Copyrightę1997 by A. Nakamura
This CCD image was taken by Akimasa Nakamura (Kuma Kogen Astronomical Observatory, Japan) on 1997 May 31.71, using a 0.60-m f/6 Ritchey-Chretien telescope.
E. L. Johnson (Johannesburg, South Africa) discovered this comet with the 25-cm Franklin-Adams Star Camera on 1949 August 24.90, while making follow-up observations of the new minor planet 1949 OG. He determined the magnitude as 13.8 and described the comet as very small, diffuse, and without a central condensation. He confirmed the comet on August 25.80 and then found prediscovery images on plates exposed on August 15.81 and August 20.82.
The comet was already passed its closest approach to Earth when discovered, having passed 1.26 AU away on August 3. Subsequently, the comet's brightness was virtually unchanged during the coming weeks as it headed for its September 16 perihelion passage. Johnson remained the most prolific observer of this comet. He reported a magnitude of 14.5 on October 16 and upon making the final observation of the comet on November 19.8 he estimated the magnitude as 15.5.
The comet was first identified as periodic during 1949 September, after less than a month's observations had been obtained. W. P. Hirst was the first to publish such an orbit, which indicated an orbital period of 7.01 years. During mid-month Nevin Sherman (Student's Observatory, Berkeley, California, USA) had computed a very similar orbit with an orbital period of 7.01 years. Sherman said his orbit indicated a possible close approach to Jupiter in 1932. Revised orbits followed during the next few months and it was eventually learned that the orbital period was 6.86 years. Latter investigations revealed the comet was moving in a very stable orbit and that no moderate approach to Jupiter had occurred since 1706 (0.42 AU).
During 1955, W. H. Julian and B. O. Wheel worked out the details of this comet's upcoming apparition and predicted it would arrive at perihelion on 1956 July 24.22. They commented that the comet would be "well placed for observation in the Southern Hemisphere during all except the beginning of the year." Jacobus Albertus Bruwer (Union Observatory Annexe, Hartbeespoort, South Africa) recovered the comet with the 25-cm Franklin-Adams Star Camera on 1956 August 6.94. He estimated the magnitude as 13.5. The position indicated the prediction by Julian and Wheel needed corrected by +2.4 days.
The comet has been seen at every return since its discovery. The perihelion distance of 2.2 to 2.3 AU prevents it from coming closer to 1.2 to 1.3 AU from out planet. Subsequently, the comet never becomes especially brighter and usually experiences a relatively slow brightening and fading as it approaches perihelion. Following the discovery apparition, the comet experienced another very favorable return in 1956 and attained a maximum magnitude of 13 around the time it passed closest to Earth (1.28 AU) on August 22. Conditions were less favorable in 1963 and the comet's maximum reported magnitude was 17, with the closest approach to Earth being 1.38 AU on September 11. Still more unfavorable conditions existed during the 1970 return with the closest approach to Earth being 1.65 AU on October 8. The maximum reported magnitude was only 18.8.
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