3095:
5980:
425:
523:
inadequate (as they note) over the age of the Solar System, since bodies "trapped in resonances" could "pass from a scattering phase to a non-scattering phase (and vice versa) numerous times." That is, trans-Neptunian objects could travel back and forth between the Kuiper belt and the scattered disc over time. Therefore, they chose instead to define the regions, rather than the objects, defining the scattered disc as "the region of orbital space that can be visited by bodies that have encountered
Neptune" within the radius of a
785:
3101:
836:
4064:
673:
705:) are very different from the scattered objects: more than 30% of all cubewanos are on low-inclination, near-circular orbits whose eccentricities peak at 0.25. Classical objects possess eccentricities ranging from 0.2 to 0.8. Though the inclinations of scattered objects are similar to the more extreme KBOs, very few scattered objects have orbits as close to the ecliptic as much of the KBO population.
6120:
6144:
5956:
6108:
5968:
6132:
724:
813:
object Eris, suggests that its paler colour could be because, at its current distance from the Sun, its atmosphere of methane is frozen over its entire surface, creating an inches-thick layer of bright white ice. Pluto, conversely, being closer to the Sun, would be warm enough that methane would freeze only onto cooler, high-
868:, are thought to have originated in the Oort cloud but to have been drawn into the inner Solar System by the gravity of the giant planets, whereas the JFCs are thought to have originated in the scattered disc. The centaurs are thought to be a dynamically intermediate stage between the scattered disc and the Jupiter family.
776:
traveled outward, it scattered many trans-Neptunian objects into higher and more eccentric orbits. This model states that 90% or more of the objects in the scattered disc may have been "promoted into these eccentric orbits by
Neptune's resonances during the migration epoch... the scattered disc might not be so scattered."
316:. Because the CCD captured more light than film (about 90% versus 10% of incoming light) and the blinking could now be done at an adjustable computer screen, the surveys allowed for higher throughput. A flood of new discoveries was the result: over a thousand trans-Neptunian objects were detected between 1992 and 2006.
266:, a population of icy bodies between Jupiter and Neptune, being the intermediate stage in an object's migration from the disc to the inner Solar System. Eventually, perturbations from the giant planets send such objects towards the Sun, transforming them into periodic comets. Many objects of the proposed
905:
The literature is inconsistent in the use of the phrases "scattered disc" and "Kuiper belt". For some, they are distinct populations; for others, the scattered disc is part of the Kuiper belt. Authors may even switch between these two uses in a single publication. In this article, the scattered disc
871:
There are many differences between SDOs and JFCs, even though many of the
Jupiter-family comets may have originated in the scattered disc. Although the centaurs share a reddish or neutral coloration with many SDOs, their nuclei are bluer, indicating a fundamental chemical or physical difference. One
758:
Models for a continuous formation throughout the age of the Solar System illustrate that at weak resonances within the Kuiper belt (such as 5:7 or 8:1), or at the boundaries of stronger resonances, objects can develop weak orbital instabilities over millions of years. The 4:7 resonance in particular
685:
The scattered disc is a very dynamic environment. Because they are still capable of being perturbed by
Neptune, SDOs' orbits are always in danger of disruption; either of being sent outward to the Oort cloud or inward into the centaur population and ultimately the Jupiter family of comets. For this
518:
The MPC, however, makes a clear distinction between the Kuiper belt and the scattered disc, separating those objects in stable orbits (the Kuiper belt) from those in scattered orbits (the scattered disc and the centaurs). However, the difference between the Kuiper belt and the scattered disc is not
812:
One explanation is the exposure of whiter subsurface layers by impacts; another is that the scattered objects' greater distance from the Sun creates a composition gradient, analogous to the composition gradient of the terrestrial and gas giant planets. Michael E. Brown, discoverer of the scattered
655:
and C. Van
Laerhoven in 2007, uses 10-million-year orbit integration instead of the Tisserand parameter. An object qualifies as an SDO if its orbit is not resonant, has a semi-major axis no greater than 2000 AU, and, during the integration, its semi-major axis shows an excursion of 1.5 AU or more.
620:
There are no clear boundaries between the scattered and detached regions. Gomes et al. define SDOs as having "highly eccentric orbits, perihelia beyond
Neptune, and semi-major axes beyond the 1:2 resonance." By this definition, all distant detached objects are SDOs. Since detached objects' orbits
803:
Astronomers originally supposed that the entire trans-Neptunian population would show a similar red surface colour, as they were thought to have originated in the same region and subjected to the same physical processes. Specifically, SDOs were expected to have large amounts of surface methane,
775:
with scattered objects. Once the orbits of
Jupiter and Saturn shifted to a 2:1 resonance (two Jupiter orbits for each orbit of Saturn), their combined gravitational pull disrupted the orbits of Uranus and Neptune, sending Neptune into the temporary "chaos" of the proto-Kuiper belt. As Neptune
522:
Morbidelli and Brown propose that the difference between objects in the Kuiper belt and scattered-disc objects is that the latter bodies "are transported in semi-major axis by close and distant encounters with
Neptune," but the former experienced no such close encounters. This delineation is
242:
Although the closest scattered-disc objects approach the Sun at about 30–35 AU, their orbits can extend well beyond 100 AU. This makes scattered objects among the coldest and most distant objects in the Solar System. The innermost portion of the scattered disc overlaps with a
493:
In contrast to the Kuiper belt, the scattered-disc population can be disturbed by
Neptune. Scattered-disc objects come within gravitational range of Neptune at their closest approaches (~30 AU) but their farthest distances reach many times that. Ongoing research suggests that the
770:
beyond Saturn, as too little primordial matter existed at that range to produce objects of such high mass. Instead, these planets, and Saturn, may have formed closer to
Jupiter, but were flung outwards during the early evolution of the Solar System, perhaps through exchanges of
708:
Although motions in the scattered disc are random, they do tend to follow similar directions, which means that SDOs can become trapped in temporary resonances with Neptune. Examples of possible resonant orbits within the scattered disc include 1:3, 2:7, 3:11, 5:22 and 4:79.
478:, allow KBOs to persist in regions which Neptune's gravitational influence would otherwise have cleared out over the age of the Solar System, since the objects are never close enough to Neptune to be scattered by its gravity. Those in 2:3 resonances are known as "
676:
Distribution of trans-Neptunian objects, with semi-major axis on the horizontal, and inclination on the vertical axis. Scattered disc objects are shown in grey, objects that are in resonance with Neptune in red. Classical Kuiper belt objects (cubewanos) and
31:
4397:
697:
greater than 50 AU, but their perihelia bring them within influence of Neptune. Having a perihelion of roughly 30 AU is one of the defining characteristics of scattered objects, as it allows Neptune to exert its gravitational influence.
727:
Simulation showing Outer Planets and Kuiper Belt: a) Before Jupiter/Saturn 2:1 resonance b) Scattering of Kuiper-belt objects into the Solar System after the orbital shift of Neptune c) After ejection of Kuiper-belt bodies by
751:. The amount of time for this process to occur remains uncertain. One hypothesis estimates a period equal to the entire age of the Solar System; a second posits that the scattering took place relatively quickly, during Neptune's early
563:
distance of 76 AU, it is too remote to be affected by the gravitational attraction of the outer planets. Under this definition, an object with a perihelion greater than 40 AU could be classified as outside the scattered disc.
502:
that orbit between Jupiter and Neptune, may simply be SDOs thrown into the inner reaches of the Solar System by Neptune, making them "cis-Neptunian" rather than trans-Neptunian scattered objects. Some objects, like (29981) 1999
519:
clear-cut, and many astronomers see the scattered disc not as a separate population but as an outward region of the Kuiper belt. Another term used is "scattered Kuiper-belt object" (or SKBO) for bodies of the scattered disc.
474:, those which Neptune has locked into a precise orbital ratio such as 2:3 (the object goes around twice for every three Neptune orbits) and 1:2 (the object goes around once for every two Neptune orbits). These ratios, called
440:, has been hypothesized, although no confirmed direct observations of the Oort cloud have been made. Some researchers further suggest a transitional space between the scattered disc and the inner Oort cloud, populated with "
410:). Although the numbers of objects in the Kuiper belt and the scattered disc are hypothesized to be roughly equal, observational bias due to their greater distance means that far fewer SDOs have been observed to date.
853:. However, studies of the region since 1992 have shown that the orbits within the Kuiper belt are relatively stable, and that ecliptic comets originate from the scattered disc, where orbits are generally less stable.
686:
reason Gladman et al. prefer to refer to the region as the scattering disc, rather than scattered. Unlike Kuiper-belt objects (KBOs), the orbits of scattered-disc objects can be inclined as much as 40° from the
759:
has large instability. KBOs can also be shifted into unstable orbits by close passage of massive objects, or through collisions. Over time, the scattered disc would gradually form from these isolated events.
808:
by sunlight from the Sun. This would absorb blue light, creating a reddish hue. Most classical objects display this colour, but scattered objects do not; instead, they present a white or greyish appearance.
5883:
5457:
5853:
856:
Comets can loosely be divided into two categories: short-period and long-period—the latter being thought to originate in the Oort cloud. The two major categories of short-period comets are
5654:
605:
may also be an inner Oort-cloud object or (more likely) a transitional object between the scattered disc and the inner Oort cloud. More recently, these objects have been referred to as
664:. (Objects with smaller eccentricity are considered classical.) In this scheme, the disc extends from the orbit of Neptune to 2000 AU, the region referred to as the inner Oort cloud.
166:
732:
The scattered disc is still poorly understood: no model of the formation of the Kuiper belt and the scattered disc has yet been proposed that explains all their observed properties.
296:
were used in astronomy to detect objects in the Solar System, because these objects would move between two exposures—this involved time-consuming steps like exposing and developing
1501:
800:. Spectral analysis of selected Kuiper belt and scattered objects has revealed signatures of similar compounds. Both Pluto and Eris, for instance, show signatures for methane.
4100:
660:
to emphasize this present mobility. If the object is not an SDO as per the above definition, but the eccentricity of its orbit is greater than 0.240, it is classified as a
1690:
Remo notes that Cis-Neptunian bodies "include terrestrial and large gaseous planets, planetary moons, asteroids, and main-belt comets within Neptune's orbit." (Remo 2007)
6181:
5890:
436:
Known trans-Neptunian objects are often divided into two subpopulations: the Kuiper belt and the scattered disc. A third reservoir of trans-Neptunian objects, the
5442:
6171:
1872:
Gomes, Rodney S.; Matese, John J.; Lissauer, Jack J. (October 2006). "A distant planetary-mass solar companion may have produced distant detached objects".
