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| − | {{Infobox Planet | discovery=yes | physical_characteristics = yes | bgcolour=#FFFFC0 | <!-- Scroll down to see the text of the article, below this table.--> | + | {{Infobox Planet | bgcolour=#FFFFC0 | <!-- Scroll down to see the text of the article, below this table.--> |
| | name=90482 Orcus | | name=90482 Orcus |
| − | | image=[[File:Orcus nasa.jpg|250px|NASA picture of 90482 Orcus]] | + | | image=Orcus nasa.jpg |
| | | discoverer=[[Michael E. Brown|M. Brown]],<br />[[Chad Trujillo|C. Trujillo]],<br />[[David L. Rabinowitz|D. Rabinowitz]] | | | discoverer=[[Michael E. Brown|M. Brown]],<br />[[Chad Trujillo|C. Trujillo]],<br />[[David L. Rabinowitz|D. Rabinowitz]] |
| | | discovered=[[February 17]], [[2004]] | | | discovered=[[February 17]], [[2004]] |
| | | alt_names=2004 DW | | | alt_names=2004 DW |
| | | mp_category=[[Plutino]]<ref name="Buie">{{cite web | | | mp_category=[[Plutino]]<ref name="Buie">{{cite web |
| − | |author=[[Marc W. Buie|Buie, Marc W.]] | + | |author = [[Marc W. Buie|Buie, Marc W.]] |
| − | |date=2007-12-22 | + | |date = 2007-12-22 |
| − | |title=Orbit Fit and Astrometric record for 90482 | + | |title = Orbit Fit and Astrometric record for 90482 |
| − | |publisher=SwRI (Space Science Department) | + | |publisher = SwRI (Space Science Department) |
| − | |url=http://www.boulder.swri.edu/~buie/kbo/astrom/90482.html | + | |url = http://www.boulder.swri.edu/~buie/kbo/astrom/90482.html |
| − | |accessdate=2008-09-19| archiveurl = http://www.webcitation.org/65IF26P0R |archivedate = 2012-02-08| deadurl=no}}</ref> | + | |accessdate = 2008-09-19 |
| | + | |archiveurl = https://www.webcitation.org/65IF26P0R?url=http://www.boulder.swri.edu/~buie/kbo/astrom/90482.html |
| | + | |archivedate = 2012-02-08 |
| | + | |url-status = dead |
| | + | }}</ref> |
| | | epoch=[[November 30]], [[2008]] ([[Julian day|JD]] 2 454 800) | | | epoch=[[November 30]], [[2008]] ([[Julian day|JD]] 2 454 800) |
| | | semimajor=5 862.44 [[Giga|Gm]] (39.188 [[Astronomical unit|AU]]) | | | semimajor=5 862.44 [[Giga|Gm]] (39.188 [[Astronomical unit|AU]]) |
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| | | avg_speed=4.68 km/[[second|s]] | | | avg_speed=4.68 km/[[second|s]] |
| | | satellites=1 (92-432 km) | | | satellites=1 (92-432 km) |
| − | | dimensions=946.3 {{±|74.1|72.3}} km (diameter)<ref name="Stansberry 2007">{{cite journal|last=Stansberry|first=J.| coauthors=Grundy, W.; Brown, M.; ''et al.''|title=Physical Properties of Kuiper Belt and Centaur Objects: Constraints from Spitzer Space Telescope|url=http://arxiv.org/abs/astro-ph/0702538v1|year=2007}}</ref> | + | | dimensions=946.3 {{±|74.1|72.3}} km (diameter)<ref name="Stansberry 2007">{{cite journal|last=Stansberry|first=J.| author2=Grundy, W.| author3= Brown, M.; | display-authors = etal|title=Physical Properties of Kuiper Belt and Centaur Objects: Constraints from Spitzer Space Telescope|url=https://arxiv.org/abs/astro-ph/0702538v1|year=2007}}</ref> |
| | | mass=~7.5×10<sup>20</sup> [[kilogram|kg]] | | | mass=~7.5×10<sup>20</sup> [[kilogram|kg]] |
| | | density=~1.5 g/[[cubic centimetre|cm³]] (assumed) | | | density=~1.5 g/[[cubic centimetre|cm³]] (assumed) |
