Discovery | |
---|---|
Discovered by | Alphonse Borrelly |
Discovery date | December 28, 1904 |
Designations | |
Alternative names | 1905 II; 1911 VIII; 1918 IV; 1925 VIII; 1932 IV; 1953 IV; 1960 V; 1967 VIII; 1974 VII; 1981 IV; 1987 XXXIII; 1994 XXX |
Orbital characteristics | |
Epoch 2022-08-09 (JD 2459800.5) | |
Aphelion | 5.90 AU |
Perihelion | 1.306 AU |
Semi-major axis | 3.61 AU |
Eccentricity | 0.6377 |
Orbital period (sidereal) | 6.85 yr |
Inclination | 29.30° |
Time of perihelion | 2028-Dec-11 February 1, 2022 (last) |
Earth MOID | 0.36 AU (54 million km) |
Physical characteristics | |
Dimensions | 8×4×4 km |
Mean radius | 2.4 km |
Mass | 2×10 kg |
Mean density | 0.3 g/cm |
Albedo | 0.03 |
Perihelion distance at recent epochs | |||||||
Epoch | Perihelion (AU) | ||||||
---|---|---|---|---|---|---|---|
2028 | 1.310 | ||||||
2022 | 1.306 | ||||||
2015 | 1.349 | ||||||
2008 | 1.355 |
Comet Borrelly /bɒˈrɛli/ or Borrelly's Comet (official designation: 19P/Borrelly) is a comet with a period of 6.85 years that was visited by the spacecraft Deep Space 1 in 2001. The comet last came to perihelion (closest approach to the Sun) on February 1, 2022 and will next come to perihelion on December 11, 2028.
Date & time of closest approach |
Earth distance (AU) |
Sun distance (AU) |
Velocity wrt Earth (km/s) |
Velocity wrt Sun (km/s) |
Uncertainty region (3-sigma) |
Reference |
---|---|---|---|---|---|---|
2028-Dec-05 19:12 ± 6 min | 0.413 AU (61.8 million km; 38.4 million mi; 161 LD) | 1.31 AU (196 million km; 122 million mi; 510 LD) | 17.3 | 33.3 | ± 41 thousand km | Horizons |
Deep Space 1 returned images of the comet's nucleus from 3400 kilometers away. At 45 meters per pixel, it was the highest resolution view ever seen of a comet up until that time.
Discovery
The comet was discovered by Alphonse Borrelly during a routine search for comets at Marseilles, France on December 28, 1904.
Exploration
Deep Space 1 flyby
On September 21, 2001 the spacecraft Deep Space 1, which was launched to test new equipment in space, performed a flyby of Borrelly. It was steered toward the comet during the extended mission of the craft, and presented an unexpected bonus for the mission scientists. Despite the failure of a system that helped determine its orientation, Deep Space 1 managed to send back to Earth what were, at the time, the best images and other science data from a comet.
References
- ^ MPC
- ^ "Horizons Batch for 19P/Borrelly (90000304) on 2028-Dec-11" (Perihelion occurs when rdot flips from negative to positive). JPL Horizons. Archived from the original on 2023-02-11. Retrieved 2023-07-06. (JPL#K222/14 Soln.date: 2023-May-25)
- Weaver, H. A.; Stern, S.A.; Parker, J. Wm. (2003). "Hubble Space Telescope STIS Observations of Comet 19P/BORRELLY during the Deep Space 1 Encounter". The Astronomical Journal. 126 (1). The American Astronomical Society: 444–451. Bibcode:2003AJ....126..444W. doi:10.1086/375752.
- "19P/Borrelly: Facts & Figures". Archived from the original on 2014-08-09. Retrieved 2014-08-08.
- Using the volume of an ellipsoid of 8x4x4km * a rubble pile density of 0.3 g/cm yields a mass (m=d*v) of 2.0E+13 kg.
- D. T. Britt; G. J. Consol-magno SJ; W. J. Merline (2006). "Small Body Density and Porosity: New Data, New Insights" (PDF). Lunar and Planetary Science XXXVII. Archived (PDF) from the original on 17 December 2008. Retrieved 2008-12-16.
- Robert Roy Britt (2001-11-29). "Comet Borrelly Puzzle: Darkest Object in the Solar System". Space.com. Archived from the original on 22 January 2009. Retrieved 2008-12-16.
- Seiichi Yoshida (2021-04-03). "19P/Borrelly". Seiichi Yoshida's Comet Catalog. Retrieved 2022-06-15.
- Beatty, Kelly (25 June 2004). "Meet Comet Borrelly". Sky & Telescope. Retrieved 27 January 2021.
External links
- http://jcometobs.web.fc2.com/pcmtn/0019p.htm
- 19P – Gary W. Kronk's Cometography
- Elements and Ephemeris for 19P/Borrelly – Minor Planet Center
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