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C/2007 N3 (Lulin)

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Not to be confused with 145523 Lulin.
For other uses, see Lulin (disambiguation).
C/2007 N3 (Lulin)
Comet Lulin as seen on January 31st (top) and February 4th of 2009.
Discovery[1][2][3]
Discovered byYe Quanzhi
Lin Chi-Sheng
Discovery site0.41-m Ritchey–Chrétien
Lulin Observatory (D35)
Discovery date11 July 2007
Designations
Comet Lulin
Orbital characteristics[4][5][6]
Epoch6 December 2008 (JD 2454806.5)
Aphelion~64000 AU (epoch 1800)
~2400 AU (epoch 2200)
Perihelion1.2122 AU
Semi-major axis1200 AU
Eccentricity0.99998 (near parabolic)
Orbital period42,000 yr (epoch 2200)
Inclination178.37°
Last perihelion10 January 2009[4]

Comet Lulin, formal designation C/2007 N3, Traditional Chinese:鹿林彗星) is a non-periodic comet. It was discovered by Ye Quanzhi and Lin Chi-Sheng from Lulin Observatory.[2][3][7] It peaked in brightness at magnitude between +4.5 and +5,[3][8][9][10] becoming visible to the naked eye,[11] and arrived at perigee for observers on Earth on February 24, 2009,[5] and at 0.411 AU (61,500,000 km; 38,200,000 mi) from Earth.[5]

Discovery

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The comet was first photographed by astronomer Lin Chi-Sheng (林啟生) with a 0.41-metre (16 in) telescope at the Lulin Observatory in Nantou, Taiwan on July 11, 2007. However, it was the 19-year-old Ye Quanzhi (葉泉志) from Sun Yat-sen University in China, who identified the new object from three of the photographs taken by Lin.[12]

Initially, the object was thought to be a magnitude 18.9 asteroid, but images taken a week after the discovery with a larger 0.61-metre (24 in) telescope revealed the presence of a faint coma.[2][1][12]

The discovery occurred as part of the Lulin Sky Survey project to identify small objects in the Solar System, particularly Near-Earth Objects. The comet was named "Comet Lulin" after the observatory, and its official designation is Comet C/2007 N3.[13]

Observations

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The comet became visible to the naked eye from dark-sky sites around February 7.[14] It figured near the double star Zubenelgenubi on February 6, near Spica on February 15 and 16, near Gamma Virginis on February 19 and near the star cluster M44 on March 5 and 6. It also figured near the planetary nebula NGC 2392 on March 14, and near the double star Wasat around March 17.[15][16] The comet was near conjunction with Saturn on February 23, and outward-first headed towards its aphelion, against the present position of background stars, in the direction of Regulus in the constellation of Leo, as noted on February 26 and 27, 2009.[3][7] It passed near Comet Cardinal on May 12, 2009.[17]

According to NASA, Comet Lulin's green color comes from a combination of gases that make up its local atmosphere, primarily diatomic carbon, which appears as a green glow when illuminated by sunlight in the vacuum of space. When SWIFT observed comet Lulin on 28 January 2009; the comet was shedding nearly 3,000 litres (800 US gal) of water each second.[18] Comet Lulin was methanol-rich.

Orbit

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Astronomer Brian Marsden of the Smithsonian Astrophysical Observatory calculated that Comet Lulin reached its perihelion on January 10, 2009, at a distance of 113 million miles (182 million kilometers) from the Sun.

The orbit of Comet Lulin is very nearly a parabola (parabolic trajectory), according to Marsden.[13] The comet had an epoch 2009 eccentricity of 0.999986,[4] and has an epoch 2010 eccentricity of 0.999998.[4] It is moving in a retrograde orbit at a very low inclination of just 1.6° from the ecliptic.[13]

Given the extreme orbital eccentricity of this object, different epochs can generate quite different heliocentric unperturbed two-body best fit solutions to the aphelion distance (maximum distance) of this object. For objects at such high eccentricity, the sun's barycentric coordinates are more stable than heliocentric coordinates. Using JPL Horizons, the barycentric orbital elements for epoch 2014-Jan-01 generate a semi-major axis of about 1200 AU and a period of about 42,000 years.[6]

