Lexell's Comet

Last updated

D/1770 L1 (Lexell)
Discovery [1]
Discovered by Charles Messier
Discovery dateJune 14, 1770
Designations
1770 I,
P/Lexell,
Lexell's Comet
Orbital characteristics
Epoch 1770-Aug-14
(JD 2367764.5) [2]
Aphelion 5.6184 ± 0.0409 AU
Perihelion 0.6746 ± 0.003 AU (before Jupiter encounter of 1779)
Semi-major axis 3.1465 ± 0.0206 AU
Eccentricity 0.7856 ± 0.0013
Orbital period 5.58 years (2039 days)
Inclination 1.550 ± 0.004°
134.50 ± 0.12
Argument of
periapsis 		224.98 ± 0.12
Longitude of
perihelion 		359.48 ± 0.24
Last perihelionAugust 14, 1770
Next perihelionunknown/Lost
Physical characteristics
Dimensions ~4–30 km
(529668) 2010 JL33
Discovery [3]
Discovered by MLS
Discovery site Mount Lemmon Obs.
Discovery dateMay 6, 2010
Designations
(529668) 2010 JL33
2010 JL33
D/1770 L1 (Lexell) (possibly)
Apollo  · NEO  · PHA   [3] [4]
Orbital characteristics   [4]
Epoch 2022-Aug-09 (JD 2459800.5)
Uncertainty parameter 0
Observation arc 22.75 yr (8,309 d)
Earliest precovery date4 June 1997
Aphelion 4.649 AU
Perihelion 0.70971 AU
2.6793 AU
Eccentricity 0.73512
4.39 yr (1,601 d)
250.87°
0° 13m 28.56s / day
Inclination 5.3772°
52.452°
2.32° [2] (good match for Lexell)
7 December 2023
309.87°
Earth  MOID 0.031  AU (12  LD)
Venus  MOID 0.00074  AU (110 thousand  km) [3]
Mars  MOID 0.039 AU
Jupiter  MOID 0.84 AU
TJupiter 2.911
Physical characteristics [5]
1.778±0.034  km [6]
9.443±0.002  h [7]
0.047±0.009 [6]
17.9 [3]

    D/1770 L1, popularly known as Lexell's Comet after its orbit computer Anders Johan Lexell, was a comet discovered by astronomer Charles Messier in June 1770. [note 1] It is notable for having passed closer to Earth than any other comet in recorded history, approaching to a distance of only 0.015 astronomical units (2,200,000 km; 1,400,000 mi), [1] [8] [9] or six times the distance from the Earth to the Moon. The comet has not been seen since 1770 and is considered a lost comet.

    Contents

    Lexell's Comet's 1770 passing still holds the record of closest observed approach of Earth by a comet. [9] However, if approaches deduced from orbit calculations are included, it may have been beaten by a small sungrazing comet, P/1999 J6 (SOHO), which may have passed even closer at about 0.012 AU (1,800,000 km; 1,100,000 mi) from Earth on June 12, 1999, [10] but the uncertainties are around ±1.5 million km [11] as the P/1999 J6 approach was unobserved. [12]

    Discovery

    Charles Messier, who discovered Lexell's Comet Charles Messier.jpg
    Charles Messier, who discovered Lexell's Comet

    The comet was discovered on June 14, 1770, in the constellation Sagittarius by Messier, who had just completed an observation of Jupiter and was examining several nebulae. [1] At this time it was very faint, but his observations over the course of the next few days showed that it rapidly grew in size, its coma reaching 27 arcminutes across by June 24: by this time it was of magnitude +2. The comet was also noted by several other astronomers.[ citation needed ]

    The comet was observed in Japan. Surviving records identify it as an astronomical and historical phenomenon. [13]

    It was observed in the Hejaz in Safar 1184 AH (June 1770), where some believed it to be the comet predicted by the poet al-Fasi, portending future events. [14] [15]

    Close approach to Earth

    On July 1, 1770, the comet passed 0.015 astronomical units from Earth, [9] or approximately 6 times the radius of the Moon's orbit. Charles Messier measured the coma as 2° 23' across, around four times the apparent angular size of the Moon. An English astronomer at the time noted the comet crossing over 42° of sky in 24 hours; he described the nucleus as being as large as Jupiter, "surrounded with a coma of silver light, the brightest part of which was as large as the moon's orb". [1]

    Messier was the last astronomer to observe the comet as it moved away from the Sun, on October 3, 1770. [1]

