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- The formation and [[wikt:evolution|evolution]] of the [[Solar System]] is estimated to have begun 4.6 [[1000000000 ...is believed to have been responsible for much of the Solar System's early evolution. ...85 KB (12,829 words) - 17:09, 18 August 2009
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- ...ds of Trojans may indicate that they have undergone a stronger collisional evolution compared to the main belt.<ref name=Barucci2002/> ==Origin and evolution== ...27 KB (3,965 words) - 06:02, 30 July 2009
- ===Evolution=== ...in the core, producing [[oxygen]], [[neon]] and [[magnesium]].<ref name="evolution">{{cite web ...42 KB (6,228 words) - 21:05, 5 February 2010
- ...p]]s) formed as a result of the expansion of its interior during its early evolution. This moon probably formed from the [[accretion disk]] that surrounded Uran ==Origin and evolution== ...25 KB (3,710 words) - 20:43, 4 August 2009
- ...After the hydrogen fuel at the core has been consumed, the star [[stellar evolution|evolves]] away from the main sequence on the HR diagram. The behavior of a | title=Principles of Stellar Evolution and Nucleosynthesis | publisher=University of Chicago Press ...49 KB (7,190 words) - 18:56, 4 June 2009
- ..., have argued about the appropriateness of the monkeys as a metaphor for [[evolution]]. ===Evolution=== ...37 KB (5,653 words) - 08:08, 11 August 2009
- ...thesis''' is the most widely accepted model explaining the [[formation and evolution of the Solar System]]. It was first proposed in 1734 by [[Emanuel Swedenbor {{main article|History of Solar System formation and evolution hypotheses}} ...50 KB (7,534 words) - 17:00, 23 June 2009
- The formation and [[wikt:evolution|evolution]] of the [[Solar System]] is estimated to have begun 4.6 [[1000000000 ...is believed to have been responsible for much of the Solar System's early evolution. ...85 KB (12,829 words) - 17:09, 18 August 2009
- ...te journal|last=Showman|first=Adam P.|coauthors=Malhotra, Renu|title=Tidal Evolution into the Laplace Resonance and the Resurfacing of Ganymede|journal=Icarus|y ....593P|pmid=12386333}}</ref> or that it developed after the [[Formation and evolution of the Solar System|formation of the Solar System]]. A possible sequence of ...62 KB (9,204 words) - 08:32, 18 August 2009
- ...d]], which has had important consequences for its internal structure and [[evolution]].<ref name=Freeman2006/> Its distance from Jupiter also means that the [[c ==Origin and evolution== ...50 KB (7,326 words) - 08:23, 11 August 2009
- ...spiff.rit.edu/classes/phys230/lectures/planneb/planneb.html Late stages of evolution for low-mass stars], Michael Richmond, lecture notes, Physics 230, [[Roches ...years.<ref>[http://adsabs.harvard.edu/abs/1997ApJS..108..339B The Chemical Evolution of Cool White Dwarfs and the Age of the Local Galactic Disk], P. Bergeron, ...77 KB (11,681 words) - 15:01, 22 October 2010
- ...avitationally.<ref>{{cite journal |author=M Woolfson |title=The origin and evolution of the solar system |doi= 10.1046/j.1468-4004.2000.00012.x |year=2000 |jour ...]]; it was born in the later stages of the [[Universe#Evolution|universe's evolution]], and thus contains more elements heavier than hydrogen and helium ("[[met ...82 KB (12,276 words) - 02:46, 16 June 2010
- ...tal mass of a star is the principal determinant in its [[stellar evolution|evolution]] and eventual fate. Other characteristics of a star are determined by its | title = Late stages of evolution for low-mass stars ...96 KB (14,170 words) - 15:20, 20 August 2009
- ...n initial condition; rather, it ''describes'' and ''explains'' the general evolution of the universe since that instant. The observed abundances of the light el |title=The Evolution of the Universe: Discussion ...71 KB (10,449 words) - 08:42, 20 August 2009
- ...an artificial construction or modification. This implies that the rate of evolution of a species which can create galaxy spanning superstructures is less than ...is only rarely a good choice and hence by no means a sure endpoint of the evolution of a [[Tree of life (science)|tree of life]]. ...74 KB (11,034 words) - 10:20, 30 July 2011
- ...r]] speculated on a similar disc having formed early in the Solar System's evolution, however, he did not believe that such a belt still existed today. Kuiper w ...igration|migrated]] outwards during the course of the Solar System's early evolution. Eventually, the orbits shifted to the point where Jupiter and Saturn exist ...58 KB (9,031 words) - 16:11, 18 August 2009
- ==Evolution under perturbed potentials== ...61 KB (8,970 words) - 23:12, 23 July 2009
- | title=The Stars: Their Structure and Evolution | title=Stellar evolution from the zero-age main sequence ...61 KB (9,014 words) - 04:56, 13 June 2010
- ...and can be used to obtain information about the large-scale properties and evolution of our cosmos.<ref>Introductions to gravitational lensing and its applicati ...f black holes are thought to be the final state in the [[stellar evolution|evolution]] of massive [[star]]s. On the other hand, [[supermassive black hole]]s wit ...67 KB (9,914 words) - 21:17, 11 August 2009
- | title=The Stars: Their Structure and Evolution | title=The Stars: Their Structure and Evolution ...58 KB (8,480 words) - 20:27, 18 August 2009
- | title=The Earth's early evolution | year=1995 | title=Our Changing Sun: The Role of Solar Nuclear Evolution and Magnetic Activity on Earth's Atmosphere and Climate ...115 KB (16,384 words) - 03:09, 14 June 2010