Horse is a horse is a ? (2009 July 21)

[emc]

http://apod.nasa.gov/apod/ap090721.html

A horse is a horse of course, of course, but this looks like a grinning bedraggled dragon to me... but who asked... no one... it's just my 'magination, runnin' away with me. Just my 'magination...

[orin stepanek]

http://apod.nasa.gov/apod/ap090721.html

A horse is a horse of course, of course, but this looks like a grinning bedraggled dragon to me... but who asked... no one... it's just my 'magination, runnin' away with me. Just my 'magination...

OK to Imagine; that's probably how it got to be called a horse. 8) If it whinnies it's a horse; if it belches fire it's a dragon!
It could become a navigation point for some future space travelers; now there's my imagination.

Orin

[Earthbelow]

My own slightly warped imagination leads me to ask if there is a nebula somewhere that is named for the other end of the horse?

[neufer]

My own slightly warped imagination leads me to ask if there is a nebula somewhere that is named for the other end of the horse?

http://antwrp.gsfc.nasa.gov/apod/ap090707.html
http://antwrp.gsfc.nasa.gov/apod/ap090503.html

[apodman]

My own slightly warped imagination leads me to ask if there is a nebula somewhere that is named for the other end of the horse?

[neufer]

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<<The Horsehead Nebula (also known as Barnard 33 in bright nebula IC 434) is a dark nebula in the constellation Orion. The nebula is located just below Alnitak, the star furthest left on Orion's Belt, and is part of the much larger Orion Molecular Cloud Complex. It is approximately 1500 light years from Earth. It is one of the most identifiable nebulae because of the shape of its swirling cloud of dark dust and gases, which is similar to that of a horse's head. The shape was first noticed in 1888 by Williamina Fleming on photographic plate B2312 taken at the Harvard College Observatory. The red glow originates from hydrogen gas predominantly behind the nebula, ionized by the nearby bright star Sigma Orionis. The darkness of the Horsehead is caused mostly by thick dust, although the lower part of the Horsehead's neck casts a shadow to the left. Streams of gas leaving the nebula are funneled by a strong magnetic field. Bright spots in the Horsehead Nebula's base are young stars just in the process of forming.>>

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<<Williamina Paton Stevens Fleming (May 15, 1857 – May 21, 1911), astronomer, was born in Dundee, Scotland, to Robert Stevens and Mary Walker Stevens. She attended public schools in Dundee, and at the age of 14, she became a pupil-teacher. She married James Orr Fleming, and they moved to the U.S. and settled in Boston, Massachusetts, when she was 21.

While she was pregnant with her son, Edward, her husband abandoned her, and she had to find work to support herself and Edward. She worked as a maid in the home of Professor Edward Charles Pickering.

Pickering became frustrated with his male assistants at the Harvard College Observatory and famously declared his maid could do a better job. So in 1881, Pickering hired Fleming to do clerical work at the observatory. While there, she devised and helped implement a system of assigning stars a letter according to how much hydrogen could be observed in their spectra. Stars classified as A had the most hydrogen, B the next most, and so on. Later, Annie Jump Cannon would improve upon this work to develop a simpler classification system based on temperature.

Fleming contributed to the cataloguing of stars that would be published as the Henry Draper Catalogue. In nine years, she catalogued more than 10,000 stars. During her work, she discovered 59 gaseous nebulae, over 310 variable stars, and 10 novae. In 1907, she published a list of 222 variable stars she had discovered.

In 1888, Mrs. Fleming discovered the Horsehead nebula on Harvard plate B2312, describing the bright nebula (later known as IC-434) as having "a semicircular indentation 5 minutes in diameter 30 minutes south of Zeta [Orionis]." William Pickering, who took the photograph, speculated that the spot was dark obscuring matter. All subsequent articles and books seem to deny Fleming and W. H. Pickering credit, because the compiler of the first Index Catalogue, J. L. E. Dreyer, eliminated Mrs. Fleming's name from the list of objects then discovered by Harvard, attributing them all instead merely to "Pickering" (taken by most readers to mean E. C. Pickering, Director of Harvard College Observatory.) But, by the release of the second Index Catalogue by Dreyer in 1908, Mrs. Fleming and others at Harvard were famous enough to receive proper credit.

Fleming was placed in charge of dozens of women hired to do mathematical classifications and edited the observatory's publications. In 1899, Fleming was given the title of Curator of Astronomical Photographs. In 1906, she was made an honorary member of the Royal Astronomical Society of London, the first American woman to be so elected. Soon after, she was appointed honorary fellow in astronomy of Wellesley College. Shortly before her death, the Astronomical Society of Mexico awarded her the Guadalupe Almendaro medal for her discovery of new stars. She published A Photographic Study of Variable Stars (1907) and Spectra and Photographic Magnitudes of Stars in Standard Regions (1911).

Williamina Fleming died in Boston of pneumonia.>>

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