Comet Zhu–Balam Explained

C/1997 L1 (Zhu-Balam)
Discoverer:David D. Balam (June 8) and Jin Zhu (June 3)
Discovery Date:June 3, 1997
Epoch:1997-Aug-22 (JD 2450682.5)
Eccentricity:0.9979
Perihelion:4.899 AU
Semimajor:~1100 AU
Aphelion:~2210 AU
Period:36,800 years (approx.)
Last P:November 22, 1996

Comet Zhu–Balam (C/1997 L1) is a long-period comet first identified by David D. Balam on June 8, 1997, and originally photographed by Jin Zhu on June 3, 1997.[1] [2] The comet is estimated at 10 kilometres in diameter[2] with a period of approximately 36,800 years.

Given the 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 2015-Jan-01 generate a semi-major axis of 1100 AU and a period of approximately 36,800 years.[3]

Notes and References

  1. Web site: New comet named after astronomers. November 13, 1998. Canadian Broadcasting Corporation. 1 February 2010.
  2. Web site: Sharp-eyed Balam co-discovers comet. McNeney. Mike. February 6, 1998. The Ring/University of Victoria. 1 February 2010 . https://web.archive.org/web/20041025100724/http://ring.uvic.ca/98feb06/Balam.html . 2004-10-25 .
  3. Web site: Horizons output . Barycentric Osculating Orbital Elements for Comet Zhu-Balam (C/1997 L1) . 2011-01-31. (Solution using the Solar System Barycenter and barycentric coordinates. Select Ephemeris Type:Elements and Center:@0)