Search results

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

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

| discovered = 8 March 2003 |earliest_precovery_date = 17 May 2002 ...

| name = S/2002 N 5 | image = S-2002 N 5 VLT-FORS1 2002-09-03 annotated.gif ...

{{Short description|Brown dwarf in the constellation Chamaleon}} ...MNRAS|language=en|volume=332|issue=3|pages=L65–L68|doi=10.1046/j.1365-8711.2002.05539.x|arxiv=astro-ph/0206365 |issn=0035-8711|bibcode=2002MNRAS.332L..65B| ...

{{Short description|Variable star in the constellation Orion}} ...msu.su/groups/cluster/gcvs/gcvs/iii/iii.dat |date=2017-06-20 }}, Sternberg Astronomical Institute, Moscow, Russia. Accessed on line December 8, 2008.</ref> ...

{{Short description|Variable star in the constellation Fornax}} ...designation|R]]&nbsp;For, [[Cordoba Durchmusterung|CD]]−26°892, [[Infrared Astronomical Satellite|IRAS]]&nbsp;02270-2619, [[2MASS]]&nbsp;J02291531-2605559 ...

...|title=A large arc in the gravitational lens system 0957 + 561|journal=The Astronomical Journal|volume=105|year=1993|pages=816|issn=0004-6256|doi=10.1086/116474|bi ...thumb|A light source passes behind a gravitational lens (point mass placed in the center of the image). The aqua circle is a source as it would be seen i ...

{{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 ...

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

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

| discovered = 7 September 2021 | p_mean_motion = 13.1009833 <!-- Temporary fix: [360°/(period in days)]*(365.25 days) --> ...

| 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" /> ...

...] {{small|(1998)}}<br/>[[E. Bright Wilson Award in Spectroscopy]] {{small|(2002)}}<br/>[[Davy Medal]] {{small|(2004)}} ...is a Japanese-American [[spectroscopist]] and [[astronomer]] specializing in the field of [[galactic astronomy]], known as a pioneer of [[astrochemistry ...

{{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|Ringed dwarf planet in the Kuiper belt}} | discovered = 4 June 2002 ...

{{Short description|Dwarf planet in the scattered-disc}} | discovered = 17 July 2007 ...

...microorganisms into space to be used as [[introduced species]] on other [[astronomical object]]s. ...lFuture" >{{Cite journal|last = Mautner |first = Michael N. | title = Life in the cosmological future: Resources, biomass and populations | journal = Jo ...

...l measurement, but it provides a way to measure the masses of astronomical objects without requiring assumptions about their composition or dynamical state. ...laxies. The distortion shown here is greatly exaggerated relative to real astronomical systems.]] ...

...body]] of the [[Solar System]] – thus completing a full cycle of [[season|astronomical season]]s. For example, it is the time from [[March equinox|vernal equinox] ...around the Sun as measured with respect to the [[fixed stars]], resulting in a duration of 20 [[minute (time)|minute]]s longer than the tropical year, b ...