From Surf Wiki (app.surf) — the open knowledge base
4015 Wilson–Harrington
Periodic comet with 4 year orbit
Periodic comet with 4 year orbit
| Field | Value |
|---|---|
| minorplanet | yes |
| background | #FFC2E0 |
| name | 4015 Wilson–Harrington |
| 107P/Wilson–Harrington | |
| image | 4015 Wilson–Harrington Eso9212b.jpg |
| caption | 4015 Wilson–Harrington at 19 November 1949, from the 48-inch Schmidt telescope at Palomar. The image was enhanced by ESO to show the tail. |
| discoverer | Albert G. Wilson and |
| Robert G. Harrington | |
| discovered | 19 November 1949 |
| mpc_name | (4015) Wilson–Harrington |
| alt_names | 107P/1949 W1 |
| 107P/1979 VA | |
| 1949 III1949g | |
| mp_category | NEOApolloComet |
| orbit_ref | |
| epoch | 2022-Aug-09 (JD 2459800.5) |
| observation_arc | 24241 days (66.37 yr) |
| uncertainty | 0 |
| semimajor | 2.6249 AU |
| perihelion | 0.96664 AU |
| time_periastron | 2026-Nov-25{{cite web |
| title | Horizons Batch for 4015 Wilson-Harrington (1979 VA) on 2026-Nov-25 |
| publisher | JPL Horizons |
| type | Perihelion occurs when rdot flips from negative to positive |
| url | https://ssd.jpl.nasa.gov/horizons_batch.cgi?batch=1&COMMAND=%27107P%27&START_TIME=%272026-Nov-25%27&STOP_TIME=%272026-Nov-26%27&STEP_SIZE=%273%20hours%27&QUANTITIES=%2719%27 |
| accessdate | 2023-04-29}} (JPL#321/Soln.date: 2023-Apr-19 |
| 2022-Aug-24 (previous) | |
| aphelion | 4.2833 AU |
| eccentricity | 0.63175 |
| period | 4.25 yr (1553.4 d) |
| inclination | 2.7992° |
| asc_node | 266.77° |
| arg_peri | 95.441° |
| mean_anomaly | 356.37° |
| moid | 0.045552 AU |
| tisserand | 3.080 |
| avg_speed | 16.39 km/s |
| dimensions | 4 km |
| rotation | 3.5736 h |
| spectral_type | (orange) |
| B−V=0.666 | |
| U−B=0.279 | |
| abs_magnitude | 15.99 |
| albedo | 0.05 ± 0.01 |
| magnitude | ~11 (1979) |
| 16 (2009) | |
| mean_motion | / day |
| mean_radius | 2 ± 0.25 km |
107P/Wilson–Harrington Robert G. Harrington 107P/1979 VA 1949 III1949g 2022-Aug-24 (previous) B−V=0.666 U−B=0.279 16 (2009)
4015 Wilson–Harrington is an active asteroid known both as comet 107P/Wilson–Harrington and as asteroid 4015 Wilson–Harrington. It passed 0.4 AU from Earth on 20 July 2022 and then passed perihelion (closest approach to the Sun) on 24 August 2022. It seldom gets brighter than apparent magnitude 16. It will return to perihelion on 25 November 2026.
Observational history
This near-Earth object is considered both an Apollo asteroid with the designation 4015 Wilson–Harrington and a periodic comet known as Comet Wilson–Harrington or 107P/Wilson–Harrington. It was initially discovered in 1949 as a comet and then lost to further observations. Thirty years later it was rediscovered as an asteroid, after which it took over a decade to determine that these observations were of the same object. Therefore, it has both a comet designation and an asteroid designation, and with a name length of 17 characters it is currently the asteroid with the longest name, having one more character than the 16-character limit imposed by the IAU.
The comet was discovered on 19 November 1949, by Albert G. Wilson and Robert G. Harrington at Palomar Observatory. Only three photographic observations were obtained and the comet was lost (insufficient observations to determine a precise enough orbit to know where to look for future appearances of the comet.)
On 15 November 1979, an apparent Mars-crosser asteroid was found by Eleanor F. Helin, also of Palomar Observatory. It received the designation 1979 VA, and when re-observed on 20 December 1988, received the permanent number 4015.
On 13 August 1992, it was reported that asteroid (4015) 1979 VA and comet 107P/Wilson–Harrington were the same object. By then, enough observations of the asteroid had accumulated to obtain a fairly precise orbit, and the search of old photographic plates for prediscovery images turned up the 1949 plates with the images of the lost comet.
Although the 1949 images show cometary features, all subsequent images appear stellar, suggesting it might be an inactive comet that undergoes only infrequent outbursts.
Orbital and physical properties
The eccentricity is 0.624, which is somewhat higher than that of a typical asteroid-belt minor planet and more typical of periodic comets. Its Minimum Orbit Intersection Distance (MOID) of less than 0.05 AU and its large size make it a potentially hazardous asteroid (PHA).
There are only eight other objects that are cross-listed as both comets and asteroids: 2060 Chiron (95P/Chiron), 7968 Elst–Pizarro (133P/Elst–Pizarro), 60558 Echeclus (174P/Echeclus), 118401 LINEAR (176P/LINEAR), (282P/2003 BM80), (288P/2006 VW139), (362P/2008 GO98), and (433P/2005 QN173). As a dual status object, astrometric observations of 4015 Wilson–Harrington should be reported under the minor planet designation.
Exploration
A flyby of 4015 Wilson–Harrington was formerly planned by Deep Space 1. It was also considered for the NEAR mission.
References
References
- (2015). "Asteroids IV". [[University of Arizona]].
- Lutz D. Schmadel. (2012). "Dictionary of Minor Planet Names". Springer.
- [https://minorplanetcenter.net/iau/ECS/MPCArchive/2021/MPC_20210920.pdf M.P.C. 133823]
- [http://spider.seds.org/spider/Comets/c_missions.html Comet Space Missions]
- (1993). "Extended-mission opportunities for a Discovery-class asteroid rendezvous mission". SAO/NASA Astrophysics Data System.
This article was imported from Wikipedia and is available under the Creative Commons Attribution-ShareAlike 4.0 License. Content has been adapted to SurfDoc format. Original contributors can be found on the article history page.
Ask Mako anything about 4015 Wilson–Harrington — get instant answers, deeper analysis, and related topics.
Research with MakoFree with your Surf account
Create a free account to save articles, ask Mako questions, and organize your research.
Sign up freeThis content may have been generated or modified by AI. CloudSurf Software LLC is not responsible for the accuracy, completeness, or reliability of AI-generated content. Always verify important information from primary sources.
Report