Main-belt asteroid
4432 McGraw-Hill , provisional designation 1981 ER22 , is a background asteroid from the inner regions of the asteroid belt , approximately 3 kilometers (2 miles) in diameter. It was discovered on 2 March 1981, by American astronomer Schelte Bus at the Siding Spring Observatory in Australia. The likely S-type asteroid was named for the McGraw-Hill Telescope located at Kitt Peak , Arizona.[ 1]
Orbit and classification
McGraw-Hill is a non-family asteroid from the main belt's background population .[ 4] It orbits the Sun in the inner asteroid belt at a distance of 1.9–2.9 AU once every 3 years and 8 months (1,346 days; semi-major axis of 2.39 AU). Its orbit has an eccentricity of 0.21 and an inclination of 0° with respect to the ecliptic .[ 2]
The asteroid was first observed as 1964 TV at Purple Mountain Observatory in October 1964. The body's observation arc begins with a precovery taken at Palomar Observatory in February 1977, or four years prior to its official discovery observation at Siding Spring.[ 1]
Physical characteristics
McGraw-Hill is an assumed, stony S-type asteroid ,[ 3] in agreement with the albedo (see below) obtained by the Wide-field Infrared Survey Explorer (WISE).
Rotation period
During the Small Main-Belt Asteroid Lightcurve Survey, McGraw-Hill has been observed photometrically . The observations gave a small brightness variation of 0.06 magnitude but resulted in no useful rotational lightcurve (U=n.a. ).[ 7] As of 2018, the body's rotation period , pole and shape remain unknown.[ 2]
Diameter and albedo
According to the survey carried out by the NEOWISE mission of NASA's WISE telescope, McGraw-Hill measures 3.042 kilometers in diameter and its surface has an albedo of 0.254,[ 5] [ 6] while the Collaborative Asteroid Lightcurve Link assumes a standard albedo for a stony asteroid of 0.20 and derives a diameter of 3.43 kilometers based on an absolute magnitude of 14.69.[ 3]
Naming
This minor planet was named after the 1.3-meter McGraw-Hill Telescope located at the MDM Observatory at the Kitt Peak National Observatory site in Arizona, United States.[ 1] The official naming citation was published by the Minor Planet Center on 18 February 1992 (M.P.C. 19697 ).[ 8]
References
^ a b c d e f g "4432 McGraw-Hill (1981 ER22)" . Minor Planet Center . Retrieved 27 May 2018 .
^ a b c d e "JPL Small-Body Database Browser: 4432 McGraw-Hill (1981 ER22)" (2018-04-23 last obs.). Jet Propulsion Laboratory . Retrieved 27 May 2018 .
^ a b c d e f g h "LCDB Data for (4432) McGraw-Hill" . Asteroid Lightcurve Database (LCDB). Retrieved 27 May 2018 .
^ a b "Asteroid 4432 McGraw-Hill" . Small Bodies Data Ferret . Retrieved 27 May 2018 .
^ a b c Masiero, Joseph R.; Mainzer, A. K.; Grav, T.; Bauer, J. M.; Cutri, R. M.; Dailey, J.; et al. (November 2011). "Main Belt Asteroids with WISE/NEOWISE. I. Preliminary Albedos and Diameters". The Astrophysical Journal . 741 (2): 20. arXiv :1109.4096 . Bibcode :2011ApJ...741...68M . doi :10.1088/0004-637X/741/2/68 . S2CID 118745497 .
^ a b c d Mainzer, A.; Grav, T.; Masiero, J.; Hand, E.; Bauer, J.; Tholen, D.; et al. (November 2011). "NEOWISE Studies of Spectrophotometrically Classified Asteroids: Preliminary Results". The Astrophysical Journal . 741 (2): 25. arXiv :1109.6407 . Bibcode :2011ApJ...741...90M . doi :10.1088/0004-637X/741/2/90 . S2CID 35447010 . (catalog )
^ a b c Binzel, Richard P.; Xu, Shui; Bus, Schelte J.; Bowell, Edward (September 1992). "Small Main-Belt Asteroid Lightcurve Survey". Icarus . 99 (1): 225– 237. Bibcode :1992Icar...99..225B . doi :10.1016/0019-1035(92)90184-9 . ISSN 0019-1035 .
^ "MPC/MPO/MPS Archive" . Minor Planet Center . Retrieved 27 May 2018 .
External links