    Orbit

    Scientists at the time largely believed that comets originated outside the solar system, and therefore initial attempts to model the comet's orbit assumed a parabolic trajectory, which indicated a perihelion date (the date of the closest approach to the Sun) of August 9–10. [16] When it turned out that the parabolic solution was not a good fit to the comet's orbit, Anders Johan Lexell suggested that the comet followed an elliptical orbit. His calculations, made over a period of several years, gave a perihelion of August 13–14 and an orbital period of 5.58 years. [1] Lexell also noted that, despite this short-period orbit, by far the shortest known at the time, the comet was unlikely to have been seen previously because its orbit had been radically altered in March 1767 by the gravitational forces of Jupiter. [17] It is, therefore, the earliest identified Jupiter family comet (as well as the first known near-Earth object). [18]

    After conducting further work in cooperation with Pierre-Simon Laplace, Lexell argued that a subsequent interaction with Jupiter in July 1779 [19] had further perturbed its orbit, either placing it too far from Earth to be seen or perhaps ejecting it from the Solar System altogether. [20] The comet likely no longer approaches any closer to the Sun than Jupiter's orbit. [21] [18]

    Although Comet Lexell was never seen again, it remained interesting to astronomers. The Paris Academy of Sciences offered a prize for an investigation into the orbit of the comet. Johann Karl Burckhardt won in 1801, and confirmed the calculations of Lexell. He calculated that the 1779 close approach to Jupiter drastically altered its orbit and left it with a perihelion of 3.33 AU. [22] In the 1840s, Urbain Le Verrier carried out further work on the comet's orbit and demonstrated that despite potentially approaching Jupiter as close as three and a half radii from the planet's centre the comet could never have become a satellite of Jupiter. [20] He showed that after the second encounter with Jupiter many different trajectories were possible, given the uncertainties of the observations, and the comet could even have been ejected from the Solar System. This foreshadowed the modern scientific idea of chaos. [20]

    Lexell's work on the orbit of the comet is considered to be the beginning of modern understanding of orbit determination. [23]

    2018 recalculation

    In a 2018 paper, Quan-Zhi Ye et al. used recorded observations of the comet to recalculate the orbit, finding Le Verrier's 1844 calculations to be highly accurate. They simulated the orbit forwards to the year 2000, finding that 98% of possible orbits remained orbiting the Sun, 85% with a perihelion nearer than the asteroid belt, and 40% crossing Earth's orbit. The numbers remain consistent even when including non-gravitational parameters caused by pressures from a comet's jets. [2]

    Based on its apparent brightness in 1770, they estimate the comet to be between 4 and 50 kilometers in diameter, most likely less than 30. Additionally, based on a lack of meteor showers, they suggest that the comet may have ceased major activity before 1800. [2]

    Identification

    The aforementioned 2018 paper also attempted to identify if any discovered object may be a remnant of Lexell's comet. With an assumed size of >4 kilometers, it is highly unlikely that this comet would remain in the inner solar system and be undiscovered. Most new asteroids discovered even in the asteroid belt (as of 2018) are only 1–4 kilometers across. If Lexell's comet remains in the inner Solar System, it would most likely be an unidentified asteroid. The paper identified four potential asteroids which could be related: (529668) 2010 JL33 (99.2% chance), 1999 XK136 (74% chance), 2011 LJ1 (0.2% chance), and 2001 YV3 (~0% chance). [2] The longitude of perihelion (a value that does not evolve much even over an extended period of time) of these asteroids are 2.32°, 6.22°, 356.98°, and 351.62°, respectively. For comparison, the longitude of perihelion of Lexell's comet was 359.48 ± 0.24°. [2]

    They find that 2010 JL33 is very likely to be a remnant of Lexell's comet, although due to a number of close approaches with Jupiter as well as uncertain non-gravitational parameters, a definite link cannot be made. [2] 2010 JL33 will pass about 0.0227  AU (3.4 million  km ) from Venus on November 3, 2184. [4]

    See also

    Notes

    1. ↑ Other comets named after their orbit computer, rather than discoverer, are 27P/Crommelin, 2P/Encke and 1P/Halley – Halley's Comet.

