| Minorplanet: | yes |
| 1940 Whipple | |
| Background: |
|
| Discovered: | 2 February 1975 |
| Mpc Name: | (1940) Whipple |
| Alt Names: | 1975 CA1932 AD 1950 LH1962 SH 1971 KNA916 AD |
| Named After: | Fred L. Whipple |
| Epoch: | 4 September 2017 (JD 2458000.5) |
| Uncertainty: | 0 |
| Observation Arc: | 54.50 yr (19,907 days) |
| Perihelion: | 2.8656 AU |
| Semimajor: | 3.0606 AU |
| Eccentricity: | 0.0637 |
| Period: | 5.35 yr (1,956 days) |
| Mean Motion: | / day |
| Inclination: | 6.5587° |
| Asc Node: | 263.80° |
| Arg Peri: | 179.82° |
| Mean Diameter: | km 33.83 km km km km km |
| Rotation: | h |
| Albedo: | 0.0560 |
| Abs Magnitude: | 11.011.1 |
1940 Whipple (prov. designation:) is a carbonaceous background asteroid from the outer region of the asteroid belt, approximately 35km (22miles) in diameter. It was discovered on 2 February 1975, by the Harvard College Observatory at its George R. Agassiz Station near Harvard, Massachusetts, in the United States, and named after astronomer Fred Whipple.
Whipple orbits the Sun in the outer main-belt at a distance of 2.9–3.3 AU once every 5 years and 4 months (1,956 days). Its orbit has an eccentricity of 0.06 and an inclination of 7° with respect to the ecliptic. The first used observation was made at Goethe Link Observatory in 1962, extending the asteroid's observation arc by 13 years prior to its discovery observation.
This minor planet was named after American astronomer Fred Lawrence Whipple (1906–2004), author of the icy conglomerate model, also known as the dirty snowball hypothesis.
Whipple worked at the Harvard College Observatory for over 70 years and was the director of the Smithsonian Astrophysical Observatory where he developed new methods imaging meteors. He was also president of several commissions at the International Astronomical Union and on NASA's panel for missions to small Solar System bodies. The official was published by the Minor Planet Center on 1 June 1975 .
Whipple has been characterized as a carbonaceous C-type asteroid by Pan-STARRS photometric survey.
According to the surveys carried out by the Infrared Astronomical Satellite IRAS, the Japanese Akari satellite, and NASA's Wide-field Infrared Survey Explorer with its subsequent NEOWISE mission, the asteroid measures between 32.6 and 40.4 kilometers in diameter and its surface has a low albedo between 0.04 and 0.06. The Collaborative Asteroid Lightcurve Link derives an albedo of 0.056 and a diameter of 33.8 kilometers using an absolute magnitude of 11.1.
In December 2011, a rotational lightcurve was obtained for this asteroid from photometric observations by American astronomer Russel Durkee at the Shed of Science Observatory . It gave a well-defined rotation period of hours with a brightness variation of 0.25 magnitude, superseding a period of hours previously obtained by French astronomer René Roy in 2005 .