Information AboutBetelgeuse |
| CATEGORIES ABOUT BETELGEUSE | |
| bayer objects | |
| orionis, alpha | |
| orion constellation | |
| red supergiants | |
| semiregular variables | |
| arabic words and phrases | |
Betelgeuse ( in the Constellation Orion , and the tenth Brightest Star in the night sky. Although it has the Bayer Designation "alpha", it is not as bright as Rigel (Beta Orionis). It is a Vertex of the Winter Triangle asterism. Betelgeuse is a and Pease using an Astronomical Interferometer on the Mount Wilson 100 inch Telescope . ORIGIN OF THE NAME "BETELGEUSE" The name is a corruption of the Arabic يد الجوزا ''yad al-jawzā'', or "hand of the central one". ''Jauza'', the central one, initially referred to Gemini among the Arabs, but at some point they decided to refer to Orion by that name. During the Middle Ages the first character of the name, ''y'' (ﻴ, with two dots under it), was misread as a ''b'' ('''ﺒ''', with one dot under it) when transliterating into Latin , and ''Yad al-Jauza'' became ''Bedalgeuze''. Then, during the Renaissance , it was theorized that the name was originally written as ''Bait al-Jauza'', thought to mean "armpit of the central one" in Arabic, which led to the modern rendering as "Betelgeuse"; however, the actual translation of "armpit" would be ابط ("Ibţ"). Because of its rich reddish color the star has frequently been referred to as the "martial one", and in Astrology portends military or civic honors. Other names are:
DISTINGUISHING CHARACTERISTICS Several features of Betelgeuse are of particular interest to astronomers. It was one of the first stars to have its angular diameter measured with an Astronomical Interferometer ; the apparent diameter was found to be variable. The distance to Betelgeuse is not precisely known, but if it is assumed to be 427 Light Years , then the actual diameter at visible wavelengths must vary between 800,000,000 Km (500 million miles) and 1,000,000,000 Km (600 million miles). At maximum diameter, the star would extend out beyond the Orbit of Mars if placed at the location of the Sun . The precise diameter is not easy to define, as the optical emission decreases very gradually with radius from the center of the star, and the color of the emission also varies with radius. Though only 15 times more massive than the Sun, it is as much as 40 million times greater in volume; a difference in volume much like a Beach Ball compared to Texas Stadium . It was also the first star to have starspots on its disk resolved in optical images by a telescope, first from Aperture Masking Interferometry and later from more detailed observations by the COAST telescope . Astronomers predict that Betelgeuse will ultimately undergo a type II Supernova explosion although it is possible that the mass is low enough for Betelgeuse to leave a rare oxygen-neon White Dwarf . Opinions are divided as to the likely timescale for this event. Some regard the star's current variability as suggesting that it is already in the Carbon burning phase of its life cycle, and will therefore undergo a supernova explosion at some time in the next thousand years or so. Skeptics dispute this contention and regard the star as being likely to survive much longer. There is a consensus that such a supernova would be a spectacular astronomical event, but would not — being so distant — represent any significant threat to life on Earth. Even so, Betelgeuse would brighten at least 10,000 times as a supernova, causing it to shine with the luminosity of a crescent Moon. Some sources predict a maximum apparent magnitude equal to about that of the full Moon (mv = -12.5). This would likely last for several months. It would look like a brilliant point, the brightness of a full Moon with the color of an incandescent bulb at night, and easily visible in daylight. After that period it would gradually diminish until after some months or years it would disappear from naked eye view. Then Orion's left shoulder would vanish for a time until, in a few centuries, a splendid Nebula would develop. However, if Betelgeuse's axis (one of its poles) is pointed towards Earth there would be tangible effects here. A shower of gamma rays and other cosmic particles would be directed at Earth. There would be spectacular Aurorae and possibly a measurable diminution of the Ozone Layer with consequent adverse radiation effects on life. In such an orientation towards the Solar System it would also appear many times brighter than if its axis were pointed away. Curiously, 1st century BC Chinese records unearthed by Shu-ren, Jianmin and Jin-Yi in 1980 refer to the color of Betelgeuse as being white or yellow. However, Ptolemy writing in 150 AD calls it a red star. Therefore, Fang Li-Zhi, a Chinese astrophysicist, proposed that Betelgeuse could have turned into a red giant star during that period. It is known that as stars use up the hydrogen fuel in their cores, their color changes from white to yellow to red. Shu-ren et al. suggest that Betelgeuse could have changed its color when it expelled a shell of dust and gas, that, even now, can be seen to be expanding away from it. Thus, if their theory is right, it is unlikely that Betelgeuse will become a supernova any time soon because a star usually stays a red giant for tens of thousands of years. EXTERNAL LINKS |
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