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    References

    1. 1 2 3 4 5 6 Kronk, G. Cometography: D/1770 L1 (Lexell) , accessed November 20, 2008.
    2. 1 2 3 4 5 6 7 Ye, Quan-Zhi; Wiegert, Paul A.; Hui, Man-To (February 24, 2018). "Finding Long Lost Lexell's Comet: The Fate of the First Discovered Near-Earth Object". The Astronomical Journal. 155 (4): 163. arXiv: 1802.08904 . Bibcode:2018AJ....155..163Y. doi: 10.3847/1538-3881/aab1f6 . S2CID   118895688.
    3. 1 2 3 4 "529668 (2010 JL33)". Minor Planet Center. Retrieved August 18, 2022.
    4. 1 2 3 "JPL Small-Body Database Browser: 529668 (2010 JL33)" (March 4, 2020 last obs.). Jet Propulsion Laboratory . Retrieved August 18, 2022.
    5. ↑ "ALCDEF: Asteroid Photometry Database". alcdef. Retrieved November 24, 2019.
    6. 1 2 Mainzer, A.; Grav, T.; Bauer, J.; Masiero, J.; McMillan, R. S.; Cutri, R. M.; et al. (December 2011). "NEOWISE Observations of Near-Earth Objects: Preliminary Results". The Astrophysical Journal. 743 (2): 17. arXiv: 1109.6400 . Bibcode:2011ApJ...743..156M. doi:10.1088/0004-637X/743/2/156. S2CID   239991.
    7. ↑ Blaauw, Rhiannon C.; Cooke, William, J.; Suggs, Robert M. (July 2011). "Lightcurve Analysis of Asteroids 890 Waltraut and 2010 JL33". The Minor Planet Bulletin. 38 (3): 131. Bibcode:2011MPBu...38..131B.{{cite journal}}: CS1 maint: multiple names: authors list (link)
    8. ↑ Kronk, G. The Closest Approaches of Comets to Earth , accessed November 20, 20, 2008. It was thought that C/1491 B1 may have approached even closer on February 20, 1491, but its orbit was retracted in 2002 due to a misunderstanding of the records. See Approximate Orbits of Ancient and Medieval Comets: 3. Remarks and Discussion
    9. 1 2 3 "Closest Approaches to the Earth by Comets". Minor Planet Center. Retrieved January 10, 2018.
    10. ↑ "JPL Close-Approach Data: P/1999 J6 (SOHO)" (2010-04-22 last obs (arc=10.9 yr; JFC)). Retrieved June 28, 2012.
    11. ↑ "Horizons Batch for P/1999 J6 on 1999-Jun-12". JPL Horizons . Retrieved August 29, 2022.
    12. ↑ Sekanina, Zdenek; Chodas, Paul W. (December 2005). "Origin of the Marsden and Kracht Groups of Sunskirting Comets. I. Association with Comet 96P/Machholz and Its Interplanetary Complex" (PDF). The Astrophysical Journal Supplement Series. 151 (2): 551–586. Bibcode:2005ApJS..161..551S. doi:10.1086/497374. S2CID   85442034. Archived from the original (PDF) on December 16, 2018. Retrieved January 11, 2018.
    13. ↑ Hall, John. (1955). Tanuma Okitsugu, 1719–1788, p. 120.
    14. ↑ Daḥlan, Aḥmad Zaynī (2007) [1887/1888]. Khulāṣat al-kalām fī bayān umarā' al-Balad al-Ḥarāmخلاصة الكلام في بيان أمراء البلد الحرام (in Arabic). Dār Arḍ al-Ḥaramayn. pp. 274–276.
    15. ↑ Scheltema, J. F. (1917). "Arabs and Turks". Journal of the American Oriental Society. 37. New Haven, Connecticut: Yale University Press: 156. doi:10.2307/592912. JSTOR   592912.
    16. ↑ Tofigh Heidarzadeh (2008). A History of Physical Theories of Comets, From Aristotle to Whipple. Springer Science & Business Media. pp. 196–197. ISBN   978-1402083235.
    17. ↑ Leverington, D. Babylon to Voyager and Beyond: A History of Planetary Astronomy, Cambridge University Press, 2003, p. 193
    18. 1 2 Valsecchi, G. 'A comet heading towards Earth: the first NEO' Archived March 26, 2012, at the Wayback Machine , in Tumbling Stone , Issue 2, accessed November 21, 2008
    19. ↑ "Horizons Batch for the nominal (best-fit) Jupiter approach in July 1779". JPL Horizons . Retrieved August 25, 2022.
    20. 1 2 3 Valsecchi, G. 'Le Verrier's computations and the concept of Chaos' Archived March 26, 2012, at the Wayback Machine , in Tumbling Stone Archived March 26, 2012, at the Wayback Machine , Issue 3, accessed February 11, 2011
    21. ↑ "JPL Horizons Batch for Heliocentric Orbit July 1779 to October 1779". JPL Horizons On-Line Ephemeris System . Jet Propulsion Laboratory . Retrieved August 25, 2022. (Perihelion after July Jupiter approach is QR= 5E+00)
    22. ↑ Barnard, E. E. (January 25, 1890). "Probable Return of Lexell's Comet". Publications of the Astronomical Society of the Pacific. 2 (6): 21–24. Bibcode:1890PASP....2...21B. doi: 10.1086/120073 . Retrieved January 11, 2018.
    23. ↑ Valsecchi, G. '236 Years Ago...' in Near Earth Objects, Our Celestial Neighbors: Opportunity and Risk : Proceedings of the 236th Symposium of the International Astronomical Union, Cambridge University Press, 2006, xvii–xviii
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