Lost minor planet

More than 700,000 minor planets have been observed, many of which must be considered lost due to insufficient observational data.[1][2]

Lost minor planets are minor planets that observers lose track of due to too short an observation arc to accurately predict the future location of the minor planet. Many of the asteroids that were discovered early were lost and rediscovered in the 1980s and 1990s, but a number of minor planets continue to be lost.[3] By some definitions, thousands, if not tens of thousands observed minor planets are lost—they cannot be found by pointing an appropriate telescope at their predicted location, because the uncertainty in their predicted orbit is too large or they are currently too faint to be detected.[2]

Some minor planets and comets discovered in previous decades were "lost" because the observational data obtained was insufficient to determine a reliable orbit. Without this information, astronomers would not know where to look for the object at future dates. Occasionally, a "newly discovered" object turns out to be a rediscovery of a previously lost object. This can be determined by calculating the "new" object's orbit backwards and checking its past positions against those previously recorded for the lost object. This may greatly extend the observation arc, thus fixing the orbit much more precisely. For lost comets the back orbit calculations are especially tricky because of nongravitational forces that can affect their orbits, such as emission of jets of gas from the comet nucleus. However, Brian G. Marsden has specialized in calculating such nongravitational forces. Notably, he successfully predicted the 1992 return of the once-lost periodic comet Swift–Tuttle.

Overview

This is a small selection of some early lost or notable asteroids with their discovery and rediscovery dates. (A more detailed description for some of these minor planets can be found in the following sections). The true number of lost asteroids may be over 150,000.[2] There are also about 30,000 unnumbered bodies with a condition code of U = 9, indicating the highest possible uncertainty of their orbit determination. Many of these bodies have been observed years if not decades ago and must be considered lost.[4][lower-alpha 1] There are also more than a thousand near-Earth objects (NEOs) with an observation arc of one or two days only.[5]

Designation Year of
discovery recovery
132 Aethra 1873 1922[6]
1892 X (330 Adalberta) 1892 false positive [lower-alpha 2]
452 Hamiltonia 1899 1987
473 Nolli 1901 1987
719 Albert 1911 2000
724 Hapag 1911 1988
843 Nicolaia 1916 1981
878 Mildred 1916 1991
1009 Sirene 1923 1982[7]
1026 Ingrid 1923 1986
1179 Mally 1931 1986
Name Year of
discovery recovery
1537 Transylvania 1940 1981
1862 Apollo 1932 1973
1916 Boreas 1953[8] 1976
1922 Zulu 1949 1974
2101 Adonis 1936 1977
3494 Purple Mountain 1962 1980
3789 Zhongguo 1928 1986
7796 Járacimrman 1973 1996
(29075) 1950 DA 1950 2000
69230 Hermes 1937 2003[8][9]
 
Designation Year of Notes
discovery recovery
1927 LA [10] 1927 still lost Observed 4 times between 1 June 1927 and 5 July 1927, MPC
1991 BA 1991 still lost Passed within a lunar distance of Earth
1993 HD 1993 still lost[11] Near-Earth asteroid, MPC
1995 SN55 1995 still lost May be the largest centaur
2007 WD5 2007 still lost Passed close to Mars
6344 P–L 1960 2007[12] Potentially hazardous object; probably a dormant comet

20th-century recoveries

The number of asteroids that were only observed once and not re-observed grew throughout the 19th and 20th centuries, but improved telescopes, searches, and detection techniques led to resolution of most of these cases between 1970 and 2000. There are earlier examples also, such as 132 Aethra, which was lost between 1873 and 1922.[6]

1970s

Recovered body Description
1862 Apollo Apollo is a Q-type asteroid, discovered by Karl Reinmuth in 1932, but lost and not recovered until 1973. Another Apollo asteroid is 2101 Adonis, discovered by Eugene Delporte in 1936 and lost until 1977 when it was rediscovered by Charles T. Kowal. It was also one of the first near-Earth asteroids to be discovered.
1916 Boreas The Amor asteroid Boreas, provisionally designated 1953 RA, was discovered on 1 September 1953 by Sylvain Julien Victor Arend at the Royal Observatory of Belgium, and rediscovered in 1974 by Richard Eugene McCrosky, G. Schwartz and JH Bulger based on a predicted position by Brian G. Marsden.[8][13]
1922 Zulu The outer main-belt asteroid, provisionally designated 1949 HC, was discovered on 25 April 1949 by Ernest Leonard Johnson at Johannesburg (UO).[8] It is one of very few asteroids located in the 2:1 mean-motion resonance with Jupiter.[14] This asteroid was lost shortly after discovery and only rediscovered in 1974 by Richard Eugene McCrosky, Cheng-yuan Shao and JH Bulger based on a predicted position by C. M. Bardwell of the Cincinnati Observatory.[8][13]

