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{{Short description|Main-belt asteroid}} {{About|the asteroid|the satellite of Jupiter|Io (moon)|other uses|Io (disambiguation)}} {{Use dmy dates|date=October 2019}} {{Infobox planet | minorplanet = yes | background = #D6D6D6 | name = 85 Io | image = 85Io (Lightcurve Inversion).png | image_scale = | caption = [[Lightcurve]]-based 3D-model of ''Io'' | discoverer = [[Christian Heinrich Friedrich Peters|C. H. F. Peters]] | discovered = 19 September 1865 | mpc_name = (85) Io | alt_names = A899 LA{{·}}A899 UA | pronounced = {{IPAc-en|ˈ|aɪ|.|oʊ}}<ref>Noah Webster (1884) ''A Practical Dictionary of the English Language''</ref> | adjective = Ionian {{IPAc-en|aɪ|ˈ|oʊ|n|i|ə|n}} | named_after = [[Io (mythology)|Io]] | mp_category = [[main-belt]]{{·}}{{small|([[Kirkwood gap|middle]])}}<br />[[Eunomia family#Interlopers|Eunomian interloper]] | orbit_ref =  <ref name="jpldata" /> | epoch = 4 September 2017 ([[Julian day|JD]] 2458000.5) | uncertainty = 0 | observation_arc = 151.35 yr (55,280 days) | aphelion = 3.1679 [[Astronomical unit|AU]] | perihelion = 2.1379 AU | semimajor = 2.6529 AU | eccentricity = 0.1941 | period = 4.32 [[Julian year (astronomy)|yr]] (1,578 days) | mean_anomaly = 83.678[[Degree (angle)|°]] | mean_motion = {{Deg2DMS|0.2281|sup=ms}} / day | inclination = 11.961° | asc_node = 203.12° | arg_peri = 123.11° | dimensions = 180 × 160 × 160 km<ref name="Torppa2003" /><ref name="Erikson99" /> | mass = (5.034 ± 0.999/1.406){{e|18}} kg<ref name="FiengaEtAl2020"/> | density = 2.14 ± 0.425/0.598 g/cm<sup>3</sup><ref name="FiengaEtAl2020"/>{{efn|Assuming a diameter of 165 ± 3 km.}} | rotation = 0.2864 d (6.875 h)<ref name=jpldata /> | albedo = 0.0666 ± 0.003<ref name=jpldata /> | spectral_type = [[F-type asteroid|F]][[C-type asteroid|C]] {{small|(Tholen)}}<ref name="jpldata" /><br />[[B-type asteroid|B]] {{small|(SMASSII)}}<ref name="jpldata" /> | abs_magnitude = 7.96<ref name=jpldata /> }} '''85 Io''' is a [[Carbonaceous chondrite|carbonaceous]] [[asteroid]] in the central region of the [[asteroid belt]], approximately 170 kilometers in diameter. It is an identified [[Eunomia family#Interlopers|Eunomian interloper]]. == Discovery and naming == It was discovered by [[Christian Heinrich Friedrich Peters|C. H. F. Peters]] on 19 September 1865, and named after [[Io (mythology)|Io]], a lover of [[Zeus]] in [[Greek mythology]]. [[Io (moon)|Io]] is also the name of the [[volcanic]] [[natural satellite|satellite]] of [[Jupiter]]. With a two-digit number and a two-letter name, 85 Io has the shortest designation of all minor planets. == Orbit and physical characteristics == Io is a [[Prograde and retrograde motion|retrograde]] rotator, with its pole pointing towards one of [[ecliptic coordinate system|ecliptic coordinates]] (β, λ) = (-45°, 105°) or (-15°, 295°) with a 10° uncertainty.<ref name="Torppa2003" /> This gives an [[axial tilt]] of about 125° or 115°, respectively. Its shape is quite regular.{{citation needed|date=August 2022}} In the [[SMASS classification]], ''Io'' is a carbonaceous [[C-type asteroid]], which means that it is probably a primitive body composed of [[carbonate]]s. Like [[141 Lumen]] it is an [[Interloper (asteroid)|interloper]] that orbits within the [[Eunomia family|Eunomia asteroid family]] but it is not related to the shattered parent body.{{citation needed|date=August 2022}} An Ionian diameter of 178 kilometres was measured from an [[occultation]] of a [[star]] on 10 December 1995.<ref name="Erikson99" /> Another [[asteroid occultation]] of Io (magnitude 13.2) occurred on 12 March 2009, from the eastern [[United States]], with the star 2UCAC 35694429 (magnitude 13.8).