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- ...scription|Angle between the orbital plane of a satellite and the vector to the sun}} ...d-orbit-analysis-program-spacecraft-thermal-design-972540 |journal=Journal of Aerospace |series=SAE Technical Paper Series |volume=1 |language=English |p ...8 KB (1,274 words) - 23:51, 23 October 2024
- ...y the Dynamical Method | last = Kochetova | first = O.M. | journal = Solar System Research | volume = 38 | issue = 1 | year = 2004 | pages = 66–75|bibcode = ...e can be as large as ~0.1 AU, for less massive asteroids the conditions of the interaction would need to be correspondingly better.<ref name=Kochetova-200 ...4 KB (599 words) - 11:35, 19 November 2022
- ...ted out instead of deleted, in case they can be improved and put back into the article.--> ...ersity Press, 2012.</ref> [[Newtonian fluid]]s, and the [[fluid dynamics]] of [[galaxies]]. ...11 KB (1,746 words) - 18:28, 6 August 2024
- ...of 6000 K to the minimum of 4400 K, the [[optical depth]] is about 1, and the radiation is thermal. ...xrt soft x-ray.gif|thumb|right|320px|The Sun in the soft X-rays as seen by the [[Hinode (satellite)|Hinode]] X-ray Telescope (XRT) on 15 Oct 2009.]] ...13 KB (1,929 words) - 08:14, 13 August 2023
- {{Short description|Boundary between solar corona and wind}} ...[[Solar System]] so fast that waves within the wind cannot make it back to the Sun.<ref name=animation/>]] ...15 KB (2,118 words) - 17:14, 27 December 2024
- ...stem on a [[hyperbolic trajectory]] due to a close approach to Jupiter. In the 43 years since its discovery only two objects with higher eccentricities ha |title=Pole, Pericenter, and Nodes of the Interstellar Minor Body A/2017 U1 ...11 KB (1,477 words) - 02:33, 9 November 2024
- ...ur Sun ([[Exoplanet|exoplanets]]). This is a nascent field of study due to the challenges in directly observing their [[Atmosphere|atmospheres]]. ...offers insights into the diverse climates that may exist beyond our solar system. ...8 KB (1,248 words) - 18:09, 16 February 2025
- {{Short description|A measure for the size of planets and other Solar System objects}} ......528A..41L }}</ref> In the case of a sphere, the mean radius is equal to the radius. ...7 KB (1,010 words) - 17:44, 5 November 2024
- ...arious studies and experiments that examine the two-dimensional geometries of these enclosures. ...rnal obstructions exist, in which the flow can circulate freely throughout the entire cavity. ...7 KB (1,075 words) - 19:46, 7 October 2024
- ...ion]] from the planet. It provides an approximation for the temperature of the [[tropopause]] on [[terrestrial planet]]s with [[greenhouse gas]]es present ...ce-Air Temperature with Satellite and Surface Observations|journal=Journal of Climate|volume=10|issue=7|pages=1505–1524|issn=0894-8755|jstor=26243273|doi ...9 KB (1,332 words) - 09:54, 27 September 2023
- {{Short description|Outer moon of Uranus}} ...-diameter"/> Given H {{=}} 13.7 and assuming an albedo range of 0.04–0.10, the diameter range is {{val|8|-|12|u=km}}.}}<br>8 km<ref name="SheppardMoons"/> ...12 KB (1,611 words) - 05:37, 19 February 2025
- ...lsion systems such as [[electrically powered spacecraft propulsion]] and [[solar sail]]. ...nsfer is occasionally posed as an [[optimal control]] problem subjected to the required objective and constraints. ...7 KB (1,066 words) - 17:22, 4 October 2024
- ...an Italian [[mathematician]] and [[astronomer]], based at the [[University of Pisa]]. ...of Mathematical Physics at the Department of Mathematics of the University of Pisa.<ref>{{Cite web|url=http://copernico.dm.unipi.it/~milani/|title = Andr ...5 KB (637 words) - 11:58, 3 February 2024
- ...try (monitoring system)|Sentry Risk Table]] with a [[Torino Scale]] rating of 1 on 2 April 2003.<ref name="Wayback2003-04"/> ...math></ref> refined the orbit.<ref name="spaceguard"/> It was removed from the Sentry Risk Table on 28 May 2003.<ref name="removed"/> ...7 KB (949 words) - 20:10, 27 November 2023
- {{short description|Star in the constellation Cygnus}} ...ar (circled). The bright star at the centre is [[γ Cygni]] and north is to the right. ...10 KB (1,434 words) - 10:15, 17 February 2025
- | caption = Orbit and current position of {{mpl|2015 TH|367}} ...2018, it was the third most distant observed natural object in the [[Solar System]], after [[Eris (dwarf planet)|Eris]] and {{mpl|2014 UZ|224}}.{{efn|name=UZ ...17 KB (2,296 words) - 22:06, 23 January 2025
- [[File:IRS46 nasa.jpg|right|300px|thumb|Illustration of a dusty disk in orbit around a young star]] ...inner Solar System resulting in smaller terrestrial planets, a small mass of [[Mars]] and a low mass asteroid belt. ...22 KB (3,279 words) - 14:22, 15 October 2024
- {{Short description|Outer moon of Neptune}} ...-diameter"/> Given H {{=}} 12.1 and assuming an albedo range of 0.04–0.10, the diameter range is {{val|16|-|25|u=km}}.}}<br>14 km<ref name="SheppardMoons" ...19 KB (2,472 words) - 13:40, 23 January 2025
- {{Short description|System of differential equations}} ...dientEverlastingArabianoryx-size_restricted.gif|thumb|527x527px|University of Texas N-body Simulation. Governed by Jeans equations in a gravitational pot ...12 KB (1,782 words) - 12:49, 4 February 2025
- {{Short description|Outer moon of Neptune}} | caption = S/2002 N 5 imaged by the [[Very Large Telescope]] in September 2002 ...15 KB (1,915 words) - 16:14, 23 January 2025