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4432 McGraw-Hill

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Main-belt asteroid

4432 McGraw-Hill
Discovery 
Discovered byS. J. Bus
Discovery siteSiding Spring Obs.
Discovery date2 March 1981
Designations
MPC designation(4432) McGraw-Hill
Named afterMcGraw-Hill Telescope
(at Kitt Peak, Arizona)
Alternative designations1981 ER22 · 1964 TV
Minor planet categorymain-belt  · (inner)
background
Orbital characteristics
Epoch 23 March 2018 (JD 2458200.5)
Uncertainty parameter 0
Observation arc53.54 yr (19,555 d)
Aphelion2.8975 AU
Perihelion1.8747 AU
Semi-major axis2.3861 AU
Eccentricity0.2143
Orbital period (sidereal)3.69 yr (1,346 d)
Mean anomaly188.28°
Mean motion0° 16 2.64 / day
Inclination0.4616°
Longitude of ascending node115.15°
Argument of perihelion246.30°
Physical characteristics
Mean diameter3.042±0.643 km
3.43 km (derived)
Synodic rotation periodinconclusive
Geometric albedo0.20 (assumed)
0.254±0.224
Spectral typeS (assumed)
Absolute magnitude (H)14.5
14.69

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.

Orbit and classification

McGraw-Hill is a non-family asteroid from the main belt's background population. 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.

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.

Physical characteristics

McGraw-Hill is an assumed, stony S-type asteroid, 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.). As of 2018, the body's rotation period, pole and shape remain unknown.

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, 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.

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. The official naming citation was published by the Minor Planet Center on 18 February 1992 (M.P.C. 19697).

References

  1. ^ "4432 McGraw-Hill (1981 ER22)". Minor Planet Center. Retrieved 27 May 2018.
  2. ^ "JPL Small-Body Database Browser: 4432 McGraw-Hill (1981 ER22)" (2018-04-23 last obs.). Jet Propulsion Laboratory. Retrieved 27 May 2018.
  3. ^ "LCDB Data for (4432) McGraw-Hill". Asteroid Lightcurve Database (LCDB). Retrieved 27 May 2018.
  4. ^ "Asteroid 4432 McGraw-Hill". Small Bodies Data Ferret. Retrieved 27 May 2018.
  5. ^ 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.
  6. ^ 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)
  7. ^ 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.
  8. "MPC/MPO/MPS Archive". Minor Planet Center. Retrieved 27 May 2018.

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