<ref>http://www.asteroidoccultation.com/2009_03/0312_85_20455.htm {{dead link|date=September 2015}}</ref> {| class="wikitable" style="align: center; font-size: 0.9em;" |- ! Conjunction to sun|| stationary, then retrograde || Opposition || Minimal distance (AE) || Maximum brightness (mag) || stationary, then prograde |- |27. April 2004 || 31.October 2004 || 23. December 2004 || 1,92017 AE || 12,3 mag || 11. February 2005 |- |3.August 2005 || 9. January 2006 || 5. March 2006 || 2,14389 AE || 11,8 mag || 25. April 2006 |- |17.October 2006 || 26. April 2007 || 9.June 2007 || 1,38393 AE || 12,1 mag || 26.July 2007 |- |7. March 2008 || 6.October 2008 || 22.November 2008 || 1,61470 AE || 10,7 mag || 9. January 2009 |- |8. July 2009 || 17. December 2009 || 12. February 2010 || 2,19864 AE || 11,1 mag || 3. April 2010 |- |21. September 2010 || 15. March 2011 || 30. April 2011 || 1,68623 AE || 12,2 mag || 20.June 2011 |- |7. January 2012 || 31.August 2012 || 12.October 2012 || 1,28465 AE || 11,1 mag || 19.November 2012 |- |9.June 2013 || 25.November 2013 || 20. January 2014 || 2,13519 AE || 10,1 mag || 12. March 2014 |- |29.August 2014 || 10. February 2015 || 1. April 2015 || 1,95222 AE || 12,2 mag || 22.May 2015 |- |22.November 2015 || 30.June 2016 || 14.August 2016 || 1,16222 AE || 11,6 mag || 17.September 2016 |- |3.May 2017 || 3.November 2017 || 26. December 2017 || 1,95048 AE || 10,2 mag || 15. February 2018 |- |6.August 2018 || 13. January 2019 || 9. March 2019 || 2,12957 AE || 11,8 mag || 28. April 2019 |- |21.October 2019 || 2.May 2020 || 14.June 2020 || 1,34977 AE || 12,0 mag || 30.July 2020 |} == See also == * [[List of Solar System objects by size]] == Notes == {{notelist}} == References == {{reflist |refs= <ref name="jpldata">{{cite web |title=JPL Small-Body Database Browser: 85 Io |url=https://ssd.jpl.nasa.gov/sbdb.cgi?sstr=85 |publisher=[[Jet Propulsion Laboratory]] |access-date=1 November 2017}}</ref> <ref name="Torppa2003">{{cite journal |last=Torppa |first=J. |display-authors=etal |journal=Icarus |volume=164 |page=346 |url=http://www.rni.helsinki.fi/~mjk/thirty.pdf |title=Shapes and rotational properties of thirty asteroids from photometric data |date=2003 |issue=2 |doi=10.1016/s0019-1035(03)00146-5|bibcode = 2003Icar..164..346T }}</ref> <ref name="Erikson99">{{cite journal |last1=Erikson |first1=A. |last2=Berthier |first2=J. |last3=Denchev |first3=P.V. |bibcode=1999P&SS...47..327E |title=Photometric observations and modelling of the asteroid 85 Io in conjunction with data from an occultation event during the 1995-96 apparition |journal=Planetary and Space Science |volume=47 |pages=327–330 |date=1999 |issue=3–4 |doi=10.1016/S0032-0633(98)00128-7}}</ref> <ref name="FiengaEtAl2020">{{Cite journal |last=Fienga |first=A. |last2=Avdellidou |first2=C. |last3=Hanuš |first3=J. |date=February 2020 |title=Asteroid masses obtained with INPOP planetary ephemerides |url=https://academic.oup.com/mnras/article/492/1/589/5658701 |journal=Monthly Notices of the Royal Astronomical Society |volume=492 |issue=1 |doi=10.1093/mnras/stz3407 |doi-access=free}}</ref> }} <!-- end of reflist --> == External links == *[http://www.rni.helsinki.fi/~mjk/thirty.pdf Shapes and rotational properties of thirty asteroids from photometric data, Torppa (2003) ] * {{AstDys|85}} * {{JPL small body}} {{Minor planets navigator |84 Klio |number=85 |86 Semele}} {{Small Solar System bodies}} {{Authority control}} {{DEFAULTSORT:Io}} [[Category:Eunomia asteroids|000085]] [[Category:Discoveries by Christian Peters]] [[Category:Named minor planets]] [[Category:Objects observed by stellar occultation|000085]] [[Category:FC-type asteroids (Tholen)|000085]] [[Category:B-type asteroids (SMASS)|000085]] [[Category:Astronomical objects discovered in 1865|18650919]]
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