 Comet NEAT andMessier 44 photographed by Oliver Stein on 16 May 2004 | |
| Discovery | |
|---|---|
| Discovered by | NEAT |
| Discovery date | 24 August 2001 |
| Orbital characteristics[1][2] | |
| Epoch | 15 May 2004 (JD 2453140.5) |
| Observation arc | 1,811 days (4.96 years) |
| Number of observations | 2,617 |
| Perihelion | 0.962 AU |
| Eccentricity | 1.00069 (inbound) 1.00067 (outbound) |
| Inclination | 99.643° |
| 210.28° | |
| Argument of periapsis | 1.204° |
| Mean anomaly | –0.000018° |
| Last perihelion | 15 May 2004 |
| EarthMOID | 0.043 AU |
| JupiterMOID | 4.279 AU |
| Physical characteristics[3][4] | |
| Dimensions | 3.6–7.2 km (2.2–4.5 mi) |
Mean diameter | 5.4 km (3.4 mi) |
| Mass | 1.1×1013 kg |
| Comet total magnitude (M1) | 8.0 |
C/2001 Q4 (NEAT) is acomet with an almost perpendicularretrograde orbit which brings it into the innerSolar System by a deeply southward path.[2] It initially emerged from its remote home spending most of its time near the south celestial pole. This comet was discovered on August 24, 2001 by theNear-Earth Asteroid Tracking program (NEAT).
In 2004, residents of the southern hemisphere had the opportunity to watch the comet gradually brighten as it raced towardperihelion. On May 6, 2004 the comet approached within 0.32AU of the Earth.[2] Beginning in early May, the comet started racing north and burst into view in the northern hemisphere when it had reached almost maximum brightness.
With a near perihelionorbital eccentricity of 1.00069 (epoch 2004-May-18)[2] that keeps abarycentric epoch 2014-Jan-01 eccentricity of 1.00067,[1] thishyperbolic comet is going to be ejected from the Solar System.
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