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Dynamical class of minor planets
Detached objects are a dynamical class of minor planets in the outer reaches of the Solar System and belong to the broader family of trans-Neptunian objects
Detached_object
Distant body in the outer Solar System
similar objects such as 2000 CR105, be placed in a new category of distant objects named extended scattered disc objects (E-SDO), detached objects, distant
Sedna_(dwarf_planet)
Solar system objects beyond Neptune
divided into the classical and resonant objects of the Kuiper belt, the scattered disc and detached objects with the sednoids being the most distant
Trans-Neptunian_object
Collection of bodies in the extreme Solar System
periodic comets. Many objects of the proposed Oort cloud are also thought to have originated in the scattered disc. Detached objects are not sharply distinct
Scattered_disc
Solar system objects beyond the other known trans-Neptunian objects
Neptune and still interact with the giant planets. The detached ETNOs (or extreme detached disc objects, EDDOs), with perihelia approximately between 40–45
Extreme trans-Neptunian object
Extreme_trans-Neptunian_object
Natural physical entity in space
An astronomical object, celestial object, stellar object or heavenly object is a naturally occurring physical entity, association, or structure that exists
Astronomical_object
Highly eccentric detached trans-Neptunian object
2015 RX245 is a detached trans-Neptunian object on a highly eccentric orbit in the outermost region of the Solar System. It measures approximately 250
2015_RX245
Large, round non-stellar astronomical object
unstable towards interactions with Neptune. Sedna is the largest known detached object, a population that never comes close enough to the Sun to interact
Planet
Planetary system consisting of the Sun and objects orbiting it
disc objects, they were likely formed as result of gravitational scattering by Neptune and still interact with the giant planets. The detached ETNOs
Solar_System
Distant planetesimals in the Solar System
Kuiper belt, the scattered disc and the detached objects—three nearer reservoirs of trans-Neptunian objects. Both regions lie well beyond the heliosphere
Oort_cloud
TC302 (612584) 2003 QX113 (87269) 2000 OO67 2015 TH367 2014 UZ224 Detached objects (612911) 2004 XR190 2017 OF201 2012 VP113 (possibly inner Oort cloud)
List_of_Solar_System_objects
Extreme trans-Neptunian object from the outer Oort cloud
trans-Neptunian objects. Its average orbital distance is noted as one of the largest among known trans-Neptunian objects. Unlike detached sednoids, it is
2014_FE72
Innermost Galilean moon of Jupiter
any known astronomical object in the Solar System. With over 400 active volcanoes, Io is the most geologically active object in the Solar System. This
Io_(moon)
Transneptunian Region IV. Size/albedo characterization of 15 scattered disk and detached objects observed with Herschel Space Observatory-PACS". Astronomy & Astrophysics
List of Solar System objects by size
List_of_Solar_System_objects_by_size
Group of trans-Neptunian objects
perihelia greater than 60 AU. The sednoids are also classified as detached objects, since their perihelion distances are large enough that Neptune's gravity
Sednoid
Detached object in the scattered disc
2013 FQ28 is a trans-Neptunian object, considered both a scattered and detached object, located in the outermost region of the Solar System. It was first
2013_FQ28
Detached trans-Neptunian object
2014 ST373 is a trans-Neptunian object and a detached object from the outermost region of the Solar System. With a perihelion of 50.2 AU, it belongs to
2014_ST373
gravitationally rounded objects of the Solar System. This also includes a list of the eight planets according to the IAU definition. For a list of objects in the Solar
Lists_of_planets
Planets visible to the naked eye
A classical planet is an astronomical object that is visible to the naked eye and moves across the sky and its backdrop of fixed stars (the common stars
Classical_planet
Overview of and topical guide to the Solar System
Gonggong Moon of Gonggong Farthest regions Extreme trans-Neptunian objects Detached objects Sedna Leleākūhonua Oort cloud Heliosphere Heliopause Boundaries