5587:
2797:
2525:
Hahn, Joseph M.; Malhotra, Renu (13 July 2005). "Neptune's Migration into a Stirred–Up Kuiper Belt: A Detailed Comparison of Simulations to Observations".
718:
159:
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Lykawka, Patryk Sofia; Mukai, Tadashi (2007). "Dynamical classification of trans-Neptunian objects: Probing their origin, evolution, and interrelation".
1701:
2109:"The Deep Ecliptic Survey: A Search for Kuiper Belt Objects and Centaurs. II. Dynamical Classification, the Kuiper Belt Plane, and the Core Population"
5353:
3653:
374:
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2874:
1107:
5508:
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5138:
5118:
4377:
152:
2272:
5452:
5185:
5148:
5143:
2657:
2189:
1853:
1613:
1470:
1429:
1264:
1246:
1187:
985:
2459:
Levison, Harold F.; Duncan, Martin J. (1997). "From the Kuiper Belt to Jupiter-Family Comets: The Spatial Distribution of Ecliptic Comets".
872:
hypothesis is that comet nuclei are resurfaced as they approach the Sun by subsurface materials which subsequently bury the older material.
5878:
5469:
5190:
5128:
5123:
762:
Computer simulations have also suggested a more rapid and earlier formation for the scattered disc. Modern theories indicate that neither
1907:
Morbidelli, Alessandro; Levison, Harold F. (November 2004). "Scenarios for the Origin of the Orbits of the Trans-Neptunian Objects 2000 CR
621:
cannot be produced by Neptune scattering, alternative scattering mechanisms have been put forward, including a passing star or a distant,
559:
has suggested instead that it should be considered an inner Oort-cloud object rather than a member of the scattered disc, because, with a
2356:; Morbidelli, Alessandro (2003-11-27). "The formation of the Kuiper belt by the outward transport of bodies during Neptune's migration".
1061:
6032:
5133:
1376:
4408:
4086:
5254:
5281:
4217:
3139:
1076:
5669:
1753:"Sedna (The coldest most distant place known in the solar system; possibly the first object in the long-hypothesized Oort cloud)"
636:(i.e. detached objects). Scattered-near objects are those whose orbits are non-resonant, non-planetary-orbit-crossing and have a
628:
A scheme introduced by a 2005 report from the Deep Ecliptic Survey by J. L. Elliott et al. distinguishes between two categories:
6176:
4430:
3302:
3094:
886:
487:
471:
429:
111:
95:
84:
4426:
4411:
5848:
5264:
5098:
4420:
4149:
2894:
1455:
881:
118:
4419:
531:> 30 AU region"; the region of the Solar System populated by objects with semi-major axes greater than 30 AU.
5373:
5269:
4417:
4414:
4410:
4406:
4308:
2578:
Thommes, E. W.; Duncan, M. J.; Levison, H. F. (May 2002). "The Formation of Uranus and Neptune Among Jupiter and Saturn".
6098:
5873:
5428:
5408:
5303:
4424:
4416:
3325:
467:
391:
78:
4413:
5948:
5474:
5403:
5368:
4431:
4427:
4134:
2867:
424:
4422:
5863:
5664:
5547:
5496:
4432:
4370:
4298:
4288:
5706:
5681:
5491:
4293:
196:
2836:
300:, and people then using a blink comparator to manually detect prospective objects. During the 1980s, the use of
5997:
5602:
5197:
4129:
2205:
Bertoldi, F.; Altenhoff, W.; Weiss, A.; Menten, K. M.; Thum, C. (2 February 2006). "The trans-Neptunian object
258:
Because of its unstable nature, astronomers now consider the scattered disc to be the place of origin for most
232:
1709:
792:
Scattered objects, like other trans-Neptunian objects, have low densities and are composed largely of frozen
5686:
5513:
5160:
5064:
4977:
4677:
4527:
4313:
4197:
4109:
3069:
793:
586:
to be influenced by it. This led to a discussion among astronomers about a new minor planet set, called the
5691:
5629:
5577:
5567:
5552:
5503:
5388:
5363:
5293:
4715:
4429:
4234:
4067:
2860:
622:
512:
495:
419:
263:
200:
66:
56:
4407:
4401:
1241:(Sixth revised and enlarged ed.). Heidelberg ; New York: Springer. pp. 925 (Appendix 10).
6166:
6057:
5984:
5858:
5711:
5674:
5562:
5557:
4363:
4139:
462:(or "doughnut") of space, extending from about 30 to 50 AU comprising two main populations of
301:
4428:
928:
784:
5619:
5572:
5530:
5229:
4687:
4652:
4647:
4541:
4492:
4465:
4207:
3083:
2965:
2957:
2946:
2812:
2749:
2706:
2680:
2649:
2641:
2597:
2544:
2468:
2425:
2367:
2297:
2221:
2177:
2120:
2058:
1991:
1934:
1881:
1785:
1655:
1605:
1597:
1565:
1421:
1415:
1312:
1122:
1024:
857:
843:
740:
407:
204:
47:
4425:
1351:
227:
10 mi). These extreme orbits are thought to be the result of gravitational "scattering" by the
6148:
6071:
5960:
5798:
5771:
5721:
5525:
4989:
4682:
4534:
4016:
3996:
3986:
3976:
3966:
3859:
3714:
3704:
3631:
3621:
3569:
3559:
3519:
3486:
3456:
3446:
3256:
3216:
3173:
3055:
2990:
2684:
641:
637:
569:
508:
395:
34:
3100:
625:. Alternatively, it has been suggested that these objects have been captured from a passing star.
6136:
6124:
6051:
5921:
5868:
5786:
5746:
5716:
5624:
5437:
4574:
4418:
4409:
4006:
3837:
3827:
3817:
3807:
3778:
3768:
3746:
3724:
3694:
3684:
3611:
3601:
3591:
3539:
3476:
3466:
3436:
3416:
3386:
3364:
3354:
3311:
3276:
3246:
3236:
3226:
3183:
2828:
2773:
2722:
2696:
2613:
2587:
2560:
2534:
2391:
2321:
2287:
2245:
2138:
2084:
2048:
2017:
1981:
1950:
1924:
1673:
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1138:
1042:
1014:
956:
463:
383:
188:
955:
Morbidelli, Alessandro (2005). "Origin and dynamical evolution of comets and their reservoirs".
428:
The eccentricity and inclination of the scattered-disc population compared to the classical and
4403:
788:
The infrared spectra of both Eris and Pluto, highlighting their common methane absorption lines
5911:
5791:
5481:
5423:
5214:
5103:
5029:
4970:
4941:
4699:
4423:
4415:
4412:
4192:
4144:
3674:
3664:
3549:
3406:
3396:
3028:
2765:
2653:
2441:
2413:
2383:
2353:
2313:
2237:
2185:
2076:
2009:
1849:
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1179:
1172:
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865:
861:
475:
321:
297:
216:
1146:
644:(relative to Neptune) greater than 3 and have a time-averaged eccentricity greater than 0.2.
6112:
5972:
5776:
5766:
5659:
5634:
5044:
5014:
4885:
4865:
4764:
4739:
4579:
4444:
4318:
3658:
3529:
3426:
3266:
3163:
2985:
2952:
2820:
2757:
2714:
2676:
2605:
2552:
2476:
2433:
2375:
2358:
2305:
2229:
2169:
2165:
2128:
2066:
1999:
1942:
1889:
1793:
1663:
1573:
1380:
1130:
1082:
1032:
772:
652:
648:
556:
359:
293:
251:, but its outer limits reach much farther away from the Sun and farther above and below the
4421:
4400:
2329:
1286:
5843:
5741:
5649:
5540:
5518:
5315:
5259:
5249:
5039:
5019:
4994:
4982:
4936:
4924:
4858:
4828:
4821:
4811:
4771:
4749:
4744:
4404:
4402:
4239:
4182:
4167:
3957:
3075:
3061:
3009:
2264:
1836:
1212:
694:
579:
540:
441:
403:
378:
271:
123:
38:
2816:
2753:
2710:
2601:
2548:
2472:
2429:
2371:
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4833:
4786:
4405:
4222:
4187:
3338:
3147:
3129:
2995:
850:
259:
61:
693:
SDOs are typically characterized by orbits with medium and high eccentricities with a
6160:
5926:
5906:
5486:
5219:
5202:
5023:
4946:
4909:
4880:
4870:
4838:
4816:
4796:
4759:
4732:
4727:
4722:
4278:
4177:
4172:
3116:
2907:
2902:
2832:
2498:
2088:
2021:
1954:
1668:
1633:
1037:
1002:
748:
313:
17:
2777:
2617:
2564:
2142:
1046:
486:
is the largest member of their group, whereas those in 1:2 resonances are known as "
6004:
5990:
5781:
5736:
5393:
5276:
5170:
5110:
5093:
4919:
4897:
4848:
4806:
4791:
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made it possible to directly produce electronic images that could then be readily
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Gomes, Rodney S.; Fernandez, Julio A.; Gallardo, Tabare; Brunini, Adrian (2008).
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5464:
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5337:
5298:
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4781:
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4283:
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3210:
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1600:. In Lucy-Ann Adams McFadden; Paul Robert Weissman; Torrence V. Johnson (eds.).
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The Kuiper belt was initially thought to be the source of the Solar System's
6025:
6018:
5447:
5413:
5244:
5165:
5088:
5083:
4801:
4754:
4623:
4606:
4339:
4229:
4078:
3941:
3929:
3917:
3905:
3756:
3579:
3496:
3286:
3124:
2761:
2071:
2036:
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3022:
2917:
2701:
2592:
2539:
2292:
1929:
1650:
1019:
961:
839:
687:
252:
2379:
2233:
1554:"Thermal Evolution and Differentiation of Edgeworth-Kuiper Belt Objects"
5320:
5308:
5234:
4633:
4611:
4486:
4471:
4030:
3800:
3197:
2929:
2912:
1755:. California Institute of Technology, Department of Geological Sciences
805:
797:
752:
678:
583:
546:
479:
357:. The first object presently classified as an SDO to be discovered was
274:
are not sharply distinct from scattered disc objects, and some such as
236:
128:
89:
723:
5761:
5054:
5049:
4958:
4953:
4667:
4662:
4628:
4616:
4561:
4513:
4506:
4481:
4476:
3047:
3042:
3036:
3014:
3003:
1071:. Austin, Texas: Astronomical Society of the Pacific. pp. 3–14.
