The Horsehead Nebula was discovered by Mrs. Williamina Fleming on Harvard College Observatory Bache Telescope plate B2312, noted by Professor E. C. Pickering in his Harvard Annals publication of new objects discovered by Photography at Harvard in Cambridge, Massachusetts, published in 1890. The discovery was made by her on June 27, 1888, and the plate was exposed on February 6, 1888. It was Mrs. Fleming's job to examine and analyze the photographs for details and possible new objects. Professor Pickering also reported that his brother, William, had immediately speculated that the nebula consisted of dark, obscuring matter: and thus from the very beginning, the correct scientific nature of the phenomenon was comprehended.
However, though the large bright nebula IC-434, upon which the Horsehead is superimposed on Earth's line of sight, was catalogued in 1895 (with a mistaken attribution to "Pickering", not Fleming), the Horsehead itself was not generally acknowledged in astronomical catalogues for some years, until Edward E. Barnard included it as his item no. 33 in a paper containing a list of 182 dark 'markings', published in 1919. Though others photographed the Horsehead after 1891, Barnard was apparently the first person to observe and study it visually, in 1913.
Stephen Waldee, a California amateur astronomer and researcher, turned up the forgotten and unacknowledged facts in the old Harvard publication and -- with the cooperation of Martha Hazen, Curator of Harvard's Historical Photographs -- the original plate, during a research project in 1989/90. The saga of Mrs. Fleming's work on the nebula and other such objects discovered in Harvard's early photographic program was chronicled and published over the next few years, in a joint Waldee-Hazen paper, a magazine article, and eventually a large research website. Mrs. Fleming's work was finally professionally recognized (unfortunately not her Horsehead discovery!) in 1908, with the publication of the second Index Catalogue; she found no fewer than 59 gaseous nebulae on various Harvard photographs made in Massachusetts and Arequipa, Peru. In addition she discovered novae and hundreds of variable stars. But her seminal discovery of the Horsehead was not understood prior to the Waldee-Hazen paper of 1990. -- Stephen R. Waldee
The Horsehead Nebula can be found in the constellation Orion. Its name comes from its resemblance to a horse's head. The Horsehead Nebula was first discovered by Williamina Fleming in 1888.
No, the Horsehead Nebula is a dark nebula in the constellation Orion and does not have any moons. Moons are natural satellites that orbit planets, whereas nebulae are large clouds of gas and dust in outer space.
Horsehead Nebula doesn't glow like other nebulae because it is older than other nebulae and was probably a lot smaller. In addition, Horsehead Nebula is farther away from the Earth than other nebulae, so it may seem that it doesn't glow as bright as other nebulae. No, this isn't right! The horsehead nebula doesn't glow for one reason - it isn't illuminated by any stars whose energy is enough to make the gas shine. That's the only difference between a 'bright' diffuse nebula (like M42) and a 'dark' one like the Horsehead or the Coalsack. M42 (the Orion nebula) is bright because there are several hot, energetic stars embedded inside it, and which cause it to 'shine'.
The Horsehead Nebula is located in the Orion constellation, specifically within the Orion Molecular Cloud Complex. It lies approximately 1,500 light-years away from Earth and is part of the Milky Way galaxy's Orion Arm, which is a minor spiral arm. The nebula is a region of star formation, characterized by its distinctive dark silhouette against the background glow of ionized gas and nearby stars.
The two most well-known nebulae are the Orion Nebula and the Crab Nebula. The Orion Nebula is one of the brightest nebulae and is visible to the naked eye, located in the Orion constellation. The Crab Nebula is the remnant of a supernova explosion observed by Chinese astronomers in 1054 AD, located in the Taurus constellation.
The Horsehead Nebula can be found in the constellation Orion. Its name comes from its resemblance to a horse's head. The Horsehead Nebula was first discovered by Williamina Fleming in 1888.
Diffuse Nebula
the horsehead nebula
No, the Horsehead Nebula is a dark nebula in the constellation Orion and does not have any moons. Moons are natural satellites that orbit planets, whereas nebulae are large clouds of gas and dust in outer space.
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Horsehead Nebula doesn't glow like other nebulae because it is older than other nebulae and was probably a lot smaller. In addition, Horsehead Nebula is farther away from the Earth than other nebulae, so it may seem that it doesn't glow as bright as other nebulae. No, this isn't right! The horsehead nebula doesn't glow for one reason - it isn't illuminated by any stars whose energy is enough to make the gas shine. That's the only difference between a 'bright' diffuse nebula (like M42) and a 'dark' one like the Horsehead or the Coalsack. M42 (the Orion nebula) is bright because there are several hot, energetic stars embedded inside it, and which cause it to 'shine'.
Planetary nebulae (the cat's eye nebula) Emission nebulae (the orion nebula) Dark nebulae (the horsehead nebula) Supernova remnant nebulae (the crab)
IC 434,Barnard 33,LDN 1630,M3T 31,[OS98] 52
That is just a funny joke. First off, the Horse-head Nebula is in a outer space, far away and second, is it a nebula. A nebula is a section of a star that exploded and is a formation of star gas. Thanks for asking away.
The Horsehead Nebula is a dark nebula located in the constellation Orion. It is a cloud of dust and gas that is backlit by a nearby bright star, giving it the distinctive shape that resembles the head of a horse. The nebula is a popular target for astrophotography due to its striking appearance.
I think it would be impossible to argue that it does NOT spin. As part of the Milky Way, the Horsehead Nebula is orbiting around the center of the galaxy. Since that is true, it would be perceived as having a spin either sidereally or synodically or both, and it may be spinning around its own axis as well. Even if it isn't, it is spinning from some valid point of view.
A nebula is a cloud of dust and gas in space. Some of the clouds block out the light from the stars behind. These are called dark nebulae. One of the best-known is the Horsehead Nebula. Other dust clouds reflect the light from the stars and shine brightly. These are called bright nebulae. : Edit: The Great Orion Nebula is M42. M43 is a close nebula close to M42.