Outline_of_the_Solar_System
Area of the Solar System beyond the planets, comprising small bodies
objects are composed largely of frozen volatiles (termed "ices"), such as methane, ammonia, and water. The Kuiper belt is home to most of the objects
Kuiper_belt
Large trans-Neptunian object in the scattered disc
2017 OF201 is an extreme trans-Neptunian object and dwarf planet candidate, estimated to be around 500 to 900 kilometres (300 to 600 miles) in diameter
2017_OF201
Dwarf planet in the scattered-disc
region. IV. Size/albedo characterization of 15 scattered disk and detached objects observed with Herschel-PACS". Astronomy & Astrophysics. 541 (A92):
Gonggong_(dwarf_planet)
Detached extreme trans-Neptunian object
474640 Alicanto (provisional designation 2004 VN112) is a detached extreme trans-Neptunian object. It was discovered on 6 November 2004, by American astronomer
474640_Alicanto
Trans-Neptunian object
(148209) 2000 CR105 is a trans-Neptunian object. Considered a detached object, it orbits the Sun in a highly eccentric orbit every 3,305 years at an average
(148209)_2000_CR105
Kuiper belt object, not controlled by an orbital resonance with Neptune
A classical Kuiper belt object, also called a cubewano (/ˌkjuːbiːˈwʌnoʊ/ "QB1-o"), is a low-eccentricity Kuiper belt object (KBO) that orbits beyond Neptune
Classical_Kuiper_belt_object
Extreme trans-Neptunian object
a small number of detached objects with perihelion distances of 30 AU or more, and semi-major axes of 250 AU or more. Such objects can not reach such
2015_KG163
Trans-Neptunian object
trans-Neptunian object, considered both a scattered and detached object, located in the outermost region of the Solar System. The object with a moderately
2015_KQ174
Largest moon of Saturn
to have a dense atmosphere (denser than Earth's), and is the only known object in the Solar System besides Earth with clear evidence of stable bodies of
Titan_(moon)
Region between the orbits of Mars and Jupiter
near-Earth objects, the centaurs, trojans, and the trans-Neptunian objects (Kuiper belt objects, scattered disc objects, sednoids, and Oort cloud objects.) Ceres
Asteroid_belt
600 km trans-Neptunian object
2021 LL37 is a large trans-Neptunian object in the scattered disc, around 600 kilometres (370 miles) in diameter. It was discovered on 12 June 2021, by
2021_LL37
Sednoid
similar to other TNOs and sednoids. Detached object – a class of high-perihelion TNOs that are gravitationally detached from Neptune's gravitational influence
2023_KQ14
Scattered disc object
region: IV. Size/albedo characterization of 15 scattered disk and detached objects observed with Herschel -PACS". Astronomy & Astrophysics. 541: A92.
42355_Typhon
Minor planet in the scattered disc
the discovery team, is a trans-Neptunian object, classified as both a scattered disc object and a detached object, located in the outermost region of the
(612911)_2004_XR190
planets, comprising small bodies Sednoid – Group of trans-Neptunian objects Detached object – Dynamical class of minor planets JPL Small-Body Database Search
List of Solar System objects by greatest aphelion
List_of_Solar_System_objects_by_greatest_aphelion
Trans-Neptunian object
(provisional designation 2007 UK126) is a large binary trans-Neptunian object and dwarf planet candidate in the scattered disc, located in the outermost
229762_Gǃkúnǁʼhòmdímà
Trans-Neptunian object
estimate the diameter as closer to 339 kilometres (211 mi). It is not a detached object, since its perihelion (closest approach to the Sun) is under the influence
(15874)_1996_TL66
Most massive dwarf planet
second-largest-known dwarf planet in the Solar System. It is a trans-Neptunian object (TNO) in the scattered disk and has a high-eccentricity orbit. Eris was
Eris_(dwarf_planet)
Hypothetical Solar System planet
perihelia of objects with semi-major axes greater than 300 AU to oscillate, delivering some into planet-crossing orbits and others into detached orbits like
Planet_Nine
Larger of the two moons of Mars
of Deimos and son of Ares (Mars). Phobos is a small, irregularly shaped object with a mean radius of 11 km (7 mi). It orbits 6,000 km (3,700 mi) from the
Phobos_(moon)
Galaxy in the constellation Serpens Caput
other galaxies share the primary characteristics of Hoag's Object, including a bright detached ring of stars, but their centers are elongated or barred