Disconnected tail

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On February 4, 2009, a team of Italian astronomers witnessed "an intriguing phenomenon in Comet Lulin's tail". Team leader Ernesto Guido explains: "We photographed the comet using a remotely controlled telescope in New Mexico, and our images clearly showed a disconnection event. While we were looking, part of the comet's plasma tail was torn away."[19]

Guido and colleagues believe the event was caused by a magnetic disturbance in the solar wind hitting the comet. Magnetic mini-storms in comet tails have been observed before—most famously in 2007, when NASA's STEREO spacecraft watched a coronal mass ejection crash into Comet Encke. Encke lost its tail in dramatic fashion, much as Comet Lulin did on February 4.[19]

See also

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References

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  1. ^ a b "MPEC 2007-O05: COMET C/2007 N3 (LULIN)". Minor Planet Electronic Circular. Minor Planet Center. 18 July 2007. Retrieved 5 July 2011.
  2. ^ a b c Kronk, Gary W. "C/2007 N3 (Lulin)". cometography.com. Archived from the original on 2012-03-06. Retrieved 2009-01-02.
  3. ^ a b c d Yoshida, Seiichi (December 31, 2008). "C/2007 N3 ( Lulin )". aerith.net. Retrieved 2009-01-02.
  4. ^ a b c d "C/2007 N3 (Lulin) Orbital Elements". IAU Minor Planet Center. Archived from the original on 2016-01-26. Retrieved 2011-05-26.
  5. ^ a b c "C/2007 N3 (Lulin) – JPL Small-Body Database Lookup". ssd.jpl.nasa.gov. Jet Propulsion Laboratory. Retrieved 23 March 2010.
  6. ^ a b Horizons output. "Barycentric Osculating Orbital Elements for Comet Lulin (C/2007 N3)". Retrieved 20 January 2011. (Solution using the Solar System Barycenter. Select Ephemeris Type:Elements and Center:@0)
  7. ^ a b Dyer, Alan (2009). "Venus Kicks Off the Year of Astronomy (pg. 24-27)". In Dickinson, Terence (ed.). SkyNews: The Canadian Magazine of Astronomy & Stargazing. Vol. XIV, Issue 5 (January/February 2009 ed.). Yarker, Ontario: SkyNews Inc. p. 38.
  8. ^ Reinder J. Bouma and Edwin van Dijk. "C/2007 N3 (Lulin) magnitude estimates". Astrosite Groningen. Retrieved 2009-03-17.
  9. ^ "Recent Comet Brightness Estimates". ICQ/CBAT/MPC. International Comet Quarterly. Retrieved 2009-02-24.
  10. ^ McRobert, Alan; Bryant, Greg (February 23, 2009). "Observing Highlights - Catch Comet Lulin at Its Best!". Sky & Telescope. SkyandTelescope.com. Archived from the original on January 10, 2009. Retrieved 2009-02-24.
  11. ^ "Comet C/2007 N3 (Lulin) observation list". cobs.si. Comet OBServation database. Archived from the original on 31 January 2023. Retrieved 31 January 2023.
  12. ^ a b "IAUC 8857: C/2007 N3; S/2007 S 4". IAU Central Bureau for Astronomical Telegrams. 2007-07-18. Archived from the original on 2012-03-27. Retrieved 2011-06-03.
  13. ^ a b c "Newfound Comet Lulin to Grace Night Skies". space.com. Retrieved 2009-02-09.
  14. ^ "Naked-Eye Comet". spaceweather.com. Retrieved 2009-02-07.
  15. ^ "Path of Comet C/2007 N3 (Lulin), Mar. 1 - 20, 2009" (PDF). Sky and Telescope. Archived from the original (PDF) on 2009-03-24. Retrieved 2009-03-16.
  16. ^ McRobert, Alan M. "This Week's Sky at a Glance". Sky and Telescope. Archived from the original on 2009-03-18. Retrieved 2009-03-16.
  17. ^ Dyer, Alan (2009). "The Top 10 Celestial Sights of 2009 (pg. 14)". In Dickinson, Terence (ed.). SkyNews: The Canadian Magazine of Astronomy & Stargazing. Vol. XIV, Issue 5 (January/February 2009 ed.). Yarker, Ontario: SkyNews Inc. p. 38.
  18. ^ "NASA's Swift Spies Comet Lulin". NASA. 2009-02-20. Retrieved 2013-08-03.
  19. ^ a b "DISCONNECTED TAIL". spaceweather.com. Retrieved 2009-02-09.
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