| Minorplanet: | yes |
| 1015 Christa | |
| Background: |
|
| Discovered: | 31 January 1924 |
| Mpc Name: | (1015) Christa |
| Alt Names: | 1924 QFA916 UE |
| Named After: | unknown |
| Epoch: | 23 March 2018 (JD 2458200.5) |
| Uncertainty: | 0 |
| Observation Arc: | 93.42 yr (34,123 d) |
| Perihelion: | 2.9262 AU |
| Semimajor: | 3.2055 AU |
| Eccentricity: | 0.0871 |
| Period: | 5.74 yr (2,096 d) |
| Mean Motion: | / day |
| Inclination: | 9.4449° |
| Asc Node: | 120.15° |
| Arg Peri: | 286.50° |
| Mean Diameter: | km km km km km km |
| Rotation: | h |
| Albedo: | |
| Spectral Type: | Tholen C SMASS XcP B–V 0.693 U–B 0.320 |
| Abs Magnitude: | 9.03 9.13 |
1015 Christa, provisional designation, is a dark background asteroid from the outermost regions of the asteroid belt, approximately 96abbr=offNaNabbr=off in diameter. It was discovered on 31 January 1924, by German astronomer Karl Reinmuth at the Heidelberg-Königstuhl State Observatory in southwest Germany. The meaning of this asteroids's name is unknown.
Christa is a non-family asteroid from the main belt's background population. It orbits the Sun in the outermost asteroid belt at a distance of 2.9–3.5 AU once every 5 years and 9 months (2,096 days; semi-major axis of 3.21 AU). Its orbit has an eccentricity of 0.09 and an inclination of 9° with respect to the ecliptic.
The asteroid was first observed as at the Simeiz Observatory in October 1916. The body's observation arc begins at Heidelberg in February 1924, two days after its official discovery observation.
In the Tholen classification, Christa is a common C-type asteroid, while in the SMASS classification, it is a Xc-subtype that transitions from the carbonaceous C-type to the X-type asteroids. It has also been characterized as a primitive P-type asteroid by the Wide-field Infrared Survey Explorer (WISE).
In April 2005, a first rotational lightcurve of Christa was obtained from photometric observations by French amateur astronomers Raymond Poncy and René Roy. Lightcurve analysis gave a rotation period of 12.189 hours with a brightness variation of 0.20 magnitude . In January 2009, a refined period of 11.230 hours and an amplitude of 0.12 magnitude was measured by photometrist Brian Warner at his Palmer Divide Observatory in Colorado, United States .
According to the surveys carried out by the Infrared Astronomical Satellite IRAS, the Japanese Akari satellite and the NEOWISE mission of NASA's WISE telescope, Christa measures between 82.35 and 101.04 kilometers in diameter and its surface has a low albedo between 0.04 and 0.064. The Collaborative Asteroid Lightcurve Link adopts the results obtained by IRAS, that is, an albedo of 0.0459 with a diameter of 96.94 kilometers based on an absolute magnitude of 9.03.
1015 Christa has been observed to occult 8 stars between 2005 and 2023.
Any reference of this minor planet's name to a person or occurrence is unknown.
Among the many thousands of named minor planets, Christa is one of 120 asteroids, for which no official naming citation has been published. All of these low-numbered asteroids have numbers between and and were discovered between 1876 and the 1930s, predominantly by astronomers Auguste Charlois, Johann Palisa, Max Wolf and Karl Reinmuth.