818:
814:
763:
640:(relative to Neptune) less than 3. Scattered-extended objects have a
1003:"Simulations of the population of Centaurs - I. The bulk statistics"
470:(or "cubewanos"), which lie in orbits untouched by Neptune, and the
2824:
2718:
2609:
2556:
2309:
2133:
2108:
2053:
1986:
1946:
1578:
1553:
319:
The first scattered-disc object (SDO) to be recognised as such was
5078:
4657:
4589:
4584:
4499:
4454:
4449:
4270:
2979:
1456:"The Kuiper Belt and the Primordial Evolution of the Solar System"
1134:
834:
830:
671:
483:
459:
336:
in Hawaii. Three more were identified by the same survey in 1999:
244:
1352:"Discovery Circumstances: Numbered Minor Planets (90001)-(95000)"
1106:
Luu, Jane X.; Marsden, Brian G.; Jewitt, David C. (5 June 1997).
735:
According to contemporary models, the scattered disc formed when
4710:
4594:
4459:
2852:
1632:
Horner, J.; Evans, N. W.; Bailey, Mark E.; Asher, D. J. (2003).
37:(center), the largest known scattered-disc object, and its moon
4359:
4355:
4082:
2856:
2107:
Elliot, J. L.; Kern, S. D.; Clancy, K. B.; et al. (2005).
747:
orbits by gravitational interaction with Neptune and the other
4439:
1839:; Delsanti, A. (2006). "The Solar System Beyond The Planets".
906:
will be considered a separate population from the Kuiper belt.
551:
The Minor Planet Center classifies the trans-Neptunian object
1465:. Tucson (AZ): University of Arizona Press. pp. 175–91.
864:. Halley-type comets, which are named after their prototype,
278:
have sometimes been considered to be included in this group.
4395:
2648:(2nd ed.). Amsterdam; Boston: Academic Press. pp.
1604:(2nd ed.). Amsterdam; Boston: Academic Press. pp.
1420:(2nd ed.). Amsterdam; Boston: Academic Press. pp.
1174:
Beyond Pluto: Exploring the Outer Limits of the Solar System
247:-shaped region of orbiting objects traditionally called the
1108:"A new dynamical class of object in the outer Solar System"
270:
are also thought to have originated in the scattered disc.
2160:
2158:
2156:
2154:
2152:
1634:"The Populations of Comet-like Bodies in the Solar System"
373:
As of 2011, over 200 SDOs have been identified, including
527:, and the Kuiper belt as its "complement ... in the
1970:"Outer Solar System Possibly Shaped by a Stellar Fly-by"
1454:
Morbidelli, Alessandro; Brown, Michael E. (2004-11-01).
1552:
De Sanctis, M. C.; Capria, M. T.; Coradini, A. (2001).
1069:
New Horizons in Astronomy: Frank N. Bash Symposium 2005
2407:
2405:
1526:"The Scattered Disk: Origins, Dynamics and End States"
1461:. In M. C. Festou; H. U. Keller; H. A. Weaver (eds.).
980:. San Diego: Academic Press. pp. 584 (footnote).
6096:
5899:
5836:
5586:
5422:
5352:
5063:
5005:
4698:
4560:
4327:
4269:
4206:
4158:
4116:
4029:
3956:
3644:
3511:
3324:
3301:
3196:
3138:
3115:
3108:
2938:
1596:Morbidelli, Alessandro; Levison, Harold F. (2007).
1171:
2102:
2100:
2098:
2041:Monthly Notices of the Royal Astronomical Society
1638:Monthly Notices of the Royal Astronomical Society
1379:. SwRI (Space Science Department). Archived from
1331:"Discovery Circumstances: Numbered Minor Planets"
1007:Monthly Notices of the Royal Astronomical Society
1500:: CS1 maint: bot: original URL status unknown (
1001:Horner, J.; Evans, N. W.; Bailey, M. E. (2004).
950:
948:
929:"Cosmic Distance Scales – The Solar System"
377:(discovered by Schwamb, Brown, and Rabinowitz),
27:Collection of bodies in the extreme Solar System
4399:
1702:"New Object in Solar System Defies Categories"
1449:
1447:
1445:
1443:
1441:
1377:"Orbit Fit and Astrometric record for 04VN112"
199:, which are a subset of the broader family of
4371:
4094:
2868:
1867:
1865:
1627:
1625:
1287:"List Of Centaurs and Scattered-Disk Objects"
647:An alternative classification, introduced by
160:
8:
2520:
2518:
1207:
1205:
231:, and the objects continue to be subject to
45:
2176:. University of Arizona Press. p. 43.
719:Formation and evolution of the Solar System
555:as a scattered-disc object. Its discoverer
5349:
4557:
4553:
4378:
4364:
4356:
4122:
4101:
4087:
4079:
3112:
3099:
3093:
2875:
2861:
2853:
2671:
2669:
2492:
2490:
1813:"Evidence for an Extended Scattered Disk?"
1483:. Archived from the original on 2009-06-21
1259:. San Diego: Academic Press. p. 218.
1060:Sheppard, Scott S. (October 16–18, 2005).
167:
153:
44:
2791:
2789:
2787:
2700:
2635:
2633:
2631:
2629:
2627:
2591:
2538:
2291:
2273:"Population of the Scattered Kuiper Belt"
2132:
2070:
2052:
2003:
1985:
1928:
1667:
1649:
1591:
1589:
1577:
1412:"Comet Populations and Cometary Dynamics"
1410:Levison, Harold F.; Donnes, Luke (2007).
1036:
1018:
960:
203:. The scattered-disc objects (SDOs) have
5891:Interstellar and circumstellar molecules
2499:"Orbital shuffle for early solar system"
1519:
1517:
1515:
1513:
1511:
1405:
1403:
1401:
1399:
1397:
1062:"Small Bodies in the Outer Solar System"
783:
722:
515:, now lists centaurs and SDOs together.
423:
29:
6182:Astronomical objects discovered in 1996
6103:
6087:) may be read as "within" or "part of".
5115:Planetary orbit-crossing minor planets
2642:"Kuiper Belt Objects: Physical Studies"
1771:
1769:
1285:IAU: Minor Planet Center (2011-01-03).
1217:"Scattered Kuiper Belt Objects (SKBOs)"
919:
898:
511:(MPC), which officially catalogues all
402:(Brown, Trujillo, and Rabinowitz), and
1493:
1280:
1278:
1276:
1178:. Cambridge University Press. p.
458:The Kuiper belt is a relatively thick
739:objects (KBOs) were "scattered" into
414:Subdivisions of trans-Neptunian space
7:
1533:Universidad de la Republica, Uruguay
582:have a perihelion too far away from
6172:Scattered disc and detached objects
567:Sedna is not the only such object:
398:(Brown, Trujillo, and Rabinowitz),
328:, originally identified in 1996 by
681:are blue and yellow, respectively.
195:that is sparsely populated by icy
25:
1333:. Minor Planet Center. 2007-05-01
448:Scattered disc versus Kuiper belt
381:(Schwamb, Brown, and Rabinowitz)
6142:
6130:
6118:
6106:
5978:
5966:
5954:
4063:
4062:
2646:Encyclopedia of the Solar System
1669:10.1046/j.1365-8711.2003.06714.x
1602:Encyclopedia of the Solar System
1417:Encyclopedia of the Solar System
1257:Encyclopedia of the solar system
1239:Dictionary of minor planet names
1038:10.1111/j.1365-2966.2004.08240.x
978:Encyclopedia of the solar system
656:Gladman et al. suggest the term
5854:Gravitationally rounded objects
2174:The Solar System Beyond Neptune
887:List of trans-Neptunian objects
507:, blur the distinction and the
2895:List of possible dwarf planets
2497:Hansen, Kathryn (2005-06-07).
1817:Observatoire de la Cote d'Azur
882:List of possible dwarf planets
821:-covered regions bare of ice.
766:nor Neptune could have formed
578:(discovered before Sedna) and
292:Traditionally, devices like a
262:in the Solar System, with the
119:Extreme trans-Neptunian object
1:
2438:10.1126/science.276.5319.1670
1732:"The 1000 km Scale KBOs"
468:classical Kuiper-belt objects
255:than the Kuiper belt proper.
1894:10.1016/j.icarus.2006.05.026
1798:10.1016/j.icarus.2007.01.001
1309:Minor Planet Electronic Circ
817:regions, leaving low-albedo
472:resonant Kuiper-belt objects
298:photographic plates or films
5949:Outline of the Solar System
5712:Interplanetary medium/space
2640:Tegler, Stephen C. (2007).
1170:Davies, John Keith (2001).
6198:
5665:Extraterrestrial materials
1237:Schmadel, Lutz D. (2012).
828:
716:
544:
538:
451:
417:
288:History of the Kuiper belt
285:
5985:Earth sciences portal
5944:
5707:Interplanetary dust cloud
4551:
4393:
4125:
4110:Small Solar System bodies
4058:
3091:
2890:
2796:Jewitt, David C. (2001).
2689:The Astrophysical Journal
2280:The Astrophysical Journal
1974:The Astrophysical Journal
1730:Jewitt, David C. (2008).
1219:. Institute for Astronomy
831:Comet § Short period
197:small Solar System bodies
5998:Local Interstellar Cloud
4716:other near-Earth objects
2805:The Astronomical Journal
2580:The Astronomical Journal
2113:The Astronomical Journal
2005:10.3847/1538-4357/aad23c
1917:The Astronomical Journal
1700:Silber, Kenneth (1999).
1558:The Astronomical Journal
927:Masetti, Maggie (2007).
804:chemically altered into
632:(i.e. typical SDOs) and
611:distant detached objects
207:ranging as high as 0.8,
5961:Solar System portal
5687:Giant-impact hypothesis
5294:Trans-Neptunian objects
2762:10.1126/science.1100553
2263:Trujillo, Chadwick A.;
2212:is larger than Pluto".
701:The classical objects (
588:extended scattered disc
513:trans-Neptunian objects
201:trans-Neptunian objects
67:Trans-Neptunian objects
6177:Trans-Neptunian region
5849:Possible dwarf planets
5692:Gravitational collapse
5630:Circumstellar envelope
4435:
4235:Trans-Neptunian object
2481:10.1006/icar.1996.5637
1848:. Springer-Praxis Ed.
1598:"Kuiper Belt Dynamics"
846:
789:
729:
682:
658:scattering disk object
433:
420:Trans-Neptunian object
205:orbital eccentricities
106:Scattered disc objects
42:
6058:Laniakea Supercluster
5675:Sample-return mission
4434:
2899:Former dwarf planets
2681:Trujillo, Chadwick A.
2072:10.1093/mnras/stv1803
1712:on September 21, 2005
1354:. Minor Planet Center
858:Jupiter-family comets
838:
787:
726:
675:
427:
48:distant minor planets
33:
18:Scattered disk object
5973:Astronomy portal
5874:Solar System objects
5620:Circumplanetary disk
4208:Distant minor planet
2685:Rabinowitz, David L.
