Comet Burnham, formally designated as C/1959 Y1, is a hyperbolic comet that became visible to the naked eye in 1960.[5] It is one of six comets discovered by American astronomer, Robert Burnham, Jr.[2] It brightened up to a magnitude of 3.5.[6]

C/1959 Y1 (Burnham)
Comet Burnham photographed by Alan McClure on 22 April 1960.[1]
Discovery[2]
Discovered byRobert Burnham, Jr.
Discovery siteLowell Observatory
Discovery date30 December 1959
Designations
1959k[3]
1960 II
Orbital characteristics[4]
Epoch4 April 1960 (JD 2437028.5)
Observation arc148 days
Number of
observations
35
Perihelion0.5044 AU
Eccentricity1.00029
Inclination159.601°
252.643°
Argument of
periapsis
306.632°
Last perihelion20 March 1960
Earth MOID0.1947 AU
Jupiter MOID0.5355 AU
Physical characteristics[5]
Comet nuclear
magnitude (M2)
15.9
3.5
(1960 apparition)

Observational history

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The comet was discovered in a photographic plates obtained by the Lowell Observatory in Arizona as part of the Lowell Proper Motion Survey program on 29−30 December 1959. Robert Burnham Jr. noticed in one of them a fairly bright, diffuse trail. He estimated its apparent magnitude to be 11. The presence of the comet was confirmed by Lick Observatory on 1 and 2 January 1960, and by Lowell observatory on 2 January. Henry L. Giclas, Lowell observatory, estimated its magnitude to be 14. The comet then was three months before perihelion and 1.71 AU from the Sun.[7]

The comet appeared moderately condensed in images obtained in early January, but the central condensation became more pronounced by the end of the month. On 28 January Elizabeth Roemer reported that the comet has a coma 1.3' across, and two tails, one short, curved tail extending 3' long, and a narrow, straight tail 15' long. On 9 March the comet reached its minimum elongation, being 8 degrees from the Sun, and continued to move southwards until 21 March, reaching a declination of -13°. The perihelion of the comet was on 20 March 1960.[7]

The comet was recovered on 25 March in the morning twilight. Its magnitude was estimated visually by Roemer to be 7 on 4 April. In the start of April no tail was visible visually, but Alan McClure detected a very faint tail 3 degrees long in a photographic plate obtained in blue light. The comet was brightening as it was approaching Earth. On April 13 George van Biesbroeck estimated its magnitude to 5.3 and on April 18 to be 4.7. On April 22 the tail was reported to be 2.5° long visually and 7.4° in photographic plates exposed in blue light. The comet was reported to have reached an apparent magnitude of 3.5 on April 26. Closest approach took place on April 27, at a distance of 0.20 AU.[7]

After the perigee, the comet faded rapidly and on 1 May van Biesbroeck estimated its magnitude to be 4.8. On May 3 its photographic magnitude was estimated to be 6.5 by Arend, while a tail was also imaged. On May 14 the photographic magnitude had dropped to 10. The comet was last detected in images obtained on 17 June by Roemer at the US Naval Observatory. It was descripted as essentially stellar with a magnitude of 18.[7]

References

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  1. ^ D. D. Meisel (1962). "Comet Burnham 1959K: Final Report, Part IV, Supplementary Notes". Strolling Astronomer. 16 (7–8). Bibcode:1962StAst..16..154M.
  2. ^ a b J. M. Vinter Hansen (7 January 1960). "Comet Burnham (1959k)". Central Bureau for Astronomical Telegrams. 1706.
  3. ^ "Comet Names and Designations". International Comet Quarterly. Retrieved 4 December 2024.
  4. ^ "C/1959 Y1 (Burnham) – JPL Small-Body Database Lookup". ssd.jpl.nasa.gov. Jet Propulsion Laboratory. Retrieved 4 December 2024.
  5. ^ a b "Comet C/1959 Y1 (Burnham)". Comet Observation Database System (COBS). Retrieved 4 December 2024.
  6. ^ "Brightest comets seen since 1935". International Comet Quarterly. Retrieved 7 December 2024.
  7. ^ a b c d G. W. Kronk (2009). Cometography: A Catalog of Comets. Vol. 4: 1933–1959. Cambridge: Cambridge University Press. pp. 582–588. ISBN 978-0-521-58507-1.
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