249P/LINEAR
 The comet on 31 July 2020 by ZTF | |
| Discovery[1] | |
|---|---|
| Discovered by | LINEAR |
| Discovery date | October 19, 2006 |
| Designations | |
| P/2006 U1, P/2011 A4 | |
| Orbital characteristics[3] | |
| Epoch | July 25, 2014 (2456863.5) |
| Aphelion | 5.038 AU |
| Perihelion | 0.502 AU |
| Semi-major axis | 2.770 AU |
| Eccentricity | 0.8187 |
| Orbital period | 4.611 a 1684.2 d |
| Inclination | 8.399° |
| 239.852° | |
| Argument of periapsis | 64.81° |
| Last perihelion | 29 June 2020[2] |
| Next perihelion | 1 February 2025[2] |
| TJupiter | 2.707 |
| Earth MOID | 0.048 AU |
| Comet total magnitude (M1) | 18.4[3] |
249P/LINEAR is a periodic Jupiter-family comet with an orbital period of 4.61 years. It was discovered by LINEAR on 19 October 2006.[1] It is only active for a brief period around perihelion.
Observational history
[edit]The comet was at first reported as an asteroidal object with an apparent magnitude of 17.3 by LINEAR on 19 October 2006. However it was quickly found to be cometary in appearance, with a narrow tail up to 12 arcminutes long and a coma 10 arcseconds across.[1] On 21 October the tail appeared almost disconnected from the head of the comet. A preliminary orbit suggested a short period object with an orbital period of 4.33 years.[1] The comet was recovered on 14 January 2011 by Leonid Elenin using a remote observatory of ISON, when it had an apparent magnitude of 19–19.5.[4]
249P/LINEAR has frequently passed through the fields of view of various solar observatories when near perihelion. Its most favorable apparition to date came in 2020 (perihelion June 29) when it was successfully observed by SOHO from June 16-21 (heliocentric distance, r = 0.58-0.52 AU; cometocentric distance, delta = 0.44-0.49 AU; phase angle = 163-171 deg), Parker Solar Probe on June 28 (r = 0.50 AU; delta = 0.11 AU; phase = 120 deg), and STEREO-A from July 2-16 (r = 0.50-0.62 AU; delta = 1.18-1.46 AU; phase = 53-28 deg). In addition, it was well observed by STEREO-A in April 2011 (r = 0.57-0.52 AU; delta =0.46-0.44 AU; phase = 135-166 deg) and was not detected by SOHO despite highly favorable viewing geometry in May 1997 (r = 0.79-0.73 AU; delta = 0.20-0.27 AU; phase = 168-171 deg). It was also not detected by SOHO and STEREO on several other apparitions at less favorable viewing geometries.[5]
During the 2020 apparition the comet appeared to lack a central condensation in images obtained in 20 and 21 July and with an apparent magnitude of 15 it was fainter than predicted, leading to speculation that the comet disintergrated.[6]
On 3 November 2029 the comet will approach Earth to a distance of 0.057 AU (8.5 million km) with a relative speed of 26.93 km/s.[3]
Scientific results
[edit]The comet has an absolute (visual) nuclear magnitude of 17.0 ± 0.4 which corresponds to a radius of 1 to 1.3 kilometers assuming an albedo of 0.04–0.07.[7] The reflection spectrum is similar to that of a B-type asteroid when the comet is near perihelion,[7] but it is weakly red when it is less active, like a typical C-type asteroid, and it appears featureless.[8]
The current orbit suggests that the orbit has been stable in the near-Earth space for about 10,000 years. It is possible that it originates from the main asteroid belt.[7] The perihelion distance appears to be slightly decreasing, meaning that it is at or near its warmest stage for the last few thousands years.[8] It is possible that the comet is dynamically linked with the Taurid complex, which was created by comet Encke.[9]
Observations of the comet during the 2006 and 2016 apparitions indicate that it is active for about 20 days around perihelion, with a dust production rate up to 145 ± 50 kg/s and a total mass loss of (2.5±0.9)×108 kg, which is low when compared with other Jupiter-family comets, indicating that it is depleted in volatiles.[7][10] It may be near the end of its active phase and evolve to a mostly inactive body, like 3200 Phaethon.[11]
References
[edit]- ^ a b c d McGaha, J. E.; Young, J.; Hicks, M.; Hug, G.; Tibbets, D.; Ries, J. G.; Reina, E.; Durig, D. T.; Pierce, E. A.; Christensen, E. J.; Stevens, B. L. (1 October 2006). "Comet P/2006 U1 (LINEAR)". International Astronomical Union Circular (8763): 1. ISSN 0081-0304.
