4790 Petrpravec

4790 Petrpravec (prov. designation: 1988 PP) is a carbonaceous background asteroid from the central regions of the asteroid belt, approximately 16 kilometers (10 miles) in diameter. It was discovered on 9 August 1988, by American astronomer Eleanor Helin at the Palomar Observatory in California, and was later named for Czech astronomer Petr Pravec.^[1]

4790 Petrpravec

Shape model of Petrpravec from its lightcurve
Discovery[1]
Discovered by	E. F. Helin
Discovery site	Palomar Obs.
Discovery date	9 August 1988
Designations
MPC designation	(4790) Petrpravec
Named after	Petr Pravec[1] (Czech astronomer)
Alternative designations	1988 PP · 1978 EA1
Minor planet category	main-belt[1][2] · (middle) background[3] · Eunomia[4]
Orbital characteristics[2]
Epoch 23 March 2018 (JD 2458200.5)
Uncertainty parameter 0
Observation arc	40.21 yr (14,685 d)
Aphelion	2.8502 AU
Perihelion	2.4002 AU
Semi-major axis	2.6252 AU
Eccentricity	0.0857
Orbital period (sidereal)	4.25 yr (1,554 d)
Mean anomaly	80.278°
Mean motion	0° 13m 54.12s / day
Inclination	12.720°
Longitude of ascending node	131.48°
Argument of perihelion	84.770°
Physical characteristics
Mean diameter	14.40±4.13 km[5] 14.53±1.05 km[6] 16.16±4.77 km[7] 16.217±0.096 km[8] 17.160±5.818 km[9] 17.62±1.5 km[10]
Synodic rotation period	undetermined[11]
Geometric albedo	0.0336±0.0384[9] 0.038±0.007[8] 0.047±0.042[7] 0.05±0.04[5] 0.1084±0.021[10] 0.160±0.024[6]
Spectral type	C (Pan-STARRS)[4][12] C (SDSS-MOC)[13][14]
Absolute magnitude (H)	11.80[6][10] 12.8[7] 12.90[7] 13.0[1][2] 13.15[9] 13.15±0.18[12] 13.17[5]

Orbit and classification

Petrpravec is a non-family asteroid of the main belt's background population when applying the hierarchical clustering method to its proper orbital elements.^[3] Based on osculating Keplerian orbital elements, the asteroid has also been classified as a member of the Eunomia family (502), a prominent family of stony S-type asteroid and the largest one in the intermediate main belt with more than 5,000 members.^[4]

It orbits the Sun in the central asteroid belt at a distance of 2.4–2.9 AU once every 4 years and 3 months (1,554 days; semi-major axis of 2.63 AU). Its orbit has an eccentricity of 0.09 and an inclination of 13° with respect to the ecliptic.^[2] The body's observation arc begins with its first observation as 1978 EA₁ at Crimea–Nauchnij in March 1978, more than 10 years prior to its official discovery observation at Palomar.^[1]

Naming

This minor planet was named after Petr Pravec (born 1967), a Czech astronomer and prolific photometrist of comets, near-Earth and binary asteroids. He has often been the first person to observe objects found in the course of the discoverer's Near-Earth Asteroid Tracking program following their tentative announcement in the Minor Planet Center's (MPC) "NEO Confirmation Page". The official naming citation was published by the Minor Planet Center on 20 June 1997 on the occasion of his marriage with Kateřina Macháčová the following day (M.P.C. 30095).^[1][15]

Physical characteristics

In the SDSS-based taxonomy, Petrpravec is a poorly determined, carbonaceous C-type asteroid.^[13][14] It has also been characterized as a dark C-type by the Pan-STARRS' survey.^[4][12]

Rotation period

A rotational lightcurve of Petrpravec from photometric observations at the Oakley Southern Sky Observatory in February 2012, gave a brightness variation of only 0.02 magnitude and was insufficient to determine a rotation period.^[4][11]

Diameter and albedo

According to the surveys carried out by the Japanese Akari satellite, the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer and the Infrared Astronomical Satellite IRAS, Petrpravec measures between 14.4 and 17.6 kilometers in diameter and its surface has an albedo between 0.0336 and 0.160.^{[5][6][7][8][9][10]}

The Collaborative Asteroid Lightcurve Link derives an albedo of 0.0369 and a diameter of 17.37 kilometers based on an absolute magnitude of 13.0.^[4]