1980s and 1990s

Leif Kahl Kristensen at the University of Aarhus rediscovered 452 Hamiltonia and 1537 Transylvania, along with numerous other small objects, in 1981.[15] At the time these results were published, only the nine numbered minor planets 330 Adalberta, 473 Nolli, 719 Albert, 724 Hapag, 843 Nicolaia, 878 Mildred, 1009 Sirene, 1026 Ingrid, and 1179 Mally remained unobserved since their discoveries:[15]

Recovered body Description
330 Adalberta Adalberta, provisionally designated 1892 X, was not rediscovered, since it turned out to be an erroneous observation. The designation was later reassigned to A910 CB after 1892 X was determined to be a false positive.[16] 2006 HH123 was another lost minor planet that turned out to be a false positive.
843 Nicolaia Nicolaia, provisionally designated 1916 AN, was rediscovered at the Heidelberg Astronomisches Rechen-Institut in 1981.[17]
473 Nolli Nolli, provisionally designated 1901 GC, was discovered by Max Wolf on 13 February 1901, but it remained lost for many decades until it was recovered finally in 1987, 86 years later.[18]
724 Hapag Hapag had first been found by Johann Palisa in 1911. It was given the provisional name 1911 NC, but was lost until it was rediscovered in 1988.[19][20]
719 Albert Near-Earth asteroid 719 Albert (1911 MT) had also been found by Johann Palisa in 1911. Due to inaccuracies in its computed orbit, Albert was also lost and not recovered until 2000, when Jeffrey A. Larsen located it using data from the Spacewatch asteroid survey project. At the time of its rediscovery, Albert was the last remaining "lost asteroid" among those assigned numbers (since 69230 Hermes was not numbered until 2003).[20]
878 Mildred Mildred, provisionally designated 1916 f, was originally discovered in 1916 using the 60-inch Hale telescope at the Californian Mount Wilson Observatory, but was subsequently lost until it was again observed on single nights in 1985 and 1991.[20][21]
1009 Sirene Sirene, provisionally designated 1923 PE, was recovered in 1982 by J. Gibson using exposures form the Samuel Oschin Telescope at Palomar Observatory, and he revised its ephemeris.[7]
1026 Ingrid Ingrid was discovered by Karl Reinmuth on 13 August 1923 and given the provisional designation 1923 NY.[8] It was reidentified in 1986 by Syuichi Nakano.[22]
1179 Mally Mally was discovered by Max Wolf on 19 March 1931 and given the provisional designation 1931 FD.[8] It was rediscovered in 1986 by Lutz Schmadel, Richard Martin West and Hans-Emil Schuster.[23]
Other notable recoveries

21st century

Recently lost minor planets

See also

Notes

  1. ↑ Note: this query at JPL's Small-Body Database lists all unnamed asteroids with an orbital uncertainty of 9, which also includes recently discovered bodies. The lost minor planets appear first, since the table is sorted by the body's first observation date.
  2. ↑ On 18 March 1892, a body discovered by Max Wolf with the provisional designation 1892 X was originally named 330 Adalberta, but was lost and never recovered. In 1982, it was determined that Wolf erroneously measured two images of stars, not asteroids. Because it was a false positive and the body never existed, the named designation 330 Adalberta was reused for another asteroid, A910 CB, discovered in 1910.

