List of Solar System objects most distant from the Sun in 2015

Positions of known outer Solar System objects.
The centaurs lie generally inwards of the Kuiper belt and outside the Jupiter trojans.
  Sun
  Jupiter trojans (6,178)
  Scattered disc (>300)
  Giant planets: J · S · U · N
  Centaurs (44,000)
  Kuiper belt (>1,000)
(scale in AU; epoch as of January 2015; # of objects in parenthesis)
The orbit of Sedna, shown in red, with the dot marking its current location. Inside are the orbits of the giant planets of the Solar System, and that of Pluto in purple. Sedna will travel out nearly 1000 AU, taking almost six millennia to do so. It is currently less than 100 AU from the Sun.
One of the Sun's "wild things", a distant TNO wrapping itself around the planets on slanted orbit. Shown highlighted here is the orbit of 2004 XR190
Eris and its moon as viewed with Hubble, 2007
Makemake viewed with Hubble, 2006
Sedna viewed with Hubble, 2004
This observation of Halley's Comet in 2003 at 28 AU from the Sun illustrates some of the difficulty in observing objects as they grow more distant.
Graph showing the numbers of KBOs for a given distance from the Sun. The plutinos are the "spike" at 39 AU, whereas the classicals are between 42 and 47 AU, the twotinos are at 48 AU, and the 5:2 resonance is at 55 AU. Note this lists semi-major axis not current distance from the Sun (see Kuiper cliff)

This list of Solar System objects most distant from the Sun in 2015 is a list of bodies orbiting the Sun by their approximate distance from the Sun in the Earth year 2015 (as opposed to those with the greatest calculated aphelion in their orbit).

V774104 was announced in November 2015. It was heralded by many news outlets as "the most distant Solar System object", surpassing Eris (not counting space probes and long-period comets).[1]

Another very distant body is Sedna, discovered in November 2003. Although it takes over 10,000 years to orbit, it will slowly get closer over the next 60 years to its perihelion.[2]

Because all these objects are moving, the list changes significantly over time. In particular, some objects are in-bound and some are out-bound. It is hard to see comets at the longer distances. It is usually their big comas that allow them to be detected more easily when they get heated by the Sun.

List

Distances are in astronomical units (AU, Sun–Earth distances); listed are current (as of 2015) locations, not future min or maxes. There are also known comets at great distances, but they are currently too faint to be observed. This is a list based on objects discovered up to this year:

Body Distance (AU)
V774104 ~103[3][4]
136199 Eris 96[5]
2014 UZ224*~92
(225088) 2007 OR10 87[5]
90377 Sedna 86[5]
2014 FC69 84.1[5]
2006 QH181 83.5[5]
2012 VP113 (aka "Biden") 83.3[5]
2013 FY27 80.1[5]
2010 GB174 70.6[5]
(148209) 2000 CR105 60.4[5]
2003 QX113 59.9[5]
2008 ST291 59.7[5]
2013 JQ64 58.4[5]
2004 XR190 (aka "Buffy") 57.5[6]
2006 HX122 55.5[6]
2009 KL30 54.7[6]
2013 GQ136 54.7[6]
2004 VU130 53.8[6]
2007 VK305 53.8[6]
2002 FV6 53.8[6]
2010 RF43 53.2[6]
2010 RE64 53[6]
2012 UT177 52.9[6]
1999 KR18 52.65[6]
(136472) Makemake 52.427[6]
2009 KK30 52.382[6]
(42301) 2001 UR163 52.285[6]
2013 JM65 52.209[6]
2013 JV64 51.996[6]
2007 LF38 51.931[6]
2013 JH64 51.626[6]
(303775) 2005 QU182 51.323[6]
2002 CY248 51.092[6]
2000 CO105 51.083[6]
2001 UP18 50.86[6]
2001 OM109 50.849[6]
(386723) 2009 YE7 50.693[6]
(136108) Haumea 50.676[6]
(437915) 2002 GD32 50.551[6]
2011 UQ411 50.521[6]
2000 AF255 50.157[6]
1999 RU214 50.089[6]
(54520) 2000 PJ30 49.758[7]
2011 UT411 49.68[7]
2003 UB292 49.676[7]
2004 DH64 49.494[7]
2000 WM183 49.313[7]
(182397) 2001 QW297 49.305[7]
1999 OG4 49.203[7]
(385362) 2002 PT170 49.173[7]
2000 SK331 49.159[7]
2011 UV412 48.961[7]
2013 GT136 48.89[7]
2013 FZ27 48.793[7]
2001 KG76 48.467[7]
2000 CK105 48.461[7]
2000 CJ105 48.412[7]
2013 GG138 48.38[7]
2011 UM411 48.359[7]
2011 UE412 48.312[7]
(202421) 2005 UQ513 48.286[7]
1999 RX214 48.09[7]
2003 FL127 48.087[7]
2012 WD36 48.084[7]
2003 HX56 48.069[7]
(90482) Orcus 48.046[7]
2005 EN302 47.967[7]
2010 VK201 47.92[7]
2014 FT71 47.872[7]
(385363) 2002 PW170 47.85[7]
2002 CZ224 47.811[7]
2006 JU58 47.803[7]
1999 CP153 47.784[7]
2001 KA77 47.755[7]
2004 MU8 47.744[7]
2002 CY154 47.73[7]
2001 KL76 47.694[7]
2005 EW318 47.657[7]
2004 VN112 47.612[7]
1998 WW31 47.578[7]
2003 QA112 47.571[7]
2013 FC28 47.404[7]
2002 PA171 47.394[7]
2013 SE99 47.387[7]
2011 HE103 47.335[7]
2002 XH91 47.318[7]
2000 PL30 47.274[7]
1999 OK4 47.254[7]
(19308) 1996 TO66 47.229[7]
2004 HD79 47.193[7]
2011 JX31 47.179[7]
2002 VE130 47.131[7]
2002 CX224 47.11[7]
2004 KK19 47.066[7]
2000 CG105 47.047[7]
174567 Varda 47.033[7]
2004 PX117 47.007[7]
2003 GF55 46.996[7]
2000 CN105 46.982[7]
2001 UN18 46.96[7]
2004 VB131 46.953[7]
2005 JA175 46.913[7]
2004 OJ14 46.907[7]
1999 CD158 46.858[7]
(307261) 2002 MS4 46.844[7]
2011 UT412 46.831[7]
2001 ES24 46.754[7]
2000 CQ114 46.736[7]
2000 PY29 46.719[7]
2003 UZ291 46.687[7]
2007 XV50 46.68[7]
1999 CL119 46.656[7]
2014 UF224 46.654[7]
2009 KO30 46.644[7]
1999 OA4 46.562[7]
2000 FC8 46.554[7]
2013 GV137 46.516[7]
2002 PO149 46.486[7]
2005 JR179 46.424[7]
1999 CH119 46.419[7]
2005 PT21 46.29[7]
2013 JJ64 46.285[7]
1998 KY61 46.219[7]
2010 FX86 46.214[7]
(145480) 2005 TB190 46.201[7]
2004 PW117 46.188[7]
2000 YF2 46.154[7]
2010 KZ39 46.148[7]
2002 FX36 46.056[7]
2011 US412 46.032[7]
2009 DR143 46.005[7]
2007 RM314 45.978[7]
2013 RD98 45.962[7]
2000 PG30 45.951[7]
2000 WL183 45.942[7]
2000 PM30 45.933[7]
1999 RZ214 45.929[7]
2005 EB318 45.924[7]
2000 PD30 45.918[7]
(66452) 1999 OF4 45.902[7]
2003 QB91 45.897[7]
2001 OQ108 45.864[7]
1999 DA 45.844[7]
2012 UH177 45.842[7]
2003 TK58 45.834[7]
148780 Altjira 45.814[7]
2013 GK137 45.771[7]
2004 LW31 45.753[7]
(55565) 2002 AW197 45.753[7]
2013 GE138 45.714[7]
(363330) 2002 PQ145 45.671[7]
(385201) 1999 RN215 45.65[7]
2005 EE296 45.645[7]
(79978) 1999 CC158 45.632[7]
2013 JG64 45.595[7]
2011 UF412 45.584[7]
2000 CP104 45.536[7]
2001 HA59 45.442[7]
1995 WY2 45.437[7]
2000 QE226 45.435[7]
2011 UZ411 45.366[7]
(78799) 2002 XW93 45.351[7]
1996 RR20 45.35[7]
2000 CQ105 45.336[7]
2003 UT291 45.331[7]
1999 OM4 45.29[7]
(69988) 1998 WA31 45.29[7]
(82075) 2000 YW134 45.277[7]
2003 KO20 45.264[7]
2005 JY185 45.264[7]
2000 WV12 45.249[7]
1999 GS46 45.232[7]
(15883) 1997 CR29 45.203[7]
2000 FB8 45.156[7]
2000 YA2 45.15[7]
88611 Teharonhiawako 45.142[7]
2005 CD81 45.131[7]
2000 PA30 45.123[7]
2011 UB412 45.095[7]
(84522) 2002 TC302 45.071[7]
2007 CQ79 45.043[7]
1998 WX24 45.038
2000 WT169 45.024[7]
(48639) 1995 TL8 45.02[7]
2013 FA28 45.015[7]

See also

Objects with very large aphelion

References

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