2527:Astronomical Journal
1784:(1). Kobe: 213–232.
844:Jupiter-family comet
408:Deep Ecliptic Survey
211:as high as 40°, and
6072:Observable universe
5869:Solar System models
5799:Protoplanetary disk
5722:Interstellar medium
5682:Frost/Ice/Snow line
2817:2002AJ....123.1039J
2754:2005Sci...307...71G
2711:2005ApJ...635L..97B
2602:2002AJ....123.2862T
2549:2005AJ....130.2392H
2473:1997Icar..127...13L
2430:1997Sci...276.1670D
2424:(5319): 1670–1672.
2412:Duncan, Martin J.;
2380:10.1038/nature02120
2372:2003Natur.426..419L
2302:2000ApJ...529L.103T
2234:10.1038/nature04494
2226:2006Natur.439..563B
2182:2008ssbn.book...43G
2125:2005AJ....129.1117E
2063:2015MNRAS.453.3157J
1996:2018ApJ...863...45P
1939:2004AJ....128.2564M
1886:2006Icar..184..589G
1790:2007Icar..189..213L
1660:2003MNRAS.343.1057H
1570:2001AJ....121.2792D
1317:2008MPEC....D...38S
1127:1997Natur.387..573L
1029:2004MNRAS.354..798H
642:Tisserand parameter
638:Tisserand parameter
623:planet-sized object
509:Minor Planet Center
464:Kuiper belt objects
432:Kuiper-belt objects
366:, found in 1995 by
312:and transferred to
73:Kuiper belt objects
50:
6052:Virgo Supercluster
6033:Milky Way subgroup
5864:Natural satellites
5747:Nebular hypothesis
5727:Interstellar space
5717:Interstellar cloud
5625:Circumstellar disc
5215:Near-Earth objects
5099:names and meanings
4436:
2414:Levison, Harold F.
2354:Levison, Harold F.
2335:on August 12, 2007
1811:Gladman, Brett J.
1751:Brown, Michael E.
1152:on August 12, 2007
862:Halley-type comets
847:
796:such as water and
790:
730:
683:
634:scattered-extended
476:orbital resonances
434:
304:-based cameras in
217:astronomical units
189:circumstellar disc
138:Oort cloud objects
43:
6094:
6093:
5939:
5938:
5935:
5934:
5912:Lagrangian points
5884:by discovery date
5482:Human spaceflight
5453:historical models
5346:
5345:
4971:S/2015 (136472) 1
4353:
4352:
4265:
4264:
4150:Meanings of names
4076:
4075:
4054:
4053:
2677:Brown, Michael E.
2659:978-0-12-088589-3
2366:(6965): 419–421.
2220:(7076): 563–564.
2191:978-0-8165-2755-7
2170:Marsden, Brian G.
2166:Gladman, Brett J.
1855:978-3-540-26056-1
1615:978-0-12-088589-3
1472:978-0-8165-2450-1
1431:978-0-12-088589-3
1266:978-0-12-226805-2
1248:978-3-642-29717-5
1189:978-0-521-80019-8
1121:(6633): 573–575.
987:978-0-12-226805-2
498:, a class of icy
177:
176:
16:(Redirected from
6189:
6147:
6146:
6145:
6135:
6134:
6133:
6123:
6122:
6121:
6111:
6110:
6109:
6102:
6088:
6086:
6077:
6070:
6063:
6056:
6050:
6044:
6038:
6031:
6024:
6017:
6010:
6003:
5996:
5983:
5982:
5981:
5971:
5970:
5969:
5959:
5958:
5957:
5660:Exozodiacal dust
5350:
5316:Detached objects
4558:
4554:
4398:
4380:
4373:
4366:
4357:
4123:
4103:
4096:
4089:
4080:
4066:
4065:
4047:
4045:
4044:
4022:
4012:
4002:
3992:
3982:
3972:
3958:Detached objects
3949:
3947:
3946:
3937:
3935:
3934:
3925:
3923:
3922:
3913:
3911:
3910:
3901:
3899:
3898:
3889:
3887:
3886:
3877:
3875:
3874:
3865:
3855:
3853:
3852:
3843:
3833:
3823:
3813:
3803:
3796:
3794:
3793:
3784:
3774:
3764:
3762:
3761:
3752:
3742:
3740:
3739:
3730:
3720:
3710:
3700:
3690:
3680:
3670:
3637:
3627:
3617:
3607:
3597:
3587:
3585:
3584:
3575:
3565:
3555:
3545:
3535:
3525:
3504:
3502:
3501:
3492:
3482:
3472:
3462:
3452:
3442:
3432:
3422:
3412:
3402:
3392:
3382:
3380:
3379:
3370:
3360:
3317:
3294:
3292:
3291:
3282:
3272:
3262:
3252:
3242:
3232:
3222:
3189:
3179:
3169:
3113:
3103:
3097:
2877:
2870:
2863:
2854:
2844:
2843:
2841:
2835:. Archived from
2811:(2): 1039–1049.
2802:
2793:
2782:
2781:
2737:
2731:
2730:
2704:
2702:astro-ph/0508633
2673:
2664:
2663:
2637:
2622:
2621:
2595:
2593:astro-ph/0111290
2575:
2569:
2568:
2542:
2540:astro-ph/0507319
2522:
2513:
2512:
2510:
2509:
2494:
2485:
2484:
2456:
2450:
2449:
2409:
2400:
2399:
2350:
2344:
2343:
2341:
2340:
2334:
2328:. Archived from
2295:
2293:astro-ph/9912428
2286:(2): L103–L106.
2277:
2265:Jewitt, David C.
2260:
2254:
2253:
2211:
2202:
2196:
2195:
2162:
2147:
2146:
2136:
2119:(2): 1117–1162.
2104:
2093:
2092:
2074:
2056:
2047:(3): 3158–3163.
2032:
2026:
2025:
2007:
1989:
1965:
1959:
1958:
1932:
1930:astro-ph/0403358
1923:(5): 2564–2576.
1904:
1898:
1897:
1869:
1860:
1859:
1847:
1837:Jewitt, David C.
1833:
1827:
1826:
1824:
1823:
1808:
1802:
1801:
1773:
1764:
1763:
1761:
1760:
1748:
1742:
1741:
1739:
1738:
1727:
1721:
1720:
1718:
1717:
1708:. Archived from
1697:
1691:
1688:
1682:
1681:
1671:
1653:
1651:astro-ph/0304319
1644:(4): 1057–1066.
1629:
1620:
1619:
1593:
1584:
1583:
1581:
1564:(5): 2792–2799.
1549:
1543:
1542:
1540:
1539:
1530:
1521:
1506:
1505:
1499:
1491:
1489:
1488:
1460:
1451:
1436:
1435:
1407:
1392:
1391:
1389:
1388:
1369:
1363:
1362:
1360:
1359:
1348:
1342:
1341:
1339:
1338:
1327:
1321:
1320:
1311:. 2008-D38: 38.
1304:
1298:
1297:
1295:
1294:
1282:
1271:
1270:
1252:
1234:
1228:
1227:
1225:
1224:
1213:Jewitt, David C.
1209:
1200:
1199:
1197:
1196:
1177:
1167:
1161:
1160:
1158:
1157:
1151:
1145:. Archived from
1112:
1103:
1097:
1096:
1094:
1093:
1087:
1081:. Archived from
1066:
1057:
1051:
1050:
1040:
1022:
1020:astro-ph/0407400
998:
992:
991:
973:
967:
966:
964:
962:astro-ph/0512256
952:
943:
942:
940:
939:
924:
907:
903:
773:angular momentum
604:
602:
601:
577:
575:
574:
570:(148209) 2000 CR
557:Michael E. Brown
535:Detached objects
442:detached objects
389:
365:
356:
349:
342:
327:
294:blink comparator
272:Detached objects
226:
222:
215:greater than 30
169:
162:
155:
124:Detached objects
51:
41:(left of object)
21:
6197:
6196:
6192:
6191:
6190:
6188:
6187:
6186:
6157:
6156:
6153:
6143:
6141:
6131:
6129:
6119:
6117:
6107:
6105:
6097:
6095:
6090:
6084:
6082:
6081:
6075:
6068:
6061:
6054:
6048:
6042:
6036:
6029:
6022:
6015:
6008:
6001:
5994:
5979:
5977:
5967:
5965:
5955:
5953:
5940:
5931:
5895:
5832:
5816:vs. Hill sphere
5742:Molecular cloud
5670:Sample curation
5650:Detached object
5589:
5582:
5426:
5418:
5355:
5342:
5287:Neptune trojans
5070:
5068:
5066:
5059:
5001:
4694:
4565:
4547:
4433:
4396:
4389:
4384:
4354:
4349:
4323:
4261:
4202:
4154:
4112:
4107:
4077:
4072:
4050:
4042:
4041:
4038:
4025:
4020:
4015:
4010:
4005:
4000:
3995:
3990:
3985:
3980:
3975:
3970:
3965:
3952:
3944:
3943:
3940:
3932:
3931:
3928:
3920:
3919:
3916:
3908:
3907:
3904:
3896:
3895:
3892:
3884:
3883:
3880:
3872:
3871:
3868:
3863:
3858:
3850:
3849:
3846:
3841:
3836:
3831:
3826:
3821:
3816:
3811:
3806:
3799:
3791:
3790:
3787:
3782:
3777:
3772:
3767:
3759:
3758:
3755:
3750:
3745:
3737:
3736:
3733:
3728:
3723:
3718:
3713:
3708:
3703:
3698:
3693:
3688:
3683:
3678:
3673:
3668:
3663:
3640:
3635:
3630:
3625:
3620:
3615:
3610:
3605:
3600:
3595:
3590:
3582:
3581:
3578:
3573:
3568:
3563:
3558:
3553:
3548:
3543:
3538:
3533:
3528:
3523:
3518:
3507:
3499:
3498:
3495:
3490:
3485:
3480:
3475:
3470:
3465:
3460:
3455:
3450:
3445:
3440:
3435:
3430:
3425:
3420:
3415:
3410:
3405:
3400:
3395:
3390:
3385:
3377:
3376:
3373:
3368:
3363:
3358:
3353:
3320:
3315:
3310:
3297:
3289:
3288:
3285:
3280:
3275:
3270:
3265:
3260:
3255:
3250:
3245:
3240:
3235:
3230:
3225:
3220:
3215:
3192:
3187:
3182:
3177:
3172:
3167:
3162:
3134:
3104:
3098:
3089:
2934:
2886:
2881:
2850:
2848:
2847:
2839:
2800:
2795:
2794:
2785:
2748:(5706): 71–75.
