A | B | C | D | E | F | G | H | CH | I | J | K | L | M | N | O | P | Q | R | S | T | U | V | W | X | Y | Z | 0 | 1 | 2 | 3 | 4 | 5 | 6 | 7 | 8 | 9
Damocloids are a class of minor planets such as 5335 Damocles and 1996 PW that have Halley-type or long-period highly eccentric orbits typical of periodic comets such as Halley's Comet, but without showing a cometary coma or tail. David Jewitt defines a damocloid as an object with a Jupiter Tisserand invariant (TJ) of 2 or less,[1][a] while Akimasa Nakamura defines this group with the following orbital elements:[2]
However, this definition that does not focus on Jupiter excludes objects such as (127546) 2002 XU93, 2003 WG166, and 2004 DA62.[3]
Using the Tisserand's parameter with respect to Jupiter of 2 or less, there are currently 220 damocloid candidates as of January 2022[update].[4] Of these objects, 189 have orbital observation arcs greater than 30 days providing reasonably decent orbits.[1][5] Their average radius is eight kilometers assuming an albedo of 0.04. The albedos of four damocloids have been measured, and they are among the darkest objects known in the Solar System.[citation needed] Damocloids are reddish in color, but not as red as many Kuiper-belt objects or centaurs. Other damocloids include: 2013 BL76, 2012 DR30, (528219) 2008 KV42, (65407) 2002 RP120, and 20461 Dioretsa.
Retrograde objects such as Halley's Comet and damocloid 343158 Marsyas can have relative velocities to Earth of 81 km/s (290,000 km/h).[6]
Origin
Damocloids are thought to be nuclei of Halley-type comets that have lost all their volatile materials due to outgassing and become dormant. Such comets probably originate from the Oort cloud. This hypothesis is strengthened by the fact that a number of objects thought to be damocloids (and assigned minor-planet provisional designations) subsequently showed a coma and were confirmed to be comets: C/2001 OG108 (LONEOS), C/2002 CE10 (LINEAR), C/2002 VQ94 (LINEAR), C/2004 HV60 (Spacewatch) and possibly others. Another strong indication of cometary origin is the fact that some damocloids have retrograde orbits, unlike any other minor planets. (Objects with an inclination beyond 90 degrees up to 180 degrees are in a retrograde orbit and orbit in the opposite direction of other objects.)
List
As of August 2021[update] this list from the JPL SBDB contains 20 numbered and 268 unnumbered bodies that meet Akimasa Nakamura's criteria for being classified as a damocloid, that is, either a retrograde orbit, or the following orbital elements: q < 5.2 AU, a > 8.0 AU, and e > 0.75
(also see § top). Tisserand's parameter with respect to Jupiter (TJupiter) is also given.[a] Akimasa Nakamura's criteria and a TJupiter of less than two are largely equivalent as only a few listed bodies do not meet the defined TJupiter threshold. Most damocloids are also listed on MPC's list of other unusual minor planets.[7] The orbital data is sourced from JPL-numbered and -unnumbered element files.[8] The list includes A/-designated objects (introduced in 2017) that were mistakenly identified as a comet, but are actually minor planets. However it excludes hyperbolic bodies such as A/2019 G4 as well as 1I/ʻOumuamua and 2I/Borisov, two interstellar objects.
