| Minorplanet: | yes |
| 4332 Milton | |
| Background: |
|
| Discovery Ref: |   |
| Discovered: | 5 September 1983 |
| Mpc Name: | (4332) Milton |
| Alt Names: | 1983 RC |
| Named After: | Daniel J. Milton  |
| Mp Category: | background  |
| Orbit Ref: |   |
| Epoch: | 23 March 2018 (JD 2458200.5) |
| Uncertainty: | 0 |
| Observation Arc: | 84.44 yr (30,841 d) |
| Perihelion: | 1.7701 AU |
| Semimajor: | 2.5846 AU |
| Eccentricity: | 0.3151 |
| Period: | 4.16 yr (1,518 d) |
| Mean Motion: | / day |
| Inclination: | 19.169° |
| Asc Node: | 166.00° |
| Arg Peri: | 198.38° |
| Mean Diameter: | |
| Rotation: | |
| Albedo: | |
| Spectral Type: | SMASS Xe C  |
| Abs Magnitude: | 11.9 12.7 12.73 12.8 |
4332 Milton, provisional designation, is a background asteroid from the central regions of the asteroid belt, approximately 11km (07miles) in diameter. It was discovered on 5 September 1983, by American astronomer Carolyn Shoemaker at the Palomar Observatory in California. The X e-subtype has a rotation period of 3.3 hours. It was named after Daniel Milton, American geologist with the USGS.
Milton is a non-family asteroid from the main belt's background population. It orbits the Sun in the central asteroid belt at a distance of 1.8–3.4 AU once every 4 years and 2 months (1,518 days; semi-major axis of 2.58 AU). Its orbit has an eccentricity of 0.32 and an inclination of 19° with respect to the ecliptic.
The asteroid was first observed as at Heidelberg Observatory in September 1933. The body's observation arc begins with its official discovery observation at Palomar in September 1983.
In the SMASS classification, Milton is a Xe-subtype that transitions between the X-type and E-type asteroids. It has also been characterized as a carbonaceous C-type by Pan-STARRS large-scale survey.
In September 2008, a rotational lightcurve of Milton was obtained from photometric observations by Julian Oey at the Kingsgrove and Leura observatories. Lightcurve analysis gave a rotation period of 3.2978 hours with a brightness variation of 0.30 magnitude . In August 2012, a refined period of 3.295 hours and an amplitude of 0.16 magnitude was measured by Afşar Kabaş at the Çanakkale University Observatory in Turkey .
According to the surveys carried out by the Infrared Astronomical Satellite IRAS and the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer, Milton measures between 11.500 and 11.54 kilometers in diameter and its surface has an albedo between 0.1002 and 0.2306.
The Collaborative Asteroid Lightcurve Link derives an albedo of 0.1158 and a diameter of 11.26 kilometers based on an absolute magnitude of 12.7.
Only one brief stellar occultation by 4332 Milton has been observed to date, in 2021.
This minor planet was named after Daniel J. Milton (1934-2024), American geologist with the United States Geological Survey, known for his geological studies of the Moon and Mars, as well as for research on impact craters and features in Australia. The official naming citation was published by the Minor Planet Center on 30 January 1991 .