2739:
2738:
2734:
2695:(1): L97–L100.
2675:
2674:
2667:
2660:
2639:
2638:
2625:
2577:
2576:
2572:
2533:(5): 2392–414.
2524:
2523:
2516:
2507:
2505:
2496:
2495:
2488:
2458:
2457:
2453:
2411:
2410:
2403:
2352:
2351:
2347:
2338:
2336:
2332:
2275:
2262:
2261:
2257:
2210:
2206:
2204:
2203:
2199:
2192:
2164:
2163:
2150:
2106:
2105:
2096:
2034:
2033:
2029:
1967:
1966:
1962:
1914:
1910:
1906:
1905:
1901:
1871:
1870:
1863:
1856:
1845:
1835:
1834:
1830:
1821:
1819:
1810:
1809:
1805:
1775:
1774:
1767:
1758:
1756:
1750:
1749:
1745:
1736:
1734:
1729:
1728:
1724:
1715:
1713:
1699:
1698:
1694:
1689:
1685:
1631:
1630:
1623:
1616:
1595:
1594:
1587:
1551:
1550:
1546:
1537:
1535:
1528:
1523:
1522:
1509:
1492:
1486:
1484:
1473:
1458:
1453:
1452:
1439:
1432:
1409:
1408:
1395:
1386:
1384:
1371:
1370:
1366:
1357:
1355:
1350:
1349:
1345:
1336:
1334:
1329:
1328:
1324:
1306:
1305:
1301:
1292:
1290:
1284:
1283:
1274:
1267:
1254:
1249:
1236:
1235:
1231:
1222:
1220:
1215:(August 2009).
1211:
1210:
1203:
1194:
1192:
1190:
1169:
1168:
1164:
1155:
1153:
1149:
1110:
1105:
1104:
1100:
1091:
1089:
1085:
1079:
1064:
1059:
1058:
1054:
1000:
999:
995:
988:
975:
974:
970:
954:
953:
946:
937:
935:
926:
925:
921:
916:
911:
910:
904:
900:
895:
878:
851:ecliptic comets
833:
827:
782:
721:
715:
695:semi-major axis
670:
599:
598:
595:
580:474640 Alicanto
572:
571:
568:
549:
543:
541:Detached object
537:
506:
456:
450:
422:
416:
404:474640 Alicanto
387:
382:
363:
358:
355:
351:
348:
344:
341:
337:
325:
320:
290:
284:
260:periodic comets
224:
223:10 km; 2.8
220:
187:) is a distant
173:
98:(1:2 resonance)
92:(2:3 resonance)
62:Neptune trojans
28:
23:
22:
15:
12:
11:
5:
6195:
6193:
6185:
6184:
6179:
6174:
6169:
6159:
6158:
6152:
6151:
6139:
6127:
6115:
6092:
6091:
5988:
5987:
5975:
5963:
5951:
5945:
5942:
5941:
5937:
5936:
5933:
5932:
5930:
5929:
5924:
5919:
5914:
5909:
5903:
5901:
5897:
5896:
5894:
5893:
5888:
5887:
5886:
5881:
5871:
5866:
5861:
5856:
5851:
5846:
5840:
5838:
5834:
5833:
5831:
5830:
5828:Scattered disc
5825:
5820:
5819:
5818:
5808:
5803:
5802:
5801:
5796:
5795:
5794:
5784:
5779:
5774:
5769:
5759:
5754:
5749:
5744:
5739:
5734:
5729:
5724:
5719:
5714:
5709:
5704:
5699:
5694:
5689:
5684:
5679:
5678:
5677:
5672:
5662:
5657:
5652:
5647:
5642:
5637:
5632:
5627:
5622:
5617:
5616:
5615:
5613:Excretion disk
5608:Accretion disk
5605:
5600:
5598:Star formation
5594:
5592:
5584:
5583:
5581:
5580:
5575:
5570:
5565:
5560:
5555:
5550:
5545:
5544:
5543:
5533:
5528:
5523:
5522:
5521:
5511:
5506:
5501:
5500:
5499:
5494:
5489:
5487:space stations
5479:
5478:
5477:
5472:
5462:
5461:
5460:
5455:
5450:
5440:
5434:
5432:
5420:
5419:
5417:
5416:
5411:
5406:
5401:
5396:
5391:
5386:
5381:
5376:
5371:
5366:
5360:
5358:
5347:
5344:
5343:
5341:
5340:
5335:
5334:
5333:
5328:
5326:Scattered disc
5323:
5318:
5313:
5312:
5311:
5306:
5291:
5290:
5289:
5284:
5274:
5273:
5272:
5267:
5262:
5257:
5252:
5247:
5242:
5237:
5232:
5222:
5217:
5212:
5211:
5210:
5205:
5200:
5195:
5194:
5193:
5188:
5178:
5173:
5168:
5158:
5157:
5156:
5151:
5146:
5141:
5136:
5131:
5126:
5121:
5113:
5108:
5107:
5106:
5101:
5091:
5086:
5081:
5075:
5073:
5061:
5060:
5058:
5057:
5052:
5047:
5042:
5037:
5032:
5027:
5017:
5011:
5009:
5003:
5002:
5000:
4999:
4998:
4997:
4987:
4986:
4985:
4975:
4974:
4973:
4963:
4962:
4961:
4951:
4950:
4949:
4944:
4934:
4933:
4932:
4927:
4922:
4917:
4912:
4902:
4901:
4900:
4890:
4889:
4888:
4883:
4878:
4873:
4863:
4862:
4861:
4856:
4851:
4846:
4841:
4836:
4826:
4825:
4824:
4819:
4814:
4809:
4804:
4799:
4794:
4789:
4784:
4779:
4769:
4768:
4767:
4762:
4757:
4752:
4747:
4737:
4736:
4735:
4730:
4720:
4719:
4718:
4713:
4704:
4702:
4696:
4695:
4693:
4692:
4691:
4690:
4685:
4680:
4675:
4670:
4665:
4660:
4655:
4650:
4640:
4639:
4638:
4637:
4636:
4631:
4621:
4620:
4619:
4614:
4599:
4598:
4597:
4592:
4587:
4582:
4571:
4569:
4552:
4549:
4548:
4546:
4545:
4538:
4531:
4524:
4517:
4510:
4503:
4496:
4489:
4484:
4479:
4474:
4469:
4462:
4457:
4452:
4447:
4442:
4394:
4391:
4390:
4385:
4383:
4382:
4375:
4368:
4360:
4351:
4350:
4348:
4347:
4342:
4337:
4331:
4329:
4325:
4324:
4322:
4321:
4316:
4311:
4309:Near-parabolic
4306:
4301:
4296:
4291:
4286:
4281:
4275:
4273:
4267:
4266:
4263:
4262:
4260:
4259:
4258:
4257:
4255:Scattered disc
4252:
4247:
4242:
4232:
4227:
4226:
4225:
4223:Neptune trojan
4220:
4212:
4210:
4204:
4203:
4201:
4200:
4198:Spectral types
4195:
4190:
4188:Jupiter trojan
4185:
4180:
4175:
4170:
4164:
4162:
4156:
4155:
4153:
4152:
4147:
4142:
4137:
4132:
4126:
4120:
4114:
4113:
4108:
4106:
4105:
4098:
4091:
4083:
4074:
4073:
4071:
4070:
4059:
4056:
4055:
4052:
4051:
4049:
4048:
4035:
4033:
4027:
4026:
4024:
4023:
4018:
4013:
4008:
4003:
3998:
3993:
3988:
3983:
3978:
3973:
3968:
3962:
3960:
3954:
3953:
3951:
3950:
3938:
3926:
3914:
3902:
3890:
3878:
3866:
3861:
3856:
3844:
3839:
3834:
3829:
3824:
3819:
3814:
3809:
3804:
3797:
3785:
3780:
3775:
3770:
3765:
3753:
3748:
3743:
3731:
3726:
3721:
3716:
3711:
3706:
3701:
3696:
3691:
3686:
3681:
3676:
3671:
3666:
3661:
3656:
3654:Gǃkúnǁʼhòmdímà
3650:
3648:
3646:Scattered disc
3642:
3641:
3639:
3638:
3633:
3628:
3623:
3618:
3613:
3608:
3603:
3598:
3593:
3588:
3576:
3571:
3566:
3561:
3556:
3551:
3546:
3541:
3536:
3531:
3526:
3521:
3515:
3513:
3509:
3508:
3506:
3505:
3493:
3488:
3483:
3478:
3473:
3468:
3463:
3458:
3453:
3448:
3443:
3438:
3433:
3428:
3423:
3418:
3413:
3408:
3403:
3398:
3393:
3388:
3383:
3371:
3366:
3361:
3356:
3351:
3346:
3341:
3336:
3330:
3328:
3322:
3321:
3319:
3318:
3313:
3307:
3305:
3299:
3298:
3296:
3295:
3283:
3278:
3273:
3268:
3263:
3258:
3253:
3248:
3243:
3238:
3233:
3228:
3223:
3218:
3213:
3208:
3202:
3200:
3194:
3193:
3191:
3190:
3185:
3180:
3175:
3170:
3165:
3160:
3155:
3150:
3144:
3142:
3136:
3135:
3133:
3132:
3127:
3121:
3119:
3110:
3106:
3105:
3092:
3090:
3088:
3087:
3080:
3079:
3078:
3066:
3065:
3064:
3052:
3051:
3050:
3045:
3033:
3032:
3031:
3019:
3018:
3017:
3012:
3000:
2999:
2998:
2993:
2988:
2976:
2975:
2974:
2962:
2961:
2960:
2955:
2942:
2940:
2936:
2935:
2933:
2932:
2927:
2922:
2921:
2920:
2915:
2910:
2905:
2897:
2891:
2888:
2887:
2882:
2880:
2879:
2872:
2865:
2857:
2846:
2845:
2842:on 2020-05-03.
2825:10.1086/338692
2783:
2732:
2719:10.1086/499336
2665:
2658:
2623:
2610:10.1086/339975
2586:(5): 2862–83.
2570:
2557:10.1086/452638
2514:
2486:
2451:
2401:
2345:
2310:10.1086/312467
2271:(2000-02-01).
2255:
2208:
2197:
2190:
2148:
2134:10.1086/427395
2094:
2027:
1960:
1947:10.1086/424617
1912:
1908:
1899:
1880:(2): 589–601.
1861:
1854:
1828:
1803:
1765:
1743:
1722:
1692:
1683:
1621:
1614:
1585:
1579:10.1086/320385
1544:
1507:
1471:
1437:
1430:
1393:
1375:(2007-11-08).