![]() | This section needs to be updated.(October 2023) |
Designation | a (AU) |
e | i (°) |
Orbital criteria and classes | q (AU) |
Q (AU) |
Unusual | Catalog | Refs | |||
---|---|---|---|---|---|---|---|---|---|---|---|---|
Cls | Retro | TJupiter[a] | TJ ≤ 2 | |||||||||
5335 Damocles | 11.85 | 0.866 | 61.6 | CEN | — | 1.158 | ![]() |
1.59 | 22.11 | — | LoMP | MPC · JPL |
(15504) 1999 RG33 | 9.37 | 0.774 | 35 | CEN | — | 1.948 | ![]() |
2.12 | 16.63 | unusual | LoMP | MPC · JPL |
20461 Dioretsa | 23.88 | 0.901 | 160.4 | CEN | ![]() |
-1.534 | ![]() |
2.37 | 45.39 | unusual | LoMP | MPC · JPL |
(65407) 2002 RP120 | 53.66 | 0.954 | 119.3 | TNO | ![]() |
-0.844 | ![]() |
2.46 | 104.86 | unusual | LoMP | MPC · JPL |
(154783) 2004 PA44 | 14.23 | 0.76 | 3.3 | CEN | — | 2.513 | — | 3.42 | 25.04 | unusual | LoMP | MPC · JPL |
(330759) 2008 SO218 | 8.12 | 0.562 | 170.3 | CEN | ![]() |
-1.397 | ![]() |
3.56 | 12.69 | unusual | LoMP | MPC · JPL |
(336756) 2010 NV1 | 278.33 | 0.966 | 140.7 | TNO | ![]() |
-2.903 | ![]() |
9.42 | 547.23 | — | LoMP | MPC · JPL |
(342842) 2008 YB3 | 11.58 | 0.442 | 105.1 | CEN | ![]() |
-0.246 | ![]() |
6.47 | 16.7 | — | LoMP | MPC · JPL |
343158 Marsyas | 2.53 | 0.807 | 154.4 | NEO | ![]() |
1.317 | ![]() |
0.49 | 4.57 | — | LoMP | MPC · JPL |
(434620) 2005 VD | 6.67 | 0.251 | 172.9 | CEN | ![]() |
-1.394 | ![]() |
5 | 8.34 | unusual | LoMP | MPC · JPL |
(459870) 2014 AT28 | 10.9 | 0.401 | 165.5 | CEN | ![]() |
-2.090 | ![]() |
6.53 | 15.27 | — | LoMP | MPC · JPL |
(468861) 2013 LU28 | 191.63 | 0.954 | 125.3 | TNO | ![]() |
-2.069 | ![]() |
8.74 | 374.53 | — | LoMP | MPC · JPL |
(471325) 2011 KT19 | 35.7 | 0.33 | 110.2 | TNO | ![]() |
-1.560 | ![]() |
23.9 | 47.5 | — | LoMP | MPC · JPL |
514107 Kaʻepaokaʻawela | 5.13 | 0.378 | 163.1 | other | ![]() |
-0.745 | ![]() |
3.19 | 7.07 | — | LoMP | MPC · JPL |
(518151) 2016 FH13 | 24.54 | 0.615 | 93.6 | CEN | ![]() |
-0.005 | ![]() |
9.45 | 39.62 | — | LoMP | MPC · JPL |
(523797) 2016 NM56 | 71.46 | 0.853 | 144 | TNO | ![]() |
-3.061 | ![]() |
10.53 | 132.38 | — | LoMP | MPC · JPL |
(523800) 2017 KZ31 | 54.3 | 0.798 | 161.7 | TNO | ![]() |
-3.601 | ![]() |
10.96 | 97.63 | — | LoMP | MPC · JPL |
(528219) 2008 KV42 | 42.03 | 0.497 | 103.4 | TNO | ![]() |
-1.021 | ![]() |
21.15 | 62.92 | — | LoMP | MPC · JPL |
(582301) 2015 RM306 | 246.87 | 0.954 | 176 | TNO | ![]() |
-4.117 | ![]() |
11.46 | 482.29 | — | LoMP | MPC · JPL |
(585899) 2020 HM98 | 83.6 | 0.841 | 137.9 | TNO | ![]() |
-3.151 | ![]() |
13.26 | 153.94 | — | LoMP | MPC · JPL |
(612093) 1999 LE31 | 8.17 | 0.468 | 151.5 | CEN | ![]() |
-1.309 | ![]() |
4.35 | 11.99 | — | LoMP | MPC · JPL |
1996 PW | 265.49 | 0.991 | 30.1 | TNO | — | 1.708 | ![]() |
2.49 | 528.5 | unusual | — | MPC · JPL |
1997 MD10 | 26.49 | 0.943 | 59.4 | CEN | — | 0.960 | ![]() |
1.51 | 51.47 | — | — | MPC · JPL |
1998 QJ1 | 11.24 | 0.815 | 23.7 | CEN | — | 2.023 | — | 2.08 | 20.41 | unusual | — | MPC · JPL |
1998 WU24 | 15.13 | 0.907 | 42.5 | CEN | — | 1.404 | ![]() |
1.41 | 28.85 | — | — | MPC · JPL |
1999 XS35 | 17.77 | 0.948 | 19.5 | NEO | — | 1.405 | ![]() |
0.93 | 34.62 | — | — | MPC · JPL |
2000 AB229 | 52.32 | 0.956 | 68.2 | TNO | — | 0.790 | ![]() |
2.31 | 102.33 | unusual | — | MPC · JPL |
2000 DG8 | 10.77 | 0.793 | 129.3 | CEN | ![]() |
-0.627 | ![]() |
2.23 | 19.31 | unusual | —
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