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{{DISPLAYTITLE:{{mp|2005 HC|4}}}} | name={{mp|2005 HC|4}} ...

| discovered = 18 July 1999 | aphelion = 39.013 [[Astronomical unit|AU]] ...

| discovered = 17 September 2010 | aphelion = 1.0785 [[Astronomical unit|AU]] ...

{{Short description|Variable star in the constellation Orion}} ...lue band]] [[light curve]] for FU Orionis, adapted from Clarke ''et al.'' (2005).<ref name="Clarke2005"/> The inset plot, adapted from Siwak, ''et al.'' (2 ...

| discovered = 27 April 2015 ...f name="PlanetarySociety"/> Observations leading to its discovery occurred in April 2015, using the [[Hubble Space Telescope]]'s [[Wide Field Camera 3]], ...

...nd its satellite imaged by the [[Hubble Space Telescope]] from May to July 2005 | discovered = 5 April 2000 ...

{{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 ...

{{Short description|Brown dwarf in the constellation Taurus}} ...emissions via particle interactions in its [[magnetic field]], as observed in other known rapidly-rotating brown dwarfs.<ref name="Tannock2021"/> ...

{{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 ...

{{short description|Galaxy in the constellation Cassiopeia}} ...after [[Paolo Maffei]], who discovered it and the neighboring [[Maffei 2]] in 1967 via their [[infrared]] emissions. ...

{{Short description|Star in the constellation Ara}} ...r Westerlund 1: The Initial Mass Function and Mass Segregation|journal=The Astronomical Journal|volume=145|issue=2|pages=46|last1=Lim|first1=Beomdu|last2=Chun|firs ...

| discovered = 24 February 2009 | aphelion = 1.7361&nbsp;[[Astronomical unit|AU]] ...

{{short description|Star in the constellation Cygnus}} ...07-2013)|journal=VizieR On-line Data Catalog: B/GCVS. Originally Published in: 2009yCat....102025S|volume=1|display-authors=etal|last1=Samus|first1=N. N. ...

{{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 ...

| discovered = 13 October 2015<br />{{small|(first observed only)}} ...ement in March 2018, it was the third most distant observed natural object in the [[Solar System]], after [[Eris (dwarf planet)|Eris]] and {{mpl|2014 UZ| ...

| discovered = 13 November 2005 | alt_names = S/2005 (90482) 1<ref name="jpldata"/> ...

{{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 ...

...groups have been called Peter Pan disks in one scientific paper published in early 2020.<ref>{{Cite web|url=https://www.nhn.ou.edu/~smsilver/PeterPanDis ...y share with the [[Lost Boys (Peter Pan)|lost boys]] and titular character in Peter Pan.<ref name="Silverberg2020" /><ref name="Disk Detective blog" /> ...

{{Short description|Carbon star in the constellation Leo Minor}} ...n Sky Survey]].<ref name="Ulrich"/> It is the second brightest carbon star in the near-infrared, after CW Leonis (which is much closer to us).<ref name=" ...

{{Short description|Star in the constellation Aquila}} ...olved stars: Application to HD 179821|journal=Monthly Notices of the Royal Astronomical Society|volume=388|issue=2|pages=716|last1=Nordhaus|first1=J.|last2=Minchev ...