mm, Eq5 Sky-watcher mount and AstroEq tracking mod. 38 Ligth Frames of 180s, 45 darks and 50 bias. 1h54 minutes total exposure. Used Optolong L-Pro filter. Processing on Pixinsight.
#astrophotography #astrofotografia #nightsky #astronomy #astromomia #CanonSL2 #dslrmod #telescopio #telescope #skywatcher #skywatcher200p #Eq5 #skywatcherEq5 #AstroEq #DeepSkyStacker #deepsky #adobephotoshop #pixinsight #asi290mc #ZwoAsi #zwoasi290mc #longexposure #NGC7293 #helix #helixnebula #asiair #guiding #lpro #optolonglpro #astfotbr
PID 2211, 2023-10-31
NGC 7293 Helix Nebula - Southern edge:
22:29:41.008 -20:57:41.08
F200W Cyan
F277W Orange
The helix nebula is one of the brightest planetary nebula in the sky due to its close proximity, only 655 light years away. It look like the Eye of Sauron but is in fact is the death throws of a star at the end of its life as it sheds its outer layers.
Helix Nebula (IC 7293), 09/03/2021
Headed up to my buddy’s property in Orofino Idaho last weekend for some light boozing and shenanigans with a bunch of friends. I took the telescope as well on the off chance there were clear skies, and I wasn’t too far gone to use it. On the first night I was able to capture this before skies and my brain got too hazy to do any more.
This is the Helix Nebula. For obvious reasons it is very often called the “Eye of God” nebula. It is found in the constellation Aquarius and is probably the nearest planetary nebula to our Solar System, located roughly 650 light years away. Based on its size, age and distance it is expanding in size at 19 miles per second. My back of the envelope math estimates that is as fast as traveling to the moon in under 3.5 minutes.
Equipment:
RASA 8
iOptron GEM45
ZWO ASI294MC-Pro
ZWO Asiair Pro
Optolong L-Pro filter
Details:
Location – Chris’s property in Idaho
Bortle Class 3
Gain 120
120 60-second Lights
30 Darks
30 Bias
30 Dark Flats
Astro Pixel Processor
StarNet++
Lightroom
Photoshop
#astrophotography #astronomy #comos #nightphotography #space #telescope #deepsky #asi294mcpro #amateurastronomy #backyardastronomy #asiair #asiairpro #rasa #celestron #ioptrongem45 #astropixelprocessor #optolong #deepskyobject #zwo #longexposurephotography #astronomyphotography #IC7293 #HelixNebula #Eyeofgod #Eyeofgodnebula
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This composite image is a view of the colorful Helix Nebula taken with the Advanced Camera for Surveys aboard NASA/ESA Hubble Space Telescope and the Mosaic II Camera on the 4-meter telescope at Cerro Tololo Inter-American Observatory in Chile. The object is so large that both telescopes were needed to capture a complete view. The Helix is a planetary nebula, the glowing gaseous envelope expelled by a dying, sun-like star. The Helix resembles a simple doughnut as seen from Earth. But looks can be deceiving. New evidence suggests that the Helix consists of two gaseous disks nearly perpendicular to each other.