The Heart Nebula
Talon Abraxas
The Heart Nebula is an emission nebula located in the constellation of Cassiopeia, around 7,500 light years away from Earth. It has an apparent magnitude of 18.3 and an absolute magnitude of 6.5. Sometimes, it is known as the Running Dog Nebula because, when seen through a telescope, it looks a bit like a running dog.
The nebula was given its name the Heart Nebula because of its intensely red glowing gas and dark dust lanes that form a shape that resembles a heart symbol. It forms a famous complex known as the Heart and Soul with its smaller neighbour Westerhout 5, also known as the Soul Nebula, which lies just 2.5 degrees to the southeast.
The Heart Nebula is around 150 arcminutes in size and has been given the designation of Sharpless 2-190 in the Sharpless Catalogue, as well as IC 1805. The brightest part of the Heart Nebula has the designation NGC 896 in the New General Catalogue. It is classified separately because it was the first part of IC 1805 to be discovered.
The glow of the nebula comes from the radiation of a small open cluster of stars known as Melotte 15. The cluster contains very young, blue, hot supergiant stars that are about 1.5 million years old and is located near the nebula’s centre.
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2023 December 13
Deep Field: The Heart Nebula
Image Credit & Copyright: William Ostling, Telescope Live
Explanation: What excites the Heart Nebula? First, the large emission nebula on the left, catalogued as IC 1805, looks somewhat like a human heart. The nebula glows brightly in red light emitted by its most prominent element, hydrogen, but this long-exposure image was also blended with light emitted by silicon (yellow) and oxygen (blue). In the center of the Heart Nebula are young stars from the open star cluster Melotte 15 that are eroding away several picturesque dust pillars with their atom-exciting energetic light and winds. The Heart Nebula is located about 7,500 light years away toward the constellation of Cassiopeia. At the bottom right of the Heart Nebula is the companion Fishhead Nebula. This wide and deep image clearly shows, though, that glowing gas surrounds the Heart Nebula in all directions.
∞ Source: apod.nasa.gov/apod/ap231213.html
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In the Heart of the Heart Nebula
“You’ll be given love. You’ll be taken care of. You have to trust it. Maybe not from the sources you have poured yours. Maybe not from the directions you are staring at. Twist your head around. It’s all around you. All is full of love.”
The Heart Nebula, or IC 1805, is a beautiful emission nebula located 7,500 light-years away in the constellation Cassiopeia. Discovered by William Herschel in 1787, it's characterized by glowing ionized hydrogen and dark molecular dust. The nebula's distinctive red color and dramatic shape are due to radiation from the nearby star cluster Melotte 15, which contains stars about 50 times brighter than our sun. A
Heart for Valentina
--Mahaboka
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The Heart Nebula on the right (IC 1805, Sharpless 2-190) and Soul Nebula, left, (Westerhout 5 with the star cluster IC 1848) in Hydrogen-alpha. These two make up a massive star-forming complex in Cassiopeia about 7500 lightyears away in the Perseus Arm of our Galaxy. The bright emission nebula on the far right is the Fishhead Nebula (NGC 896, IC 1795). The small circular cloud, middle top, is another emission nebula Sh2-198, much further away, around 18,000 lightyears (still, well within the galaxy). The bright cluster of stars in the core of the Heart Nebula is Melotte 15.
Imaging Notes: 51 x 5-minute exposures stacked in PI, ZWO ASI2600MM-Pro monochrome camera cooled to -10C, 3nm Antlia Pro Hydrogen-alpha filter, William Optics SpaceCat 51 apo refractor, Sky-Watcher EQ6-R Pro mount. Shot from my backyard in coastal New Hampshire, bortle 4-ish.
https://SaltwaterWitch.com
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Follow here and never miss another James Webb Telescope Discovery. Chronological List of All James Webb Space Telescope Discoveries since the release of first images in July, 2022
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04-06-2023 - James Webb Telescope Reveals Unprecedented Image of Uranus and its Features. Full article here
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01-23-2023 - New James Webb Discovery find Complex Organic Molecules in Pre-Stellar Ice. Full article here
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01-09-2023 - Webb Telescope Discovers Connections Between Nearby and Faraway Galaxies. Full article here
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12-01-2022 - The Largest moon of Saturn known as Titan imaged by the Webb Telescope. Full article here
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08-22-2022 - James Webb Telescope captures images of Jupiter in great detail. Full article here
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APOD December 13, 2023
Deep Field: The Heart Nebula
What excites the Heart Nebula? First, the large emission nebula on the left, catalogued as IC 1805, looks somewhat like a human heart. The nebula glows brightly in red light emitted by its most prominent element, hydrogen, but this long-exposure image was also blended with light emitted by silicon (yellow) and oxygen (blue). In the center of the Heart Nebula are young stars from the open star cluster Melotte 15 that are eroding away several picturesque dust pillars with their atom-exciting energetic light and winds. The Heart Nebula is located about 7,500 light years away toward the constellation of Cassiopeia. At the bottom right of the Heart Nebula is the companion Fishhead Nebula. This wide and deep image clearly shows, though, that glowing gas surrounds the Heart Nebula in all directions.
©
William Ostling,
Telescope Live
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