C/2001 Q4 (NEAT)

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C/2001 Q4 (NEAT)
Comet-Neat-Messier-44 log.jpg
Comet NEAT and Messier 44 photographed by Oliver Stein on 16 May 2004
Discovery
Discovered by NEAT
Discovery date24 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 perihelion15 May 2004
Earth MOID 0.043 AU
Jupiter MOID 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 a comet with an almost perpendicular retrograde orbit which brings it into the inner Solar 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 the Near-Earth Asteroid Tracking program (NEAT).

Contents

In 2004, residents of the southern hemisphere had the opportunity to watch the comet gradually brighten as it raced toward perihelion. On May 6, 2004 the comet approached within 0.32 AU 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 perihelion orbital eccentricity of 1.00069 (epoch 2004-May-18) [2] that keeps a barycentric epoch 2014-Jan-01 eccentricity of 1.00067, [1] this hyperbolic comet is going to be ejected from the Solar System.

References

  1. 1 2 Horizons output. "Barycentric Osculating Orbital Elements for Comet C/2001 Q4 (NEAT)" . Retrieved 10 March 2011. (Solution using the Solar System Barycenter and barycentric coordinates. Select Ephemeris Type:Elements and Center:@0)
  2. 1 2 3 4 "C/2001 Q4 (NEAT) – JPL Small-Body Database Lookup". ssd.jpl.nasa.gov. Jet Propulsion Laboratory . Retrieved 11 March 2011.
  3. A. Sosa; J. A. Fernández (2011). "Masses of long-period comets derived from non-gravitational effects" (PDF). Monthly Notices of the Royal Astronomical Society. 416 (1): 767–782. doi: 10.1111/j.1365-2966.2011.19111.x .
  4. D. C. Jewitt (2022). "Destruction of Long-period Comets". Astronomical Journal. 164 (4): 158–166. arXiv: 2208.04469 . Bibcode:2022AJ....164..158J. doi: 10.3847/1538-3881/ac886d .