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| | | escape_velocity=~0.44 km/s | | | escape_velocity=~0.44 km/s |
| | | rotation=13.19h<ref name="BBC h2g2">{{cite web |url=http://www.bbc.co.uk/dna/h2g2/A32537720 |title=Overlooked dwarf planet candidates |accessdate=2008-07-25 |publisher=BBC |date=2008-02-19 }}</ref> | | | rotation=13.19h<ref name="BBC h2g2">{{cite web |url=http://www.bbc.co.uk/dna/h2g2/A32537720 |title=Overlooked dwarf planet candidates |accessdate=2008-07-25 |publisher=BBC |date=2008-02-19 }}</ref> |
| − | | spectral_type=B-V=0.68; V-R=0.37 <ref>{{cite web|url=http://www.physics.nau.edu/~tegler/research/survey.htm |title=Kuiper Belt Object Magnitudes and Surface Colors |accessdate=2006-11-05 |last=Tegler |first=Stephen C. |coauthors= |date=2006-01-26| archiveurl = http://www.webcitation.org/5TO84zdpq | archivedate = 2007-11-16| deadurl=no}}</ref> | + | | spectral_type=B-V=0.68; V-R=0.37 <ref>{{cite web |url=http://www.physics.nau.edu/~tegler/research/survey.htm |title=Kuiper Belt Object Magnitudes and Surface Colors |accessdate=2006-11-05 |last=Tegler |first=Stephen C. |date=2006-01-26 |archiveurl=https://www.webcitation.org/5TO84zdpq?url=http://www.physics.nau.edu/~tegler/research/survey.htm |archivedate=2007-11-16 |url-status=dead }}</ref> |
| | | magnitude = 19.1 ([[Opposition (astronomy and astrology)|opposition]])<ref name="Horizons">{{cite web | | | magnitude = 19.1 ([[Opposition (astronomy and astrology)|opposition]])<ref name="Horizons">{{cite web |
| | |title=HORIZONS Web-Interface | | |title=HORIZONS Web-Interface |
| − | |publisher=[http://ssd.jpl.nasa.gov JPL Solar System Dynamics] | + | |publisher=JPL Solar System Dynamics |
| | |url=http://ssd.jpl.nasa.gov/horizons.cgi?find_body=1&body_group=sb&sstr=Orcus | | |url=http://ssd.jpl.nasa.gov/horizons.cgi?find_body=1&body_group=sb&sstr=Orcus |
| − | |accessdate=2008-07-02| archiveurl = http://www.webcitation.org/65IEzVrtJ |archivedate = 2012-02-08| deadurl=no}}</ref> | + | |accessdate=2008-07-02 |
| | + | |archiveurl=https://www.webcitation.org/65IEzVrtJ?url=http://ssd.jpl.nasa.gov/horizons.cgi?find_body=1 |
| | + | |archivedate=2012-02-08 |
| | + | |url-status=live |
| | + | }}</ref> |
| | | abs_magnitude=2.3<ref name="jpldata">{{cite web | | | abs_magnitude=2.3<ref name="jpldata">{{cite web |
| − | |date=2008-02-10 last obs | + | |date=2008-02-10 |
| | |title=JPL Small-Body Database Browser: 90482 Orcus (2004 DW) | | |title=JPL Small-Body Database Browser: 90482 Orcus (2004 DW) |
| | |url=http://ssd.jpl.nasa.gov/sbdb.cgi?sstr=Orcus | | |url=http://ssd.jpl.nasa.gov/sbdb.cgi?sstr=Orcus |
| − | |accessdate=2008-07-02| archiveurl = http://www.webcitation.org/65IEzxEJN |archivedate = 2012-02-08| deadurl=no}}</ref> | + | |accessdate=2008-07-02 |
| | + | |archiveurl=https://www.webcitation.org/65IEzxEJN?url=http://ssd.jpl.nasa.gov/sbdb.cgi?sstr=Orcus |
| | + | |archivedate=2012-02-08 |
| | + | |url-status=live |
| | + | }}</ref> |
| | | albedo=19.75 {{±|3.40|2.76}} % | | | albedo=19.75 {{±|3.40|2.76}} % |
| | | single_temperature=~45 [[kelvin|K]]}} | | | single_temperature=~45 [[kelvin|K]]}} |
| | | | |
