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- | discovered = 18 July 1999 | aphelion = 39.013 [[Astronomical unit|AU]] ...9 KB (1,058 words) - 04:14, 8 February 2025
- | name = (410777) 2009 FD | image = 2009 FD.png ...19 KB (2,431 words) - 21:09, 13 February 2025
- {{Short description|Small temporary satellite of Earth that impacted in 2015}} | discovered = {{Ubl ...17 KB (2,409 words) - 11:50, 26 January 2025
- {{Short description|Triplet of galaxies in the constellation Virgo}} ...r Galaxies]], compiled by [[Halton Arp]] in 1966. Galaxies 269 through 274 in his catalogue are galaxies that appear to have connected [[Spiral arm|arms] ...5 KB (765 words) - 18:38, 5 December 2024
- ...asurement indicates the log<sub>10</sub> of the relative abundance of iron in the measured star to that of the Sun.</ref> ...72''', is a [[star]] located in the constellation [[Lyra]]. Observed since 2009 by the [[Kepler (spacecraft)|Kepler space observatory]], it has since been ...10 KB (1,317 words) - 06:26, 10 September 2024
- {{Short description|Red supergiant star in the Large Magellanic Cloud}} |caption=The supergiant IRAS 05280–6910 in the open cluster [[NGC 1984]]. It is the bright reddened object near the ce ...6 KB (783 words) - 01:49, 10 December 2024
- {{Short description|Disappearing red supergiant star in the galaxy NGC 6946 }} ...lion solar luminosities, but by 2015 it had disappeared from optical view. In the mid and [[near infrared]] an object is still visible; however, it is fa ...7 KB (1,051 words) - 03:45, 24 January 2025
- {{short description|Meteoroid that impacted near Ontario, Canada in November 2022}} | discovered = 19 November 2022 ...14 KB (1,804 words) - 09:37, 31 January 2025
- {{Short description|Variable star in the constellation Fornax}} ...designation|R]] For, [[Cordoba Durchmusterung|CD]]−26°892, [[Infrared Astronomical Satellite|IRAS]] 02270-2619, [[2MASS]] J02291531-2605559 ...8 KB (1,037 words) - 12:15, 3 August 2024
- {{short description|Star in the constellation Cygnus}} ...ay-authors=etal|last1=Samus|first1=N. N.|last2=Durlevich|first2=O. V.|year=2009}}</ref> ...10 KB (1,434 words) - 10:15, 17 February 2025
- {{Short description|Millisecond pulsar in the constellation Serpens}} | radial_v = <!--Radial velocity (in km/sec)--> ...10 KB (1,463 words) - 14:07, 9 December 2024
- {{Short description|Variable star in the constellation Scutum}} ...pulsating variable]] known as an [[RV Tauri variable]]. It was discovered in 1795 by [[Edward Pigott]] at a time when only a few [[variable star]]s were ...12 KB (1,731 words) - 00:12, 22 June 2024
- {{Short description|Binary star in the constellation Cetus}} '''Mu Ceti''' (μ Ceti) is a [[binary star]] in the [[constellation]] [[Cetus]], the whale, close to [[Pisces (constellatio ...12 KB (1,580 words) - 03:53, 2 February 2025
- {{Short description|1944 nova in the constellation Telescopium}} | appmag_v = ≈12 (in 2013)<ref name=AAVSO/> ...14 KB (2,066 words) - 02:38, 19 May 2024
- | discovered = 13 November 2005 ...ems formed similarly, most likely by a [[Impact event|giant impact]] early in the Solar System's history.<ref name="Brown2023"/> Compared to Orcus, Vanth ...34 KB (4,469 words) - 21:27, 5 February 2025
- {{Short description|Star in the constellation Pictor}} | caption = Location of HD 40307 in the night sky. The star is marked within the red diamond below the word "Pi ...19 KB (2,346 words) - 03:10, 14 October 2024
- {{Short description|Binary star in the constellation Dorado}} '''WOH G64''' ('''IRAS 04553-6825''') is a [[symbiotic binary]] in the [[Large Magellanic Cloud]] (LMC), roughly 160,000 [[light-year]]s from ...21 KB (3,012 words) - 20:01, 23 February 2025
- {{short description|Luminous blue variable star in the constellation Sagittarius}} ...= 1403.5298|title = Nature Versus Nurture: Luminous Blue Variable Nebulae in and Near Massive Stellar Clusters at the Galactic Center|journal=The Astrop ...13 KB (1,939 words) - 23:07, 14 August 2024
- | discovered = 21 March 2018 (suspected since 2002) ...lescope]] in 2023<ref name="JWSTProposal2243"/> and the image was released in 24 july, 2024.<ref name="JWSTImages2024-07-24" /> ...16 KB (2,242 words) - 00:34, 13 February 2025
- ...ravitational force from the supermassive black hole keeps the stars moving in very tight orbits about the center of the cluster. ...is happens when two SMBHs in a binary system coalesce, after losing energy in the form of [[gravitational wave]]s. Because the gravitational waves are no ...12 KB (1,788 words) - 15:32, 6 February 2025