Discovery date July 11, 2007 Semi-major axis 1200 AU Orbital period 42,000 years Discovered 11 July 2007 Epoch 6 December 2008 | Alternative
designations Comet Lulin Inclination 178.37° Aphelion 2,400 m Last perihelion 10 January 2009 Discoverers Ye Quanzhi, Chi-Sheng Lin | |
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Discovered by Ye Quanzhi, Lin Chi-Sheng
0.41-m Ritchey-Chretien (D35) Eccentricity 0.99998 (near parabolic) Similar Comet Holmes, Solar System, Comet Machholz, C/2006 P1, C/2001 Q4 (NEAT) | ||
Comet Lulin (official designation C/2007 N3 (Lulin), Traditional Chinese:鹿林彗星) is a non-periodic comet. It was discovered by Ye Quanzhi and Lin Chi-Sheng from Lulin Observatory. It peaked in brightness and arrived at perigee for observers on Earth on February 24, 2009, at magnitude +5, and at 0.411 AU from Earth. The comet was near conjunction with Saturn on February 23, and passed near Regulus in the constellation of Leo on February 26 and 27, 2009. It was expected to pass near Comet Cardinal on May 12, 2009. The comet became visible to the naked eye from dark-sky sites around February 7. It passed 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 passed near the planetary nebula NGC 2392 on March 14, and near the double star Wasat around March 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 800 gallons (approximately 3028 liters) of water each second. Comet Lulin was methanol-rich.
Contents
- February 2009 comet lulin s tail terminates disconnects first visit to inner solar system
- Discovery
- Orbit
- Disconnected tail
- References
February 2009 comet lulin s tail terminates disconnects first visit to inner solar system
Discovery
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.
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.
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.
Orbit
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. The comet had an epoch 2009 eccentricity of 0.999986, and has an epoch 2010 eccentricity of 0.999998. It is moving in a retrograde orbit at a very low inclination of just 1.6° from the ecliptic.
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 Suns 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.
Disconnected tail
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."
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.