C/2014 Q2 (Lovejoy)

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C/2014 Q2 (Lovejoy) is a long-period comet discovered on 17 August 2014 by Terry Lovejoy using a 0.2-meter (8 in) Schmidt–Cassegrain telescope.[2] It was discovered at apparent magnitude 15 in the southern constellation of Puppis.[2] It is the fifth comet discovered by Terry Lovejoy. Its blue-green glow is the result of organic molecules and water released by the comet fluorescing under the harsh UV and optical light of the sun as it passes through space.[5][6]

History

By December 2014, the comet had brightened to roughly magnitude 7.4,[7] making it a small telescope and binoculars target. By mid-December, the comet was visible to the naked eye for experienced observers with dark skies and keen eyesight.[8] On 28−29 December 2014, the comet passed 1/3° from globular cluster Messier 79.[9] In January 2015, it brightened to roughly magnitude 4,[10] and became one of the brightest comets located high in a dark sky since comet C/1995 O1 (Hale-Bopp) in 1997. On 7 January 2015, the comet passed Lua error in Module:Convert at line 1851: attempt to index local 'en_value' (a nil value). from Earth.[11] It crossed the celestial equator on 9 January 2015 becoming better seen from the Northern Hemisphere.[12] The comet came to perihelion (closest approach to the Sun) on 30 January 2015 at a distance of Lua error in Module:Convert at line 1851: attempt to index local 'en_value' (a nil value). from the Sun.[3] At perihelion, its water production rate exceeded 20 metric tons per second.[5]

C/2014 Q2 originated from the Oort cloud,[5] but is not a dynamically new comet.[13] Before entering the planetary region (epoch 1950), C/2014 Q2 had an orbital period of about 11000 years with aphelion about Lua error in Module:Convert at line 1851: attempt to index local 'en_value' (a nil value). from the Sun.[4] After leaving the planetary region (epoch 2050), it will have an orbital period of about 8000 years with aphelion of about 800 AU.[4]

The comet was observed to release 21 different organic molecules in gas, including ethanol and glycolaldehyde, a simple sugar.[5][14] The presence of organic molecules suggests that they are preserved materials synthesized in the outskirts of the solar nebula or at earlier stages of the Solar System formation.[5]

Gallery

References

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External links

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