1364:
1343:
1322:
1299:
1272:
1265:
1247:
1229:
1201:
1188:
1162:
1098:
1077:
1052:
1013:(3): 798–810.
993:
986:
968:
944:
918:
917:
915:
912:
909:
908:
897:
896:
894:
891:
890:
889:
884:
877:
874:
866:Halley's Comet
829:Main article:
826:
823:
781:
778:
714:
711:
669:
666:
630:scattered-near
539:Main article:
536:
533:
504:
449:
446:
418:Main article:
415:
412:
385:
375:Gǃkúnǁʼhòmdímà
361:
353:
346:
339:
323:
314:digital images
283:
280:
235:by the planet
185:scattered disk
181:scattered disc
175:
174:
172:
171:
164:
157:
149:
146:
145:
144:
143:
142:
141:
135:
134:
133:
132:
131:
116:
115:
114:
103:
102:
101:
100:
99:
93:
82:
79:Classical KBOs
64:
59:
26:
24:
14:
13:
10:
9:
6:
4:
3:
2:
6194:
6183:
6180:
6178:
6175:
6173:
6170:
6168:
6165:
6164:
6162:
6155:
6150:
6140:
6138:
6128:
6126:
6116:
6114:
6104:
6100:
6089:
6080:
6073:
6066:
6059:
6053:
6047:
6041:
6034:
6027:
6020:
6013:
6006:
5999:
5992:
5986:
5976:
5974:
5964:
5962:
5952:
5950:
5947:
5946:
5943:
5928:
5927:Tidal locking
5925:
5923:
5920:
5918:
5915:
5913:
5910:
5908:
5907:Double planet
5905:
5904:
5902:
5898:
5892:
5889:
5885:
5882:
5880:
5877:
5876:
5875:
5872:
5870:
5867:
5865:
5862:
5860:
5859:Minor planets
5857:
5855:
5852:
5850:
5847:
5845:
5842:
5841:
5839:
5835:
5829:
5826:
5824:
5821:
5817:
5814:
5813:
5812:
5809:
5807:
5804:
5800:
5797:
5793:
5792:Merging stars
5790:
5789:
5788:
5785:
5783:
5780:
5778:
5775:
5773:
5770:
5768:
5765:
5764:
5763:
5760:
5758:
5755:
5753:
5750:
5748:
5745:
5743:
5740:
5738:
5735:
5733:
5730:
5728:
5725:
5723:
5720:
5718:
5715:
5713:
5710:
5708:
5705:
5703:
5700:
5698:
5695:
5693:
5690:
5688:
5685:
5683:
5680:
5676:
5673:
5671:
5668:
5667:
5666:
5663:
5661:
5658:
5656:
5653:
5651:
5648:
5646:
5643:
5641:
5638:
5636:
5633:
5631:
5628:
5626:
5623:
5621:
5618:
5614:
5611:
5610:
5609:
5606:
5604:
5601:
5599:
5596:
5595:
5593:
5591:
5585:
5579:
5576:
5574:
5571:
5569:
5566:
5564:
5561:
5559:
5556:
5554:
5551:
5549:
5546:
5542:
5539:
5538:
5537:
5534:
5532:
5529:
5527:
5524:
5520:
5517:
5516:
5515:
5512:
5510:
5507:
5505:
5502:
5498:
5495:
5493:
5490:
5488:
5485:
5484:
5483:
5480:
5476:
5473:
5471:
5468:
5467:
5466:
5463:
5459:
5456:
5454:
5451:
5449:
5446:
5445:
5444:
5441:
5439:
5436:
5435:
5433:
5430:
5425:
5421:
5415:
5412:
5410:
5407:
5405:
5402:
5400:
5397:
5395:
5394:Subsatellites
5392:
5390:
5387:
5385:
5382:
5380:
5377:
5375:
5372:
5370:
5367:
5365:
5362:
5361:
5359:
5357:
5354:Hypothetical
5351:
5348:
5339:
5336:
5332:
5329:
5327:
5324:
5322:
5319:
5317:
5314:
5310:
5307:
5305:
5302:
5301:
5300:
5297:
5296:
5295:
5292:
5288:
5285:
5283:
5280:
5279:
5278:
5275:
5271:
5268:
5266:
5263:
5261:
5258:
5256:
5253:
5251:
5248:
5246:
5243:
5241:
5238:
5236:
5233:
5231:
5228:
5227:
5226:
5223:
5221:
5220:Asteroid belt
5218:
5216:
5213:
5209:
5206:
5204:
5201:
5199:
5196:
5192:
5189:
5187:
5184:
5183:
5182:
5179:
5177:
5174:
5172:
5169:
5167:
5164:
5163:
5162:
5159:
5155:
5152:
5150:
5147:
5145:
5142:
5140:
5137:
5135:
5132:
5130:
5127:
5125:
5122:
5120:
5117:
5116:
5114:
5112:
5109:
5105:
5102:
5100:
5097:
5096:
5095:
5094:Minor planets
5092:
5090:
5087:
5085:
5082:
5080:
5077:
5076:
5074:
5072:
5062:
5056:
5053:
5051:
5048:
5046:
5043:
5041:
5038:
5036:
5033:
5031:
5028:
5025:
5021:
5018:
5016:
5013:
5012:
5010:
5008:
5004:
4996:
4993:
4992:
4991:
4988:
4984:
4981:
4980:
4979:
4976:
4972:
4969:
4968:
4967:
4964:
4960:
4957:
4956:
4955:
4952:
4948:
4945:
4943:
4940:
4939:
4938:
4935:
4931:
4928:
4926:
4923:
4921:
4918:
4916:
4913:
4911:
4908:
4907:
4906:
4903:
4899:
4896:
4895:
4894:
4891:
4887:
4884:
4882:
4879:
4877:
4874:
4872:
4869:
4868:
4867:
4864:
4860:
4857:
4855:
4852:
4850:
4847:
4845:
4842:
4840:
4837:
4835:
4832:
4831:
4830:
4827:
4823:
4820:
4818:
4815:
4813:
4810:
4808:
4805:
4803:
4800:
4798:
4795:
4793:
4790:
4788:
4785:
4783:
4780:
4778:
4775:
4774:
4773:
4770:
4766:
4763:
4761:
4758:
4756:
4753:
4751:
4748:
4746:
4743:
4742:
4741:
4738:
4734:
4731:
4729:
4726:
4725:
4724:
4721:
4717:
4714:
4712:
4709:
4708:
4706:
4705:
4703:
4701:
4697:
4689:
4686:
4684:
4681:
4679:
4676:
4674:
4671:
4669:
4666:
4664:
4661:
4659:
4656:
4654:
4651:
4649:
4646:
4645:
4644:
4641:
4635:
4632:
4630:
4627:
4626:
4625:
4622:
4618:
4615:
4613:
4610:
4609:
4608:
4605:
4604:
4603:
4600:
4596:
4593:
4591:
4588:
4586:
4583:
4581:
4578:
4577:
4576:
4573:
4572:
4570:
4568:
4563:
4559:
4556:
4555:
4550:
4544:
4543:
4539:
4537:
4536:
4532:
4530:
4529:
4525:
4523:
4522:
4518:
4516:
4515:
4511:
4509:
4508:
4504:
4502:
4501:
4497:
4495:
4494:
4490:
4488:
4485:
4483:
4480:
4478:
4475:
4473:
4470:
4468:
4467:
4463:
4461:
4458:
4456:
4453:
4451:
4448:
4446:
4443:
4441:
4438:
4437:
4392:
4388:
4381:
4376:
4374:
4369:
4367:
4362:
4361:
4358:
4346:
4343:
4341:
4338:
4336:
4333:
4332:
4330:
4326:
4320:
4317:
4315:
4312:
4310:
4307:
4305:
4302:
4300:
4297:
4295:
4292:
4290:
4287:
4285:
4282:
4280:
4277:
4276:
4274:
4272:
4268:
4256:
4253:
4251:
4248:
4246:
4243:
4241:
4238:
4237:
4236:
4233:
4231:
4228:
4224:
4221:
4219:
4216:
4215:
4214:
4213:
4211:
4209:
4205:
4199:
4196:
4194:
4191:
4189:
4186:
4184:
4181:
4179:
4178:Asteroid belt
4176:
4174:
4173:Aten asteroid
4171:
4169:
4166:
4165:
4163:
4161:
4157:
4151:
4148:
4146:
4143:
4141:
4138:
4136:
4133:
4131:
4128:
4127:
4124:
4121:
4119:
4118:Minor planets
4115:
4111:
4104:
4099:
4097:
4092:
4090:
4085:
4084:
4081:
4069:
4061:
4060:
4057:
4046:
4037:
4036:
4034:
4032:
4028:
4021:
4014:
4011:
4004:
4001:
3994:
3991:
3984:
3981:
3974:
3971:
3964:
3963:
3961:
3959:
3955:
3948:
3939:
3936:
3927:
3924:
3915:
3912:
3903:
3900:
3891:
3888:
3879:
3876:
3867:
3864:
3857:
3854:
3845:
3842:
3835:
3832:
3825:
3822:
3815:
3812:
3805:
3802:
3798:
3795:
3786:
3783:
3776:
3773:
3766:
3763:
3754:
3751:
3744:
3741:
3732:
3729:
3722:
3719:
3712:
3709:
3702:
3699:
3692:
3689:
3682:
3679:
3672:
3669:
3662:
3660:
3657:
3655:
3652:
3651:
3649:
3647:
3643:
3636:
3629:
3626:
3619:
3616:
3609:
3606:
3599:
3596:
3589:
3586:
3577:
3574:
3567:
3564:
3557:
3554:
3547:
3544:
3537:
3534:
3527:
3524:
3517:
3516:
3514:
3510:
3503:
3494:
3491:
3484:
3481:
3474:
3471:
3464:
3461:
3454:
3451:
3444:
3441:
3434:
3431:
3424:
3421:
3414:
3411:
3404:
3401:
3394:
3391:
3384:
3381:
3372:
3369:
3362:
3359:
3352:
3350:
3347:
3345:
3342:
3340:
3337:
3335:
3332:
3331:
3329:
3327:
3323:
3316:
3309:
3308:
3306:
3304:
3300:
3293:
3284:
3281:
3274:
3271:
3264:
3261:
3254:
3251:
3244:
3241:
3234:
3231:
3224:
3221:
3214:
3212:
3209:
3207:
3204:
3203:
3201:
3199:
3195:
3188:
3181:
3178:
3171:
3168:
3161:
3159:
3156:
3154:
3151:
3149:
3146:
3145:
3143:
3141:
3137:
3131:
3128:
3126:
3123:
3122:
3120:
3118:
3117:Asteroid belt
3114:
3111:
3107:
3102:
3096:
3086:
3085:
3081:
3077:
3074:
3073:
3072:
3071:
3067:
3063:
3060:
3059:
3058:
3057:
3053:
3049:
3046:
3044:
3041:
3040:
3039:
3038:
3034:
3030:
3027:
3026:
3025:
3024:
3020:
3016:
3013:
3011:
3008:
3007:
3006:
3005:
3001:
2997:
2994:
2992:
2989:
2987:
2984:
2983:
2982:
2981:
2977:
2973:
2970:
2969:
2968:
2967:
2963:
2959:
2956:
2954:
2951:
2950:
2949:
2948:
2944:
2943:
2941:
2937:
2931:
2928:
2926:
2923:
2919:
2916:
2914:
2911:
2909:
2906:
2904:
2901:
2900:
2898:
2896:
2893:
2892:
2889:
2885:
2884:Dwarf planets
2878:
2873:
2871:
2866:
2864:
2859:
2858:
2855:
2851:
2838:
2834:
2830:
2826:
2822:
2818:
2814:
2810:
2806:
2799:
2792:
2790:
2788:
2784:
2779:
2775:
2771:
2767:
2763:
2759:
2755:
2751:
2747:
2743:
2736:
2733:
2728:
2724:
2720:
2716:
2712:
2708:
2703:
2698:
2694:
2690:
2686:
2682:
2678:
2672:
2670:
2666:
2661:
2655:
2651:
2647:
2643:
2636:
2634:
2632:
2630:
2628:
2624:
2619:
2615:
2611:
2607:
2603:
2599:
2594:
2589:
2585:
2581:
2574:
2571:
2566:
2562:
2558:
2554:
2550:
2546:
2541:
2536:
2532:
2528:
2521:
2519:
2515:
2504:
2500:
2493:
2491:
2487:
2482:
2478:
2474:
2470:
2466:
2462:
2455:
2452:
2447:
2443:
2439:
2435:
2431:
2427:
2423:
2419:
2415:
2408:
2406:
2402:
2397:
2393:
2389:
2385:
2381:
2377:
2373:
2369:
2365:
2361:
2360:
2355:
2349:
2346:
2331:
2327:
2323:
2319:
2315:
2311:
2307:
2303:
2299:
2294:
2289:
2285:
2281:
2274:
2270:
2266:
2259:
2256:
2251:
2247:
2243:
2239:
2235:
2231:
2227:
2223:
2219:
2215:
2201:
2198:
2193:
2187:
2183:
2179:
2175:
2171:
2167:
2161:
2159:
2157:
2155:
2153:
2149:
2144:
2140:
2135:
2130:
2126:
2122:
2118:
2114:
2110:
2103:
2101:
2099:
2095:
2090:
2086:
2082:
2078:
2073:
2068:
2064:
2060:
2055:
2050:
2046:
2042:
2038:
2031:
2028:
2023:
2019:
2015:
2011:
2006:
2001:
1997:
1993:
1988:
1983:
1979:
1975:
1971:
1964:
1961:
1956:
1952:
1948:
1944:
1940:
1936:
1931:
1926:
1922:
1918:
1903:
1900:
1895:
1891:
1887:
1883:
1879:
1875:
1868:
1866:
1862:
1857:
1851:
1844:
1843:
1838:
1832:
1829:
1818:
1814:
1807:
1804:
1799:
1795:
1791:
1787:
1783:
1779:
1772:
1770:
1766:
1754:
1747:
1744:
1733:
1726:
1723:
1711:
1707:
1703:
1696:
1693:
1687:
1684:
1679:
1675:
1670:
1665:
1661:
1657:
1652:
1647:
1643:
1639:
1635:
1628:
1626:
1622:
1617:
1611:
1607:
1603:
1599:
1592:
1590:
1586:
1580:
1575:
1571:
1567:
1563:
1559:
1555:
1548:
1545:
1534:
1527:
1520:
1518:
1516:
1514:
1512:
1508:
1503:
1497:
1482:
1478:
1474:
1468:
1464:
1457:
1450:
1448:
1446:
1444:
1442:
1438:
1433:
1427:
1423:
1419:
1418:
1413:
1406:
1404:
1402:
1400:
1398:
1394:
1383:on 2010-08-18
1382:
1378:
1374:
1373:Buie, Marc W.
1368:
1365:
1353:
1347:
1344:
1332:
1326:
1323:
1318:
1314:
1310:
1303:
1300:
1288:
1281:
1279:
1277:
1273:
1268:
1262:
1258:
1250:
1244:
1240:
1233:
1230:
1218:
1214:
1208:
1206:
1202:
1191:
1185:
1181:
1176:
1175:
1166:
1163:
1148:
1144:
1140:
1136:
1135:10.1038/42413
1132:
1128:
1124:
1120:
1116:
1109:
1102:
1099:
1088:on 2006-10-12
1084:
1080:
1078:1-58381-220-2
1074:
1070:
1063:
1056:
1053:
1048:
1044:
1039:
1034:
1030:
1026:
1021:
1016:
1012:
1008:
1004:
997:
994:
989:
983:
979:
972:
969:
963:
958:
951:
949:
945:
934:
930:
923:
920:
913:
902:
899:
892:
888:
885:
883:
880:
879:
875:
873:
869:
867:
863:
859:
854:
852:
845:
841:
837:
832:
824:
822:
820:
816:
810:
807:
801:
799:
795:
786:
779:
777:
774:
769:
765:
760:
756:
754:
750:
749:outer planets
746:
742:
738:
733:
725:
720:
712:
710:
706:
704:
699:
696:
691:
689:
680:
674:
667:
665:
663:
659:
654:
653:B. G. Marsden
650:
649:B. J. Gladman
645:
643:
639:
635:
631:
626:
624:
618:
616:
612:
608:
603:
593:
589:
585:
581:
576:
565:
562:
558:
554:
548:
542:
534:
532:
530:
526:
520:
516:
514:
510:
501:
497:
491:
489:
485:
481:
477:
473:
469:
465:
461:
455:
447:
445:
443:
439:
431:
426:
421:
413:
411:
409:
405:
401:
397:
393:
388:
380:
376:
371:
369:
364:
335:
331:
326:
317:
315:
311:
307:
303:
299:
295:
289:
281:
279:
277:
273:
269:
265:
261:
256:
254:
250:
246:
240:
238:
234:
230:
218:
214:
210:
206:
202:
198:
194:
190:
186:
182:
170:
165:
163:
158:
156:
151:
150:
148:
147:
139:
136:
130:
127:
126:
125:
122:
121:
120:
117:
113:
112:Resonant SDOs
110:
109:
107:
104:
97:
94:
91:
88:
87:
86:
85:Resonant KBOs
83:
80:
77:
76:
74:
71:
70:
68:
65:
63:
60:
58:
55:
54:
53:
52:
49:
40:
36:
32:
19:
6167:Solar System
6154:
6149:Solar system
6083:Each arrow (
6005:Local Bubble
5991:Solar System
5989:
5827:
5782:Planetesimal
5737:Kuiper cliff
5465:Space probes
5438:Colonization
5325:
5277:Kirkwood gap
5198:Saturn Moons
5111:Planetesimal
4575:Terrestrials
4540:
4533:
4526:
4519:
4512:
4505:
4498:
4491:
4464:
4387:Solar System
4345:Space debris
4254:
3645:
3082:
3068:
3054:
3035:
3021:
3002:
2978:
2964:
2945:
2849:
2837:the original
2808:
2804:
2745:
2741:
2735:
2692:
2688:
2645:
2583:
2579:
2573:
2530:
2526:
2506:. Retrieved
2502:
2467:(1): 13–32.
2464:
2460:
2454:
2421:
2417:
2363:
2357:
2348:
2337:. Retrieved
2330:the original
2283:
2279:
2269:Luu, Jane X.
2258:
2217:
2213:
2200:
2173:
2116:
2112:
2044:
2040:
2030:
1977:
1973:
1963:
1920:
1916:
1902:
1877:
1873:
1841:
1831:
1820:. Retrieved
1816:
1806:
1781:
1777:
1757:. Retrieved
1746:
1735:. Retrieved
1725:
1714:. Retrieved
1710:the original
1705:
1695:
1686:
1641:
1637:
1601:
1561:
1557:
1547:
1536:. Retrieved
1532:
1485:. Retrieved
1462:
1416:
1385:. Retrieved
1381:the original
1367:
1356:. Retrieved
1346:
1335:. Retrieved
1325:
1308:
1302:
1291:. Retrieved
1256:
1238:
1232:
1221:. Retrieved
1193:. Retrieved
1173:
1165:
1154:. Retrieved
1147:the original
1118:
1114:
1101:
1090:. Retrieved
1083:the original
1068:
1055:
1010:
1006:
996:
977:
971:
936:. Retrieved
932:
922:
901:
870:
855:
848:
811:
802:
791:
767:
761:
757:
734:
731:
707:
700:
692:
684:
662:detached TNO
661:
657:
646:
633:
629:
627:
619:
614:
610:
606:
591:
587:
566:
550:
528:
521:
517:
492:
466:(KBOs): the
457:
435:
430:5:2 resonant
372:
318:
291:
257:
241:
233:perturbation
209:inclinations
193:Solar System
184:
180:
178:
105:
6137:Outer space
6125:Spaceflight
6046:Local Sheet
6040:Local Group
5823:Rubble pile
5811:Roche limit
5806:Ring system
5757:Outer space
5732:Kuiper belt
5702:Hill sphere
5697:Hills cloud
5645:Debris disk
5640:Cosmic dust
5424:Exploration
5379:Planet Nine
5364:Fifth giant
5338:Hills cloud
5299:Kuiper belt
5270:exceptional
5186:Trojan camp
4335:Cosmic dust
4299:Long-period
4289:Halley-type
4245:Kuiper belt
4130:Designation
1911:and 2003 VB
860:(JFCs) and
780:Composition
737:Kuiper belt
553:90377 Sedna
525:Hill sphere
482:", because
454:Kuiper belt
330:astronomers
249:Kuiper belt
81:(cubewanos)
6161:Categories
6065:Local Hole
6012:Gould Belt
5752:Oort cloud
5588:Formation,
5578:Deep space
5414:Vulcanoids
5331:Oort cloud
5255:first 1000
5191:Greek camp
5089:Meteoroids
5084:Damocloids
5030:Charikloan
4340:Meteoroids
4319:Sungrazing
4294:Hyperbolic
4250:Oort cloud
4193:Near-Earth
3512:Other KBOs
3130:Interamnia
2991:Atmosphere
2958:Atmosphere
2925:Mesoplanet
2508:2007-08-26
2339:2008-07-02
2054:1506.03105
1987:1807.02960
1822:2008-08-02
1759:2008-07-02
1737:2010-01-23
1716:2008-08-12
1538:2008-08-10
1487:2008-07-27
1387:2008-07-17
1358:2010-10-25
1337:2010-10-25
1293:2011-01-03
1223:2010-01-23
1195:2008-07-02
1156:2008-08-02
1092:2008-08-14
938:2008-07-12
914:References
717:See also:
607:"detached"
561:perihelion
545:See also:
500:planetoids
452:See also:
438:Oort cloud
368:Spacewatch
306:telescopes
286:See also:
268:Oort cloud
229:gas giants
140:(ICO/OCOs)
6113:Astronomy
6026:Milky Way
6019:Orion Arm
5787:Formation
5772:Migration
5767:Disrupted
5635:Coatlicue
5603:Accretion
5590:evolution
5536:Asteroids
5448:astronomy
5443:Discovery
5304:Cubewanos
5225:Asteroids
5055:Quaoarian
5045:Neptunian
5035:Chironean
5020:Saturnian
4802:Enceladus
4230:Damocloid
3659:Dziewanna
3326:Cubewanos
3109:Candidate
2939:Consensus
2833:122240711
2089:119188358
2081:0035-8711
2022:119197960
2014:1538-4357
1980:(1): 45.
