152P/Helin–Lawrence
| Discovery[1] | |
|---|---|
| Discovered by | Eleanor F. Helin Kenneth J. Lawrence |
| Discovery site | Palomar Observatory |
| Discovery date | 17 May 1993 |
| Designations | |
| P/1993 K2 P/2001 Y1 | |
| 1993 XI, 1993l[2] | |
| Orbital characteristics[5][6] | |
| Epoch | 9 February 2015 (JD 2457062.5) |
| Observation arc | 31.71 years |
| Earliest precovery date | 21 April 1993 |
| Number of observations | 1,298 |
| Aphelion | 5.874 AU |
| Perihelion | 3.113 AU |
| Semi-major axis | 4.493 AU |
| Eccentricity | 0.30722 |
| Orbital period | 9.52 years |
| Inclination | 9.868° |
| 91.899° | |
| Argument of periapsis | 163.59° |
| Mean anomaly | 97.858° |
| Last perihelion | 13 January 2022[3] |
| Next perihelion | 9 July 2031[4] |
| TJupiter | 2.901 |
| Earth MOID | 2.099 AU |
| Jupiter MOID | 0.338 AU |
| Physical characteristics[5] | |
Mean diameter | 4.6 km (2.9 mi)[7] |
| Comet total magnitude (M1) | 12.7 |
152P/Helin–Lawrence is a Jupiter-family comet with a 9.52-year orbit around the Sun. It is the third comet co-discovered by Eleanor F. Helin and Kenneth J. Lawrence.[a][b]
Observational history
Both Helin and Lawrence discovered the diffuse trails of the comet from the photographic plates exposed from the Palomar Observatory on the night of 17 May 1993.[1] At the time, it was a 17th-magnitude object within the constellation Scorpio.[c] Shortly after the announcement of its discovery, Robert H. McNaught was able to observe it during the total lunar eclipse of 4 June 1995.[9]
It was recovered from the Saji Observatory by T. Oribe and Shuichi Nakano on 24 December 2001.[10]
Physical characteristics
Polarimetric observations from the European Southern Observatory in 2012 revealed that both 74P/Smirnova–Chernykh and 152P/Helin–Lawrence still produce cometary activity even at large heliocentric distances, suggesting that both comets were relative newcomers to the inner Solar System and thus contain large reservoirs of volatile material in their respective interiors.[11]
The nucleus of 152P/Helin–Lawrence is estimated to be around 4.6 km (2.9 mi) in diameter,[7] based on observations conducted using the Hubble and Keck telescopes in 1998.[12]
Notes
References
- ^ a b E. F. Helin; K. J. Lawrence; M. Nassir; et al. (2 June 1993). D. W. Green (ed.). "Comet Helin–Lawrence (1993l)". IAU Circular. 5810 (1). Bibcode:1993IAUC.5810....1H.
- ^ "Comet Names and Designations". International Comet Quarterly. Retrieved 26 November 2025.
- ^ S. Nakano (6 February 2011). "152P/Helin–Lawrence (NK 2031)". OAA Computing and Minor Planet Sections. Retrieved 25 February 2012.
- ^ "Horizons Batch for 152P/Helin–Lawrence on 2031-Jul-09" (Perihelion occurs when rdot flips from negative to positive). JPL Horizons. Retrieved 22 June 2022. (JPL#72 Soln.date: 2022-Jun-20)
- ^ a b "152P/Helin–Lawrence – JPL Small-Body Database Lookup". ssd.jpl.nasa.gov. Jet Propulsion Laboratory. Retrieved 26 November 2025.
- ^ "152P/Helin–Lawrence Orbit". Minor Planet Center. Retrieved 18 June 2014.
- ^ a b P. L. Lamy; I. Toth; Y. R. Fernández; H. A. Weaver (2004). "The Sizes, Shapes, Albedos, and Colors of Cometary Nuclei" (PDF). Comets II. University of Arizona Press. pp. 223–264. Bibcode:2004come.book..223L. doi:10.2307/j.ctv1v7zdq5.22. ISBN 978-0-8165-2450-1. JSTOR j.ctv1v7zdq5.22.
- ^ G. W. Kronk; M. Meyer; D. A. J. Seargent (2017). Cometography: A Catalog of Comets. Vol. 6: 1983–1993. Cambridge University Press. pp. 783–787. ISBN 978-0-521-87216-4.
- ^ E. F. Helin; K. J. Lawrence; M. Nassir; et al. (4 June 1993). D. W. Green (ed.). "Periodic Comet Helin–Lawrence (1993l)". IAU Circular. 5811 (1). Bibcode:1993IAUC.5811....1H.
- ^ S. Nakano; T. Oribe; B. G. Marsden; et al. (14 January 2002). D. W. Green (ed.). "Comet P/2001 Y1 (Helin–Lawrence)". IAU Circular. 7790 (1). Bibcode:2002IAUC.7790....1N.
- ^ A. Stinson; S. Bagnulo; G. P. Tozzi; et al. (2016). "Polarimetry of comets 67P/Churyumov–Gerasimenko, 74P/Smirnova–Chernykh, and 152P/Helin–Lawrence" (PDF). Astronomy & Astrophysics. 594 (A110): 1–16. arXiv:1606.05192. Bibcode:2016A&A...594A.110S. doi:10.1051/0004-6361/201527696.
- ^ K. J. Meech; O. R. Hainaut; B. G. Marsden (2004). "Comet nucleus size distributions from HST and Keck telescopes". Icarus. 170 (2): 463–491. Bibcode:2004Icar..170..463M. doi:10.1016/j.icarus.2004.03.014.
External links
- 152P/Helin–Lawrence at the JPL Small-Body Database
- 152P/Helin–Lawrence at Gary W. Kronk's Cometography
- 152P/Helin–Lawrence at Seiichi Yoshida's website