Hoag's_Object
unauthorized modifications to the original data objects. However, there is a risk that the detached signature could become separated from its associated
Detached_signature
Trans-Neptunian object
2014 FZ71 is a trans-Neptunian object, classified as a scattered and detached object, located in the outermost region of the Solar System. It was first
2014_FZ71
Trans-Neptunian object
2014 SR349 is a trans-Neptunian object and scattered disc object in the outermost part of the Solar System. It was first observed on 19 September 2014
2014_SR349
Kuiper belt Plutinos Cubewanos Arrokoth Other Sednoids Detached objects Damocloids Oort cloud objects Hills cloud Comets Lists of comets Periodic comets Non-periodic
List of largest craters in the Solar System
List_of_largest_craters_in_the_Solar_System
Trans-Neptunian object
2013 FT28 is a trans-Neptunian object. It was discovered on 16 March 2013 at Cerro Tololo Observatory, La Serena and announced on 30 August 2016. 2013
2013_FT28
Extreme trans-Neptunian object
Chile. The detached extended scattered disc object (ESDO) is on a highly eccentric orbit and belongs to the extreme trans-Neptunian objects. 2013 UH15
2013_UH15
Scattered disc object
2014 UZ224 is a large trans-Neptunian object and possible dwarf planet orbiting in the scattered disc of the outermost regions of the Solar System, estimated
2014_UZ224
Trans-Neptunian object
(690420) 2014 FC72 is a trans-Neptunian object, classified as a scattered and detached object, located in the outermost region of the Solar System. It
(690420)_2014_FC72
Long-period comet
comets ever discovered. It was initially thought to be an asteroid-like object with a very eccentric orbit at the time of its discovery on 21 May 2011
C/2011_KP36_(Spacewatch)
Detached object
2010 GB174 is a detached object, discovered on 12 April 2010 on data taken at the Canada–France–Hawaii Telescope as part of the Next Generation Virgo
2010_GB174
Extreme trans-Neptunian object
(768325) 2015 BP519, internally nicknamed Caju, is an extreme trans-Neptunian object from the scattered disc on a highly eccentric and inclined orbit in the
(768325)_2015_BP519
Trans-Neptunian object
2018 AG37 is a distant trans-Neptunian object and centaur that was discovered 132.2 ± 1.5 AU (19.78 ± 0.22 billion km) from the Sun, farther than any other
2018_AG37
Resonant trans-Neptunian object
(84522) 2002 TC302 is an unnamed trans-Neptunian object in the scattered disk, orbiting the Sun on a highly distant and elliptical orbit. It is in a 2:5
(84522)_2002_TC302
Kuiper belt Plutinos Cubewanos Arrokoth Other Sednoids Detached objects Damocloids Oort cloud objects Hills cloud Comets Lists of comets Periodic comets Non-periodic
List of largest rifts, canyons and valleys in the Solar System
List_of_largest_rifts,_canyons_and_valleys_in_the_Solar_System
Topics referred to by the same term
Detachments (British band), an English art rock/electronic group Detached objects, objects which have orbits whose perihelia are sufficiently distant from
Detachment
Trans-Neptunian object
2015 FJ345 is a trans-Neptunian object and detached object, located in the scattered disc, the outermost region of the Solar System. It was first observed
2015_FJ345
Trans-Neptunian object in the scattered disc
(290 miles) in diameter. The detached, extended scattered disc object belongs to the group of extreme trans-Neptunian objects. 2013 FS28 was discovered on
2013_FS28
mountain-like peak was detected via an occultation on the trans-Neptunian object 307261 Máni, qualifying it as one of the tallest known mountains in the
List of tallest mountains in the Solar System
List_of_tallest_mountains_in_the_Solar_System
Trans-Neptunian object
a small number of detached objects with perihelion distances of 30 AU or more, and semi-major axes of 250 AU or more. Such objects cannot reach such orbits
2015_GT50
Entries listed in bold are Solar System-wide extremes. List of Solar System objects most distant from the Sun Astronomy portal Solar System Lists of geological
List_of_Solar_System_extremes
Trans-Neptunian object
region. IV. Size/albedo characterization of 15 scattered disk and detached objects observed with Herschel-PACS". Astronomy and Astrophysics. 541: 18.