| − | '''90482 Orcus''', originally known by the [[provisional designation]] '''2004 DW''') is a [[Kuiper belt]] object (KBO) and could be a [[dwarf planet]]. It was found by [[Michael E. Brown|Michael Brown]], [[Chad Trujillo]] and [[David L. Rabinowitz|David Rabinowitz]] on [[February 17]], [[2004]]. It was also seen in pictures from [[November 8]], [[1951]]. | + | '''90482 Orcus''', originally known by the [[provisional designation]] '''2004 DW''', is a [[Kuiper belt]] object (KBO). It is also a [[dwarf planet]]. It was found by [[Michael E. Brown|Michael Brown]], [[Chad Trujillo]] and [[David L. Rabinowitz|David Rabinowitz]] on February 17, 2004. It was also seen in pictures from November 8, 1951. Like [[Pluto]] it is in [[orbital resonance]] with [[Neptune]] but it stays on the opposite side of the Sun from Pluto. |
| | | | |
| | == Moon == | | == Moon == |
| | | | |
| − | A moon of Orcus was found on [[22 February]] [[2007]].<ref>[http://www.johnstonsarchive.net/astro/astmoons/am-90482.html (90482) Orcus and Vanth] {{WebCite|url=http://www.webcitation.org/65IF3ZmvN|date =2012-02-08}}</ref> The orbit of this moon has yet to be found out. | + | A moon of Orcus was found on [[22 February]] [[2007]].<ref>{{Cite web |url=http://www.johnstonsarchive.net/astro/astmoons/am-90482.html |title=(90482) Orcus and Vanth |access-date=2009-02-27 |archive-date=2012-02-08 |archive-url=https://www.webcitation.org/65IF3ZmvN?url=http://www.johnstonsarchive.net/astro/astmoons/am-90482.html |url-status=bot: unknown }}</ref> |
| | | | |
| − | The satellite was found at 0.25 [[arcsecond|arcsec]] from Orcus with [[absolute magnitude|magnitude]] difference of 2.7.<ref name="EKO51"> [http://www.boulder.swri.edu/ekonews/issues/past/n051/html/index.html Distant EKO] The Kuiper Belt Electronic newsletter, March 2007</ref> | + | The satellite was found at 0.25 [[arcsecond|arcsec]] from Orcus with [[absolute magnitude|magnitude]] difference of 2.7.<ref name="EKO51">[http://www.boulder.swri.edu/ekonews/issues/past/n051/html/index.html Distant EKO] The Kuiper Belt Electronic newsletter, March 2007</ref> Assuming an [[albedo]] similar to that of the primary, the magnitude suggests a diameter of about 220 km. It is thought to be a smaller KBO that was captured. |
| − | Assuming an [[albedo]] similar to that of the primary, the magnitude suggests a diameter of about 220 km. It is thought to be a smaller KBO that was captured. | |
| | | | |
| | == Other websites == | | == Other websites == |
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| | * [http://www.chadtrujillo.com/2004dw/ Chad Trujillo's page on 2004 DW] | | * [http://www.chadtrujillo.com/2004dw/ Chad Trujillo's page on 2004 DW] |
| | * [http://news.bbc.co.uk/2/hi/science/nature/3506329.stm First BBC article] | | * [http://news.bbc.co.uk/2/hi/science/nature/3506329.stm First BBC article] |
| − | * [http://www.newscientist.com/news/news.jsp?id=ns99994702 First New Scientist article] | + | * [https://www.newscientist.com/news/news.jsp?id=ns99994702 First New Scientist article] |
| | * [http://www.lowell.edu/users/buie/kbo/astrom/90482.html Updated orbital elements from Lowell Observatory] | | * [http://www.lowell.edu/users/buie/kbo/astrom/90482.html Updated orbital elements from Lowell Observatory] |
| | * [http://hamilton.dm.unipi.it/cgi-bin/astdys/astibo?objects:Orcus;main AstDys] orbital elements | | * [http://hamilton.dm.unipi.it/cgi-bin/astdys/astibo?objects:Orcus;main AstDys] orbital elements |