| Minorplanet: | yes |
| 1455 Mitchella | |
| Background: |
|
| Discovered: | 5 June 1937 |
| Mpc Name: | (1455) Mitchella |
| Alt Names: | 1937 LF1947 LB |
| Named After: | Maria Mitchell |
| Epoch: | 4 September 2017 (JD 2458000.5) |
| Uncertainty: | 0 |
| Observation Arc: | 79.81 yr (29,152 days) |
| Perihelion: | 1.9665 AU |
| Semimajor: | 2.2469 AU |
| Eccentricity: | 0.1248 |
| Period: | 3.37 yr (1,230 days) |
| Mean Motion: | / day |
| Inclination: | 7.7548° |
| Asc Node: | 128.33° |
| Arg Peri: | 100.60° |
| Dimensions: | km km km km 7.47 km |
| Albedo: | 0.24 |
| Abs Magnitude: | 12.712.8013.03 |
1455 Mitchella, provisional designation, is a Florian asteroid, slow rotator and suspected tumbler from the inner regions of the asteroid belt, approximately 7 kilometers in diameter. It was discovered on 5 June 1937, by astronomer Alfred Bohrmann at the Heidelberg-Königstuhl State Observatory in southwest Germany. The asteroid was named after American astronomer Maria Mitchell.
Mitchella is a non-family asteroid of the main belt's background population when applying the Hierarchical Clustering Method to its proper orbital elements. It has also been classified as a member of the Flora family, a giant asteroid family and the largest family of stony asteroids in the main-belt.
It orbits the Sun in the inner main-belt at a distance of 2.0–2.5 AU once every 3 years and 4 months (1,230 days). Its orbit has an eccentricity of 0.12 and an inclination of 8° with respect to the ecliptic. The body's observation arc begins at Heidelberg, one month after its official discovery observation.
Mitchella is an assumed stony S-type asteroid, which is also the overall spectral type for members of the Flora family.
In June 2006, a rotational lightcurve of Mitchella was obtained from photometric observations by Australian astronomer David Higgins at the Hunters Hill Observatory . Lightcurve analysis gave a rotation period of 118.7 hours with a brightness variation of 0.60 magnitude . With a period above 100 hours, Mitchella is one of few hundred slow rotators currently known to exists. Its high brightness amplitude is indicative for a somewhat elongated shape. Also, the photometric observations suggested that it might be in a tumbling motion.
According to the survey carried out by the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer, Mitchella measures between 6.449 and 7.00 kilometers in diameter and its surface has an albedo between 0.26 and 0.353.
The Collaborative Asteroid Lightcurve Link assumes an albedo of 0.24 – derived from 8 Flora, the Flora family's parent body – and calculates a diameter of 7.47 kilometers based on an absolute magnitude of 12.8.
This minor planet was named after Maria Mitchell (1818–1889), an American professor of astronomy and director of Vassar College Observatory. The official naming citation was mentioned in The Names of the Minor Planets by Paul Herget in 1955 . The lunar crater Mitchell is also named in her honor, as is the Maria Mitchell Observatory in, Massachusetts, United States.