|Discovered by||Caroline Herschel & Roger Rigollet|
|Discovery date||1788-12-21 & 1939-07-28|
|35P/1788 Y1, 1788II Herschel;|
1939 O1, 1939 IX
|Orbital characteristics A|
|Semi-major axis||28.843 AU|
|Orbital period||155 yr|
|Next perihelion||2092-Feb-13 (MPC)|
2092 Mar. 16
35P/Herschel-Rigollet is a periodic comet with an orbital period of 155 years. It fits the classical definition of a Halley-type comet with (20 years < period < 200 years). It was discovered by Caroline Herschel (Slough, United Kingdom) on 1788-12-21. Given that the comet takes 155 years to orbit the Sun, predictions for the next perihelion passage in 2092 vary by about a month.
Caroline Herschel first observed the comet on 21 December 1788 and it was observed later that night by her brother William Herschel who described it as looking like a bright nebula and about 5-6 minutes in diameter, and much larger than the planetary nebula M57.
Through December and January the comet was observed by Nevil Maskelyne at the Greenwich Observatory and by Charles Messier at the Paris Observatory. Maskelyne was the last observer of the comet, his final observation taking place on 1789-02-05.
Similar possible orbits for the comet were calculated in 1789 by Pierre Méchain and in 1922 by Margaretta Palmer. Palmer considered that the orbit which best fitted the observations was an elliptical one with a period of 1,066 years.
Roger Rigollet (Lagny, France) rediscovered the comet on 1939-07-28; it was described as diffuse and with a magnitude of 8.0. The sighting was confirmed the next day by Alfonso Fresa of the Observatory of Turin (Italy) and George van Biesbroeck of the Yerkes Observatory. The comet steadily faded after August, final (photographic) observations being obtained on 1940-01-16.
Following the 1939 rediscovery, the comet's orbit was calculated by Jens P. Möller (Copenhagen, Denmark), and Katherine P. Kaster and Thomas Bartlett (Berkeley, USA). A perihelion date of 1939-08-09 was indicated. Based on these early orbits, Leland E. Cunningham of the Harvard College Observatory suggested that the comet was likely identical with Herschel's comet of 1788.
The final calculation of the orbit, by Brian G. Marsden in 1974, used 75 positions from both apparitions of the comet in 1788 and 1939-40 in addition to perturbations by planets, and linked the two sightings, with a perihelion date of 1939-08-09 and a period of 155 years.