(82158)_2001_FP185
Trans-Neptunian object
an object of the scattered disc rather than one of the regular Kuiper belt. However its perihelion of 37.5 AU is too low to make it a detached object, which
(589683)_2010_RF43
Trans-Neptunian object
program at the Palomar Observatory, California. It is classified as a detached object by the Deep Ecliptic Survey (DES), since its orbit appears to be beyond
(120132)_2003_FY128
Trans-Neptunian object
2013 SY99 is a trans-Neptunian object discovered on 29 September 2013 by the Outer Solar System Origins Survey using the Canada–France–Hawaii Telescope
2013_SY99
Type of Solar System object
that were a mixture of horse and human. Observational bias toward large objects makes determination of the total centaur population difficult. Estimates
Centaur (small Solar System body)
Centaur_(small_Solar_System_body)
these kind are: Basic gravity. Following the trajectory of free falling objects, the Earth is "below" us and the sky is "above" us. Characterization of
Timeline of Solar System astronomy
Timeline_of_Solar_System_astronomy
Trans-Neptunian object
a small number of detached objects with perihelion distances of 30 AU or more, and semi-major axes of 150 AU or more. Such objects can not reach such
(508338)_2015_SO20
Trans-Neptunian object
relatively low perihelion of 41.5 AU, contrary to the extended-scattered/detached objects and sednoids, the latter of which stay well beyond the Kuiper cliff
(674118)_2015_KH162
Trans-Neptunian object
(709487) 2013 BL76 is a trans-Neptunian object and centaur from the scattered disk and Inner Oort cloud approximately 30 kilometers in diameter. Using
(709487)_2013_BL76
BCE, Anaxagoras was the first philosopher to consider the Sun as a huge object (larger than the land of Peloponnesus), and consequently, to realize how
Historical models of the Solar System
Historical_models_of_the_Solar_System
Trans-Neptunian object
2013 RF98 is a trans-Neptunian object. It was discovered on September 12, 2013, at Cerro Tololo-DECam. It is part of the evidence for the Planet Nine hypothesis
2013_RF98
Trans-Neptunian object and centaur
(668643) 2012 DR30 is a trans-Neptunian object and centaur with an extremely eccentric orbit that brings it from the inner Oort cloud, the outermost region
(668643)_2012_DR30
Centaur
65° with respect to the ecliptic. As of July 2017, it is one of 7 known objects with inclination (i) > 60° and perihelion (q) > 15 AU, along with the first
2007_BP102
appears to be "detached" from the rest of the Solar System. Detached objects are thus distinct from other populations of trans-Neptunian objects, such as cubewanos
Glossary_of_astronomy
Trans-Neptunian object
trans-Neptunian region IV. Size/albedo characterization of 15 scattered disk and detached objects observed with Herschel-PACS". Astronomy & Astrophysics. 541: A92. arXiv:1202
(303775)_2005_QU182
Scattered disc object
471143 Dziewanna (provisional designation 2010 EK139) is a trans-Neptunian object in the scattered disc, orbiting the Sun in the outermost region of the Solar
471143_Dziewanna
Extreme trans-Neptunian object
(765047) 2013 RA109 is an extreme trans-Neptunian object discovered on 12 September 2013. This object orbits the Sun between 46.0 and 869 AU (6.9 and 130 billion km)
(765047)_2013_RA109
Astronomical object that is neither a planet nor a comet
scattered disc objects. Detached objects such as Sedna, with both an aphelion and a perihelion outside the Kuiper belt. Sednoids, detached objects with a perihelion
Minor_planet
Scattered disc object
145451 Rumina (provisional designation 2005 RM43) is a large trans-Neptunian object in the scattered disc region beyond the Kuiper belt. It was discovered on
145451_Rumina
Star in the constellation Cetus
Circumstellar disc Circumstellar envelope Cosmic dust Debris disk Detached object Disrupted planet Excretion disk Exozodiacal dust Extraterrestrial materials
LHS_1140
Binary trans-Neptunian object