1955:119486916
1706:space.com
1496:cite book
1463:Comets II
1253:Also see
794:volatiles
753:migration
741:eccentric
713:Formation
703:cubewanos
334:Mauna Kea
332:based at
310:digitized
282:Discovery
213:perihelia
46:Types of
6079:Universe
5917:Moonlets
5497:programs
5470:timeline
5458:timeline
5389:Planet X
5384:Planet V
5321:Sednoids
5309:Plutinos
5282:Centaurs
5260:families
4995:Dysnomia
4983:Xiangliu
4978:Gonggong
4966:Makemake
4925:Kerberos
4812:Hyperion
4750:Callisto
4745:Ganymede
4678:Gonggong
4673:Makemake
4528:Gonggong
4521:Makemake
4314:Periodic
4240:Detached
4160:Asteroid
4068:Category
4031:Sednoids
3303:Twotinos
3198:Plutinos
3148:Chariklo
3140:Centaurs
3070:Gonggong
3023:Makemake
2778:33160822
2770:15637267
2618:17510705
2565:14153557
2503:Geotimes
2388:14647375
2318:10622765
2242:16452973
2143:19385887
1481:56755773
1047:16002759
876:See also
840:Tempel 1
745:inclined
688:ecliptic
679:sednoids
496:centaurs
488:twotinos
480:plutinos
379:Gonggong
264:centaurs
253:ecliptic
129:Sednoids
96:Twotinos
90:Plutinos
57:Centaurs
39:Dysnomia
6099:Portals
5900:Related
5879:by size
5568:Neptune
5553:Jupiter
5504:Mercury
5429:outline
5374:Phaeton
5369:Nemesis
5356:objects
5208:Neptune
5181:Jupiter
5161:Trojans
5154:Neptune
5139:Jupiter
5119:Mercury
5050:Haumean
5040:Uranian
5022: (
4942:Hiʻiaka
4876:Proteus
4866:Neptune
4854:Miranda
4844:Umbriel
4834:Titania
4822:all 146
4787:Iapetus
4740:Jupiter
4634:Neptune
4612:Jupiter
4580:Mercury
4562:Planets
4487:Neptune
4472:Jupiter
4445:Mercury
4279:Extinct
4218:Centaur
4040:2012 VP
4017:2008 ST
4007:2007 JJ
3997:2005 TB
3987:2004 XR
3977:2003 QX
3967:2003 FY
3942:2021 LL
3930:2021 DR
3918:2018 VG
3906:2018 AG
3894:2017 FO
3882:2015 RR
3870:2015 KH
3860:2014 WK
3848:2014 UZ
3838:2014 EZ
3828:2014 AN
3818:2013 FY
3808:2010 VZ
3801:2010 TJ
3789:2010 JO
3779:2010 RF
3769:2010 RE
3757:2010 KZ
3747:2008 OG
3735:2006 QH
3725:2005 RM
3715:2005 QU
3705:2004 XA
3695:2002 TC
3685:2001 UR
3675:1996 TL
3665:1996 GQ
3632:2015 RR
3622:2015 AM
3612:2014 UM
3602:2013 FZ
3592:2011 GM
3580:2011 FW
3570:2010 VK
3560:2010 JO
3550:2002 XW
3540:2000 YW
3530:1999 DE
3520:1999 CD
3497:2010 FX
3487:2005 UQ
3477:2005 RN
3467:2004 UX
3457:2004 TY
3447:2004 PF
3437:2004 NT
3427:2004 GV
3417:2003 QW
3407:2002 UX
3397:2002 MS
3387:2002 KX
3375:2002 CY
3365:2002 AW
3355:1998 SN
3339:Salacia
3312:2002 WC
3287:2017 OF
3277:2007 JH
3267:2003 VS
3257:2003 UZ
3247:2003 AZ
3237:2002 XV
3227:2002 VR
3217:2001 QF
3184:2014 NW
3174:2013 TC
3164:1999 OX
2986:Geology
2953:Geology
2930:Planemo
2813:Bibcode
2750:Bibcode
2742:Science
2727:1761936
2707:Bibcode
2650:605–620
2598:Bibcode
2545:Bibcode
2469:Bibcode
2446:9180070
2426:Bibcode
2418:Science
2396:4395099
2368:Bibcode
2326:8240136
2298:Bibcode
2250:4369483
2222:Bibcode
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2121:Bibcode
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1992:Bibcode
1935:Bibcode
1882:Bibcode
1786:Bibcode
1678:2822011
1656:Bibcode
1606:589–604
1566:Bibcode
1422:575–588
1313:Bibcode
1143:4370529
1123:Bibcode
1025:Bibcode
806:tholins
798:methane
768:in situ
755:epoch.
728:Jupiter
597:2000 CR
584:Neptune
547:Sednoid
384:2002 TC
360:1995 TL
352:1999 CF
345:1999 CY
338:1999 CV
322:1996 TL
237:Neptune
191:in the
108:(SDOs)
75:(KBOs)
69:(TNOs)
6074:
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5922:Syzygy
5844:Comets
5777:System
5762:Planet
5655:EXCEDE
5563:Uranus
5558:Saturn
5548:Comets
5541:mining
5519:mining
5409:Vulcan
5250:active
5245:Hygiea
5240:Pallas
5203:Uranus
5149:Uranus
5144:Saturn
5079:Comets
5071:bodies
5069:System
5015:Jovian
4959:Weywot
4954:Quaoar
4947:Namaka
4937:Haumea
4910:Charon
4886:all 16
4881:Nereid
4871:Triton
4859:all 28
4839:Oberon
4829:Uranus
4817:Phoebe
4797:Tethys
4772:Saturn
4765:all 95
4760:Europa
4733:Deimos
4728:Phobos
4707:Earth
4668:Quaoar
4663:Haumea
4643:Dwarfs
4629:Uranus
4617:Saturn
4602:Giants
4567:dwarfs
4514:Quaoar
4507:Haumea
4482:Uranus
4477:Saturn
4271:Comets
4183:Family
4168:Active
4135:Groups
3349:Varuna
3158:Pholus
3153:Chiron
3125:Hygiea
3037:Quaoar
3004:Haumea
2918:Pallas
2908:Triton
2903:Phoebe
2831:
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2461:Icarus
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1874:Icarus
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1115:Nature
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825:Comets
819:tholin
815:albedo
764:Uranus
668:Orbits
350:, and
5837:Lists
5573:Pluto
5531:Ceres
5509:Venus
5404:Tyche
5399:Theia
5235:Vesta
5230:Ceres
5171:Earth
5166:Venus
5129:Earth
5124:Venus
5104:moons
5067:Solar
5065:Small
5024:Rhean
5007:Rings
4920:Hydra
4905:Pluto
4898:Vanth
4893:Orcus
4849:Ariel
4807:Mimas
4792:Dione
4777:Titan
4700:Moons
4688:Sedna
4658:Pluto
4653:Orcus
4648:Ceres
4590:Earth
4585:Venus
4542:Sedna
4500:Pluto
4493:Orcus
4466:Ceres
4455:Earth
4450:Venus
4328:Other
4284:Great
3344:Varda
3334:Chaos
3211:Ixion
3084:Sedna
3048:Rings
3010:Moons
2996:Moons
2980:Pluto
2966:Orcus
2947:Ceres
2913:Vesta
2840:(PDF)
2829:S2CID
2801:(PDF)
2774:S2CID
2723:S2CID
2697:arXiv
2614:S2CID
2588:arXiv
2561:S2CID
2535:arXiv
2392:S2CID
2333:(PDF)
2322:S2CID
2288:arXiv
2276:(PDF)
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2139:S2CID
2085:S2CID
2049:arXiv
2018:S2CID
1982:arXiv
1951:S2CID
1925:arXiv
1846:(PDF)
1674:S2CID
1646:arXiv
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1459:(PDF)
1150:(PDF)
1139:S2CID
1111:(PDF)
1086:(PDF)
1065:(PDF)
1043:S2CID
1015:arXiv
957:arXiv
893:Notes
609:, or
592:E-SDO
484:Pluto
460:torus
400:Sedna
276:Sedna
245:torus
5526:Mars
5514:Moon
5492:list
5475:list
5176:Mars
5134:Mars
4990:Eris
4930:Styx
4782:Rhea
4723:Mars
4711:Moon
4683:Eris
4595:Mars
4535:Eris
4460:Mars
4304:Lost
4145:Moon
4140:List
3206:Huya
3076:Moon
3062:Moon
3056:Eris
3043:Moon
3029:Moon
3015:Ring
2972:Moon
2766:PMID
2654:ISBN
2442:PMID
2384:PMID
2314:PMID
2238:PMID
2186:ISBN
2077:ISSN
2010:ISSN
1850:ISBN
1610:ISBN
1502:link
1477:OCLC
1467:ISBN
1426:ISBN
1261:ISBN
1243:ISBN
1184:ISBN
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982:ISBN
842:, a
743:and
396:Eris
392:NEAT
219:(4.5
183:(or
179:The
35:Eris
5265:PHA
4915:Nix
4624:Ice
4607:Gas
4440:Sun
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3999:190
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