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</html>";s:4:"text";s:3771:"<br>40 Eridani B est la première naine blanche à avoir été découverte. THE DISTANCE AND MASS OF 40 ERIDANI B 40 Eri B is the second brightest white dwarf and among the first to be discovered. A new mystery surrounding 40 Eridani B arose in 1998 when J. L. Provencal and collaborators estimated the radius of the star using parallax measurements. <br> <br>40 Eridani B: The secondary star was classified as a AVII star with an absolute magnitude of 11.2. 40 Eiridani is a triple star system so 40 Eridani A, B and C are already taken as designators of these stars.  <br>Most researchers use parallaxes … The star in question is 40 Eridani B, which is part of triple stellar system in the Sun’s neighbourhood, only 5.0 parsec away from us. It was classified as an A-type star by Williamina Fleming, one of the women computers working at the Harvard College Observatory. 40 Eridani A is located in visible on a clear night in the southern Eridanus constellation. So assuming the mass for 40 Eridani B was correct, it would have to be a helium-core white dwarf resulting from a binary-star merger. <br> <br>40 Eridani C: The tertiary star was classified as a M4V star with an absolute magnitude of 12.3. - SIMBAD4 rel 1.7 - 2020.04.10CEST07:25:11 Available data : Basic data • Identifiers • Plot & images • Bibliography • Measurements • External archives • Notes • Annotations It has a mass estimated from about 50.1 percent of Sol's ( Provencal et al, 1998 ), only two percent of its diameter, and 33/10,000th of its brightness. Credit: IAU/Sky and Telescope Magazine. The distance between Eridani A and B is 400 astronomical units. The most massive is 40 Eridani A, a dwarf star that is the mythical Vulcan’s sun. 40 Eridani B is not part of the constellation outline but is within the borders of the constellation. Its parallax has been determined many times in the 20th century, mostly with long-focus refractors. 40 Eridani (also known as Omicron 2 Eridani, or Keid, from the Arabic word qayd, (egg) shells) is a triple star system less than 16.5 light years away from Earth.It is in the constellation Eridanus.The primary star of the system, 40 Eridani A, is easily visible to the naked eye. §2. <br> <br>It was originally discovered by Díaz et al. Vulcan orbits the primary star, and the two companion stars “would gleam brilliantly in the Vulcan sky,” they wrote in their 1991 letter. <br> <br>It has the designation name of 40 Eridani which is the star that Gene Roddenberry said was host star for the Vulcan homeworld. 40 Eridani. The pair 40 Eridani B/C was discovered on January 31, 1783, by William Herschel. <br> <br>ref: N.A.S.A. The other two are a pair, orbiting each other at a distance from 40 Eridani A. The distance between Eridani A and B is 400 astronomical units. The description is based on the spectral class. For other stars with this Bayer designation, see ο Eridani. (2018) and confirmed by the Dharma Planet Search (Ma et al., 2018). About a hundred years ago, one particular star made many astronomers scratch their heads. Best Binoculars for Astronomy 2019 - BBR Best Astronomy Binocular Awards - Duration: 7:15. What we do. 40 Eridani ; A star chart of the Eridanus constellation showing the position of 40 Eridani … The planet around 40 Eridani B is reckoned to have a mass about 8.5 times that of Earth so might well have a surface gravity over 2 times greater. 40 Eridani B Facts. In this situation, the stars release energy when spiralling into each other, and this energy carries away material from the outer layers, allowing the formation of a lower mass white dwarf with a helium core. <br> Every page goes through several hundred of perfecting techniques; in live mode. Quite the same Wikipedia. <br>";s:7:"keyword";s:12:"40 Eridani B";s:5:"links";s:2660:"<a href='https://boxwoodballs.com/docs/page.php?790614=oh-nana-dance'>Oh Nana Dance</a>,
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