Region IV - Size/albedo characterization of 15 scattered disk and detached objects observed with Herschel Space Observatory-PACS Grundy, W.M.; Stansberry
65489_Ceto
Trans-Neptunian object
(470308) 2007 JH43 is a trans-Neptunian object in the outer regions of the Solar System, approximately 500 kilometers in diameter. It was discovered on
(470308)_2007_JH43
Small Solar System body
1996 PW is an exceptionally eccentric trans-Neptunian object and damocloid on an orbit typical of long-period comets but one that showed no sign of cometary
1996_PW
Object in outer Solar System
group of detached objects with perihelion distances of 30 AU or more, and semi-major axes of 150 AU or more. These extreme trans-Neptunian objects (ETNOs)
(527603)_2007_VJ305
Trans-Neptunian object
(87269) 2000 OO67 is a trans-Neptunian object, approximately 64 kilometers (40 miles) in diameter, on a highly eccentric orbit in the outermost region
(87269)_2000_OO67
Trans-Neptunian object and highly eccentric centaur
(308933) 2006 SQ372 is a trans-Neptunian object and highly eccentric centaur on a cometary-like orbit in the outer region of the Solar System, approximately
(308933)_2006_SQ372
Trans-Neptunian object
TG422 is an extended scattered disc object, as its large aphelion distance is similar to that of the detached objects such as the sednoids (e.g. 90377 Sedna)
(523622)_2007_TG422
Trans-Neptunian object in a mean-motion orbital resonance with Neptune
trans-Neptunian object is a trans-Neptunian object (TNO) in mean-motion orbital resonance with Neptune. The orbital periods of the resonant objects are in a
Resonant trans-Neptunian object
Resonant_trans-Neptunian_object
Trans-Neptunian binary
estimated diameter of 161 kilometres (100 mi). 1995 TL8 is classified as detached object (scattered–extended) by the Deep Ecliptic Survey, since its orbit appears
(48639)_1995_TL8
Classical Kuiper belt object
(120348) 2004 TY364 is a trans-Neptunian object. It is an inner classical Kuiper belt object in the definition by Gladman, Marsden, and Van Laerhoven
(120348)_2004_TY364
Trans-Neptunian object
characterization of 15 scattered disk and detached objects observed with Herschel Space Observatory-PACS List of Transneptunian Objects, Minor Planet Center Asteroid
(40314)_1999_KR16
Large trans-Neptunian object
(574372) 2010 JO179 is a large, high-order resonant trans-Neptunian object in the outermost regions of the Solar System, probably somewhere between 600
(574372)_2010_JO179
Hypothetical planets further than Neptune
inclinations of the trans-Neptunian objects, truncated the planetesimal disk at 48 AU, and detached the orbits of objects like Sedna from Neptune. During
Planets_beyond_Neptune
Extreme trans-Neptunian object
(506479) 2003 HB57 is an extreme trans-Neptunian object of the extended scattered disc in the outermost region of the Solar System, approximately 180 kilometers
(506479)_2003_HB57
Trans-Neptunian object
(523692) 2014 EZ51 is a large trans-Neptunian object in the scattered disc, approximately 600 kilometres (400 miles) in diameter. It was discovered on
(523692)_2014_EZ51
Trans-Neptunian object
2015 TH367 is a trans-Neptunian object on the order of 200 kilometers (120 miles) in diameter. As of 2021[update] it is approximately 90 AU (13 billion km)
2015_TH367
Trans-Neptunian object
(184212) 2004 PB112 is a trans-Neptunian object from the scattered disc, approximately 154 kilometers (96 miles) in diameter, and in a rare high-order
(184212)_2004_PB112
Trans-Neptunian object
Lunar and Planetary Laboratory, at the University of Arizona, as a detached object with a perihelion greater than 40 AUs, a 6:1 orbital period ratio with
(496315)_2013_GP136
Propagating disturbance
supersonic object propagating shows how the transition induced by a shock wave is analogous to a dynamic phase transition. When an object (or disturbance)
Shock_wave
DETACHED OBJECT
DETACHED OBJECT
DETACHED OBJECT
DETACHED OBJECT
DETACHED OBJECT
DETACHED OBJECT
DETACHED OBJECT
DETACHED OBJECT
DETACHED OBJECT