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- ...r 1,048 times the mass of Jupiter. Masses of other [[star]]s and groups of stars are listed in terms of solar masses. Its mathematical symbol and value are: ...461 bytes (71 words) - 00:14, 25 January 2017
- ...cs/ask_astro/answers/980603a.html |title=Ask an astrophysicist: Wolf-Rayet Stars |last=Cannizzo J.K. 1998 |work=Nasa.gov }}</ref> ...0,000 K.<ref name=wc>Sander A; Hamann W.R. & Todt H. 2012. The galactic WC stars. ''Astronomy & Astrophysics'' '''540''': A144. [http://www.aanda.org/index. ...2 KB (381 words) - 20:05, 10 October 2014
- ...30px|[[Hubble telescope]] image known as ''[[Pillars of Creation]]'' where stars are forming in the [[Eagle nebula]]]] ...985ApJ...289..373S}}</ref> The nearest nebula to the [[Sun]] where massive stars are being formed is the [[Orion nebula]], {{convert|1300|ly|km|abbr=on}} aw ...6 KB (950 words) - 11:37, 2 November 2016
- As the Earth orbits around the Sun, the position of nearby stars will appear to shift slightly against the more distant background. These sh | journal=Binary stars as critical tools and tests in contemporary astrophysics: International Ast ...10 KB (1,469 words) - 22:59, 15 September 2015
- ...ty of the central star clusters, suggesting there are 10 to 100 supergiant stars in each of these, packed into regions just a few [[parsecs]] across.]] ...1 KB (225 words) - 11:44, 21 June 2017
- ...ings. He also thought that [[perpetual motion]] was impossible, except for stars. ...2 KB (231 words) - 11:28, 9 March 2013
- ...on moves around the earth. It is also used to calculate how other planets, stars and objects in space move around. ...3 KB (548 words) - 15:02, 5 April 2017
- * The masses of stars are very large and are sometimes expressed in units of [[Solar mass]]es. ...3 KB (496 words) - 11:10, 5 July 2017
- ...ive sooner than the light from the receding star. This would cause binary stars to appear to move in ways that violate Kepler's Laws, but this is not seen. ...15 KB (2,495 words) - 16:23, 9 April 2017
- ...8tefabzS28C&pg=PA136 An Introduction to the Evolution of Single and Binary Stars]. Springer, 2012, p. 136</ref> which is inversely proportional to the [[squ ...mple would be twice as great'''. By such reasoning, Lane concluded that as stars get smaller they grow hotter to withstand gravitation and resist collapse." ...23 KB (3,626 words) - 09:52, 1 September 2017
- 13 KB (1,977 words) - 14:34, 21 July 2017
- 36 KB (5,991 words) - 08:00, 24 August 2017