| Minorplanet: | yes |
| 1780 Kippes | |
| Background: |
|
| Discovered: | 12 September 1906 |
| Mpc Name: | (1780) Kippes |
| Alt Names: | A906 RA1935 CC 1943 TL 1943 VD1947 NB 1953 SA 1957 LD1962 JU A911 QE |
| Named After: | Otto Kippes |
| Epoch: | 4 September 2017 (JD 2458000.5) |
| Uncertainty: | 0 |
| Observation Arc: | 110.38 yr (40,315 days) |
| Perihelion: | 2.8538 AU |
| Semimajor: | 3.0165 AU |
| Eccentricity: | 0.0539 |
| Period: | 5.24 yr (1,914 days) |
| Mean Motion: | / day |
| Inclination: | 9.0022° |
| Asc Node: | 290.98° |
| Arg Peri: | 340.31° |
| Dimensions: | km km km km km |
| Albedo: | |
| Spectral Type: | S |
| Abs Magnitude: | 10.68 |
1780 Kippes, provisional designation, is an Eoan asteroid from the outer regions of the asteroid belt, approximately 28 kilometers in diameter. It was discovered on 12 September 1906, by astronomer August Kopff at the Heidelberg-Königstuhl State Observatory in southwest Germany. The asteroid was named after German Catholic priest and amateur astronomer Otto Kippes.
Kippes is a member the Eos family, the largest asteroid family of the outer main belt consisting of nearly 10,000 asteroids. It orbits the Sun in the outer main-belt at a distance of 2.9–3.2 AU once every 5 years and 3 months (1,914 days). Its orbit has an eccentricity of 0.05 and an inclination of 9° with respect to the ecliptic.
The body's observation arc begins at Heidelberg in 1906, one week after its official discovery observation.
Kippes is an assumed S-type asteroid, while the overall spectral type of the Eos family is that of a K-type.
In July 1984, a rotational lightcurve of Kippes was obtained from photometric observations by astronomer Richard P. Binzel at the CTIO and McDonald Observatory. Lightcurve analysis gave a rotation period of 18.0 hours with a brightness amplitude of 0.23 magnitude .
According to the surveys carried out by the Infrared Astronomical Satellite IRAS, the Japanese Akari satellite and the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer, Kippes measures between 25.77 and 31.262 kilometers in diameter and its surface has an albedo between 0.0966 and 0.143.
The Collaborative Asteroid Lightcurve Link adopts the results obtained by IRAS, that is, an albedo of 0.1212 and a diameter of 27.92 kilometers based on an absolute magnitude of 10.68.
This minor planet was named after German Catholic priest and amateur astronomer Otto Kippes (1905–1994). He was a precise observer, acknowledged for his orbit calculations and identifications of hundreds of minor planets in widely separated oppositions. The official was published by the Minor Planet Center on 15 June 1973 .