C/2006 VZ13 (LINEAR)
Comet LINEAR and ι Draconis photographed from Mount Laguna, California on 11 July 2007 | |
| Discovery[1] | |
|---|---|
| Discovery site | LINEAR |
| Discovery date | 13 November 2006 |
| Orbital characteristics[2] | |
| Epoch | 13 June 2007 (JD 2454264.5) |
| Observation arc | 274 days |
| Number of observations | 1,025 |
| Perihelion | 1.015 AU |
| Eccentricity | 1.000249 |
| Inclination | 134.79° |
| 66.027° | |
| Argument of periapsis | 174.12° |
| Last perihelion | 10 August 2007 |
| Earth MOID | 0.0047 AU |
| Jupiter MOID | 2.8204 AU |
| Physical characteristics | |
Mean radius | 0.723 km (0.449 mi)[a] |
| Comet total magnitude (M1) | 8.0[3] |
| 7.5 (2007 apparition) | |
C/2006 VZ13 (LINEAR) is a non-periodic comet discovered by the LINEAR survey on 13 November 2006.
Discovery and observations
[edit]
The object was initially believed to be an asteroid due to its stellar appearance in the early images.[1] However, observers soon detected a small coma and the telltale green cometary cast.[1]
The comet peaked at approximately magnitude +7.5,[4] much brighter than predicted.[5] The comet made its closest approach to Earth on 14 July 2007 at a distance of 0.575 AU (86.0 million km).[2] It reached perihelion on 10 August 2007 at a distance of 1.015 AU (151.8 million km).
Physical characteristics
[edit]Infrared measurements from the NASA Infrared Telescope Facility (IRTF) in July 2007 yielded a mean grain temperature of 275±5 K, which was 6 percent higher than the equivalent radiative equilibrium blackbody of the comet at its distance from the Sun, which was approximately 1.02 AU at the time.[6] Spectroscopic observations on the following month reveal that the comet's composition is depleted of carbon compounds, comparable to what was observed from 9P/Tempel.[7]
Notes
[edit]References
[edit]- 1 2 3 C. W. Hergenrother (4 December 2006). D. W. Green (ed.). "Comet C/2006 VZ13 (LINEAR)". IAU Circular. 8781 (1). Bibcode:2006IAUC.8781....1H.
- 1 2 "C/2006 VZ13 (LINEAR) – JPL Small-Body Database Lookup". ssd.jpl.nasa.gov. Jet Propulsion Laboratory. Retrieved 3 January 2024.
- 1 2 J. A. Fernández; A. Sosa (2012). "Magnitude and size distribution of long-period comets in Earth-crossing or approaching orbits". Monthly Notices of the Royal Astronomical Society. 423 (2): 1674–1690. arXiv:1204.2285. Bibcode:2012MNRAS.423.1674F. doi:10.1111/j.1365-2966.2012.20989.x.
- ↑ S. Yoshida. "C/2006 VZ13 (LINEAR)". www.aerith.net. Retrieved 13 July 2007.
- ↑ T. Flanders (10 July 2007). "Comet LINEAR Graces the Northern Sky". Sky & Telescope. Archived from the original on 1 October 2011. Retrieved 12 July 2007.
- ↑ M. L. Sitko; L. Beerman; R. W. Russell; et al. (12 July 2007). D. W. Green (ed.). "Comet C/2006 VZ13 (LINEAR)". IAU Circular. 8855 (2). Bibcode:2007IAUC.8855....2S.
- ↑ A. M. Gilbert; P. A. Wiegert; E. Unda-Sanzana; O. Vaduvescu (2010). "Spectroscopic observations of new Oort cloud comet 2006 VZ13 and four other comets" (PDF). Monthly Notices of the Royal Astronomical Society. 401 (4): 2399–2405. arXiv:0910.0416. Bibcode:2010MNRAS.401.2399G. doi:10.1111/j.1365-2966.2009.15822.x.