4001 Ptolemaeus, provisional designation 1949 PV, is a Florian asteroid from the inner regions of the asteroid belt, approximately 5 kilometers (3.1 miles) in diameter. It was discovered on 2 August 1949, by German astronomer Karl Reinmuth at the Heidelberg-Königstuhl State Observatory in Heidelberg, Germany. In 1991, the International Astronomical Union named the S-type asteroid after Greco-Roman astronomer Ptolemy.[1]
![]() Orbit of 4001 Ptolemaeus | |
Discovery [1] | |
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Discovered by | K. Reinmuth |
Discovery site | Heidelberg Obs. |
Discovery date | 2 August 1949 |
Designations | |
MPC designation | (4001) Ptolemaeus |
Pronunciation | /tɒləˈmiːəs/ |
Named after | Ptolemy [1] (Greco-Roman astronomer) |
Alternative designations | 1949 PV · 1949 QD1 1982 BU9 · 1987 OE |
Minor planet category | main-belt [1][2] · (inner) Flora [3] |
Orbital characteristics [2] | |
Epoch 23 March 2018 (JD 2458200.5) | |
Uncertainty parameter 0 | |
Observation arc | 67.75 yr (24,744 d) |
Aphelion | 2.6809 AU |
Perihelion | 1.8940 AU |
Semi-major axis | 2.2874 AU |
Eccentricity | 0.1720 |
Orbital period (sidereal) | 3.46 yr (1,264 d) |
Mean anomaly | 294.51° |
Mean motion | 0° 17m 5.64s / day |
Inclination | 5.4568° |
Longitude of ascending node | 130.67° |
Argument of perihelion | 204.09° |
Physical characteristics | |
Mean diameter | 4.641±0.297 km[4] 5.0 km (est. at 0.24)[5] |
Geometric albedo | 0.392±0.056[4] |
Spectral type | SMASS = S [2] |
Absolute magnitude (H) | 13.7[2] |
Ptolemaeus is a member of the Flora family (402),[3] a giant asteroid family and the largest family of stony asteroids in the main-belt.[6] It orbits the Sun in the inner main-belt at a distance of 1.9–2.7 AU once every 3 years and 6 months (1,264 days; semi-major axis of 2.29 AU). Its orbit has an eccentricity of 0.17 and an inclination of 5° with respect to the ecliptic.[2]
The body's observation arc begins with its observations as 1949 QD1 at Lowell Observatory on 24 August 1949, or three weeks after its official discovery observation at Heidelberg.[1] On 24 April 1989, Ptolemaeus approached the asteroid 6 Hebe within 5.5 million kilometers at a relative velocity of 3.7 km/s.[2]
In the SMASS classification, Ptolemaeus is a common, stony S-type asteroid, which is in agreement with the overall spectral type for members of the Flora family.[6]: 23
According to the survey carried out by the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer, Ptolemaeus measures 4.641 kilometers in diameter and its surface has a high albedo of 0.392.[4] Based on a generic magnitude-to-diameter conversion, assuming a Flora-type typical albedo of 0.24, the asteroid measures 5.0 kilometers for an absolute magnitude of 13.7.[5]
As of 2018, no rotational lightcurve of Ptolemaeus has been obtained from photometric observations. The body's rotation period, poles and shape remain unknown.[2]
This minor planet was named after 2nd-century Greco-Roman astronomer Ptolemy (Latin: "Ptolemaeus") by IAU's Minor Planet Names Committee. He is best known for his influential Almagest, a mathematical and astronomical treatise on the apparent motions of the stars and planetary paths. Its ideas dominated astronomy for 1200 years until Copernicus in the early Renaissance.[1] The official naming citation was published by the Minor Planet Center on 21 November 1991 (M.P.C. 19335).[7]
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