- ^ a b "249P/LINEAR". www.aerith.net. Retrieved 17 August 2024.
- ^ a b c "Small-Body Database Lookup: 249P/LINEAR". ssd.jpl.nasa.gov. Retrieved 20 July 2023.
- ^ Elenin, L.; Nakano, S.; Green, D. W. E. (1 January 2011). "Comet P/2011 a4 = P/2006 u1 (linear)". International Astronomical Union Circular (9194): 1. Bibcode:2011IAUC.9194....1E. ISSN 0081-0304.
- ^ Knight, M. M.; Battams, K.; Kelley, M. S.; Stenbourg, G.; Marcus, J. N.; Hsieh, H. H. (1 October 2020). "Multi-spacecraft study of the activity of comet 249P/LINEAR near perihelion from 1997-2020". Bulletin of the American Astronomical Society. 52 (6): 319.05. Bibcode:2020DPS....5231905K.
This article contains quotations from this source, which is available under the Creative Commons Attribution 4.0 Unported (CC BY 4.0) license.
- ^ Lin, Zhong-Yi; Ip, Wing-Huen; Kelley, Michael S. P.; Lin, Chi-Sheng; Hsiao, Hsiang-Yao; Hou, Wei-Jir; Lin, Hung-Chin (1 July 2020). "The Disintegration of Comet 249P/LINEAR". The Astronomer's Telegram. 13890: 1. Bibcode:2020ATel13890....1L.
- ^ a b c d Fernández, Julio A.; Licandro, Javier; Moreno, Fernando; Sosa, Andrea; Cabrera-Lavers, Antonio; de León, Julia; Birtwhistle, Peter (October 2017). "Physical and dynamical properties of the anomalous comet 249P/LINEAR". Icarus. 295: 34–45. arXiv:1704.04639. Bibcode:2017Icar..295...34F. doi:10.1016/j.icarus.2017.04.004.
- ^ a b Kareta, Theodore; Hergenrother, Carl; Reddy, Vishnu; Harris, Walter M. (1 February 2021). "Surfaces of (Nearly) Dormant Comets and the Recent History of the Quadrantid Meteor Shower". The Planetary Science Journal. 2 (1): 31. Bibcode:2021PSJ.....2...31K. doi:10.3847/PSJ/abd403.
- ^ Orofino, Vincenzo (4 October 2022). "Main Belt Comets and other "Interlopers" in the Solar System". Universe. 8 (10): 518. Bibcode:2022Univ....8..518O. doi:10.3390/universe8100518.
- ^ Moreno, Fernando (3 July 2022). "Monte Carlo Models of Comet Dust Tails Observed from the Ground". Universe. 8 (7): 366. Bibcode:2022Univ....8..366M. doi:10.3390/universe8070366.
- ^ Kareta, Theodore; Reddy, Vishnu; Hergenrother, Carl; Lauretta, Dante S.; Arai, Tomoko; Takir, Driss; Sanchez, Juan; Hanuš, Josef (1 December 2018). "Rotationally Resolved Spectroscopic Characterization of Near-Earth Object (3200) Phaethon". The Astronomical Journal. 156 (6): 287. arXiv:1810.11157. Bibcode:2018AJ....156..287K. doi:10.3847/1538-3881/aaeb8a.
External links
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