References

  1. ↑ "Running Tallies – Minor Planets Discovered". IAU Minor Planet Center. Retrieved 19 August 2015.
  2. 1 2 3 '''Asteroids: overview, abstracts, and bibliography''' (2002), by Edward C. Blair, Page 177. Books.google.com. Retrieved 2013-07-23.
  3. ↑ Lost asteroid. (2009). In Encyclopædia Britannica. Retrieved 27 February 2009, from Encyclopædia Britannica Online: http://www.britannica.com/topic/lost-asteroid
  4. ↑ "JPL Small-Body Database Search Engine: Unnumbered asteroids with condition code of 9, oldest first obs. shown first". JPL Solar System Dynamics. Retrieved 24 May 2016.
  5. ↑ "JPL Small-Body Database Search Engine: NEOs with observation arc of 1 or 2 days only". JPL Small-Body Database. Retrieved 24 May 2016.
  6. 1 2 '''The planet observer's handbook''' (2000), By Fred William Price, Page 192. (Google Books 2010). Books.google.com. 2000-10-26. Retrieved 2013-07-23.
  7. 1 2 "(1009) Sirene Gibson, J.; Kristensen, L. K. IAU Circ., 3714, 1 (1982). Edited by Marsden, B. G". Adsabs.harvard.edu. Retrieved 2013-07-23.
  8. 1 2 3 4 5 6 7 "Discovery Circumstances: Numbered Minor Planets (1)–(5000)". IAU: Minor Planet Center. Retrieved 5 July 2011.
  9. ↑ "MPEC 2003-T74 : 1937 UB (HERMES)". Minorplanetcenter.net. Retrieved 2013-07-23.
  10. ↑ "1927 LA". Minor Planet Center. Retrieved 24 May 2016.
  11. ↑ "1993 HD". Minor Planet Center. Retrieved 2013-07-23.
  12. 1 2 "Long-Lost, Dangerous Asteroid Is Found Again – ScienceDaily (15 Oct. 2007)". Sciencedaily.com. 2007-10-15. Retrieved 2015-08-18.
  13. 1 2 Brian G. Marsden (24 October 1974). "International Astronomical Union Circular 2710". Central Bureau for Astronomical Telegrams. Retrieved 5 July 2011.
  14. ↑ Roig; Nesvorny, D.; Ferraz-Mello, S. (2002). "Asteroids in the 2 : 1 resonance with Jupiter: dynamics and size distribution". Monthly Notices of the Royal Astronomical Society. 335 (2): 417–431. Bibcode:2002MNRAS.335..417R. doi:10.1046/j.1365-8711.2002.05635.x.
  15. 1 2 Kristensen, L. K.; Gibson, J.; Shao, C.-Y.; Bowell, E.; Marsden, B. G. (April 1981). "(1537) Transylvania and (452) Hamiltonia". IAU Circ. (3595). Bibcode:1981IAUC.3595....1K. Retrieved 24 May 2016.
  16. ↑ "JPL Small-Body Database Browser: 330 Adalberta (A910 CB)" (2016-04-17 last obs.). Jet Propulsion Laboratory. Retrieved 24 May 2016.
  17. ↑ http://www3.interscience.wiley.com/journal/112427258/abstract?CRETRY=1&SRETRY=0 Recovery of the Long Lost Minor Planet (843) Nicolaia after 65 Years (Astronomisches Rechen-Institut Heidelberg – Mitteilungen Serie B) L. D. Schmadel 1 *, L. Kohoutek 2 * Heidelberg Astronomisches Rechen-Institut
  18. ↑ IAUC 4292
  19. ↑ Schmadel, Lutz D. (1997). Dictionary of Minor Planet Names. Springer Science+Business Media. p. 70. ISBN 0-354-06174-7.
  20. 1 2 3 Cowen, Ron (20 May 2000). "Astronomers Rediscover Long-Lost Asteroid". 157 (21). Science News.
  21. ↑ "IAU Circular: IAUC 5275". 25 May 1991.
  22. ↑ Brian G. Marsden (8 December 1986). "International Astronomical Union Circular 4281". Central Bureau for Astronomical Telegrams. Retrieved 5 July 2011.
  23. ↑ Brian G. Marsden (5 December 1986). "International Astronomical Union Circular 4278". Central Bureau for Astronomical Telegrams. Retrieved 5 July 2011.
  24. ↑ Schmadel, Lutz D. (2007). Dictionary of Minor Planet Names – (3789) Zhongguo. Springer Berlin Heidelberg. p. 320. ISBN 978-3-540-00238-3. Retrieved 24 May 2016.
  25. ↑ "Earth Impact Risk Summary: 29075 1950 DA". NASA/JPL Near-Earth Object Program Office. Nov 26, 2013. Retrieved 2014-06-23.
  26. ↑ "JPL Small-Body Database Browser: 2007 WD5". Retrieved 12 January 2008.
  27. 1 2 Don Yeomans, Paul Chodas and Steve Chesley (28 December 2007). "Mars Impact Probability Increases to 4 Percent". NASA/JPL Near-Earth Object Program Office. Retrieved 28 December 2007.
  28. 1 2 Steve Chesley, Paul Chodas and Don Yeomans (9 January 2008). "2007 WD5 Mars Collision Effectively Ruled Out – Impact Odds now 1 in 10,000". NASA/JPL Near-Earth Object Program Office. Retrieved 9 January 2008.
  29. ↑ Lakdawalla, Emily (4 February 2008). "WD5 most likely missed Mars, but we may never know". Retrieved 24 February 2008.
  30. ↑ "Horizons Archive Mars/Earth 2003/2008". Retrieved 23 December 2007. (Soln.date: 2007-Dec-23)
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