Damocloid asteroid - Biblioteka.sk

Upozornenie: Prezeranie týchto stránok je určené len pre návštevníkov nad 18 rokov!
Zásady ochrany osobných údajov.
Používaním tohto webu súhlasíte s uchovávaním cookies, ktoré slúžia na poskytovanie služieb, nastavenie reklám a analýzu návštevnosti. OK, súhlasím


Panta Rhei Doprava Zadarmo
...
...


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

Damocloid asteroid
 ...

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]

  • q < 5.2 AU, a > 8.0 AU, and e > 0.75,
  • or alternatively, i > 90°

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.[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 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.

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 Green tickY 1.59 22.11 LoMP MPC · JPL
(15504) 1999 RG33 9.37 0.774 35 CEN 1.948 Green tickY 2.12 16.63 unusual LoMP MPC · JPL
20461 Dioretsa 23.88 0.901 160.4 CEN Green tickY -1.534 Green tickY 2.37 45.39 unusual LoMP MPC · JPL
(65407) 2002 RP120 53.66 0.954 119.3 TNO Green tickY -0.844 Green tickY 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 Green tickY -1.397 Green tickY 3.56 12.69 unusual LoMP MPC · JPL
(336756) 2010 NV1 278.33 0.966 140.7 TNO Green tickY -2.903 Green tickY 9.42 547.23 LoMP MPC · JPL
(342842) 2008 YB3 11.58 0.442 105.1 CEN Green tickY -0.246 Green tickY 6.47 16.7 LoMP MPC · JPL
343158 Marsyas 2.53 0.807 154.4 NEO Green tickY 1.317 Green tickY 0.49 4.57 LoMP MPC · JPL
(434620) 2005 VD 6.67 0.251 172.9 CEN Green tickY -1.394 Green tickY 5 8.34 unusual LoMP MPC · JPL
(459870) 2014 AT28 10.9 0.401 165.5 CEN Green tickY -2.090 Green tickY 6.53 15.27 LoMP MPC · JPL
(468861) 2013 LU28 191.63 0.954 125.3 TNO Green tickY -2.069 Green tickY 8.74 374.53 LoMP MPC · JPL
(471325) 2011 KT19 35.7 0.33 110.2 TNO Green tickY -1.560 Green tickY 23.9 47.5 LoMP MPC · JPL
514107 Kaʻepaokaʻawela 5.13 0.378 163.1 other Green tickY -0.745 Green tickY 3.19 7.07 LoMP MPC · JPL
(518151) 2016 FH13 24.54 0.615 93.6 CEN Green tickY -0.005 Green tickY 9.45 39.62 LoMP MPC · JPL
(523797) 2016 NM56 71.46 0.853 144 TNO Green tickY -3.061 Green tickY 10.53 132.38 LoMP MPC · JPL
(523800) 2017 KZ31 54.3 0.798 161.7 TNO Green tickY -3.601 Green tickY 10.96 97.63 LoMP MPC · JPL
(528219) 2008 KV42 42.03 0.497 103.4 TNO Green tickY -1.021 Green tickY 21.15 62.92 LoMP MPC · JPL
(582301) 2015 RM306 246.87 0.954 176 TNO Green tickY -4.117 Green tickY 11.46 482.29 LoMP MPC · JPL
(585899) 2020 HM98 83.6 0.841 137.9 TNO Green tickY -3.151 Green tickY 13.26 153.94 LoMP MPC · JPL
(612093) 1999 LE31 8.17 0.468 151.5 CEN Green tickY -1.309 Green tickY 4.35 11.99 LoMP MPC · JPL
1996 PW 265.49 0.991 30.1 TNO 1.708 Green tickY 2.49 528.5 unusual MPC · JPL
1997 MD10 26.49 0.943 59.4 CEN 0.960 Green tickY 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 Green tickY 1.41 28.85 MPC · JPL
1999 XS35 17.77 0.948 19.5 NEO 1.405 Green tickY 0.93 34.62 MPC · JPL
2000 AB229 52.32 0.956 68.2 TNO 0.790 Green tickY 2.31 102.33 unusual MPC · JPL
2000 DG8 10.77 0.793 129.3 CEN Green tickY -0.627 Green tickY 2.23 19.31 unusual Zdroj:https://en.wikipedia.org?pojem=Damocloid_asteroid
Text je dostupný za podmienok Creative Commons Attribution/Share-Alike License 3.0 Unported; prípadne za ďalších podmienok. Podrobnejšie informácie nájdete na stránke Podmienky použitia.






Text je dostupný za podmienok Creative Commons Attribution/Share-Alike License 3.0 Unported; prípadne za ďalších podmienok.
Podrobnejšie informácie nájdete na stránke Podmienky použitia.

Your browser doesn’t support the object tag.

www.astronomia.sk | www.biologia.sk | www.botanika.sk | www.dejiny.sk | www.economy.sk | www.elektrotechnika.sk | www.estetika.sk | www.farmakologia.sk | www.filozofia.sk | Fyzika | www.futurologia.sk | www.genetika.sk | www.chemia.sk | www.lingvistika.sk | www.politologia.sk | www.psychologia.sk | www.sexuologia.sk | www.sociologia.sk | www.veda.sk I www.zoologia.sk