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4897 Tomhamilton, provisional designation 1987 QD6, is a stony asteroid from the outer region of the asteroid belt, approximately 14 kilometers in diameter. It was discovered on 22 August 1987, by American astronomer Eleanor Helin at Palomar Observatory, California. It was later named after American writer Thomas Hamilton, author of astronomy books and participant in the Apollo program.[2]

4897 Tomhamilton
Discovery[1]
Discovered byE. F. Helin
Discovery sitePalomar Obs.
Discovery date22 August 1987
Designations
MPC designation
(4897) Tomhamilton
Named after
Thomas Hamilton
(American writer)[2]
Alternative designations
1987 QD6 · 1971 QV1
1971 SB1 · 1990 BN1
Minor planet category
main-belt · (outer)
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc66.81 yr (24,402 days)
Aphelion3.4356 AU
Perihelion2.6792 AU
Semi-major axis
3.0574 AU
Eccentricity0.1237
Orbital period (sidereal)
5.35 yr (1,953 days)
Mean anomaly
262.29°
Mean motion
0° 11m 3.84s / day
Inclination11.067°
Longitude of ascending node
188.47°
Argument of perihelion
107.13°
Physical characteristics
Dimensions13.711±0.369 km[3]
Geometric albedo
0.215±0.065[3]
Absolute magnitude (H)
12.0[1]

    Classification and orbit


    Tomhamilton orbits the Sun in the outer main-belt at a distance of 2.7–3.4 AU once every 5 years and 4 months (1,953 days). Its orbit has an eccentricity of 0.12 and an inclination of 11° with respect to the ecliptic.[1]

    In August 1950, a first precovery was taken at Palomar, extending the asteroid's observation arc by 37 years prior to its official discovery observation.[2] It had also been previously identified as 1971 QV1 and 1971 SB1 at Crimea–Nauchnij.

    On 11 January 2011, it was at opposition (coinciding with Hamilton's 72nd birthday) at a distance of 2.476 AU. Given the moderately elliptical orbit, this asteroid can on rare occasions reach an apparent magnitude from Earth of about 10.9.[citation needed]


    Naming


    This minor planet was named after Thomas William Hamilton, an American (born San Francisco, 1939) who was a child actor (he played "Barnaby" in Barnaby and Mr. O'Malley and was on the early television show Mr. I-Magination). As an adult he abandoned acting to return to his primary interest as an astronomer. As such he worked on the Apollo program, determining fuel requirements and radar accuracy requirements for lunar orbit rendezvous. He later worked as an astronomy educator and planetarium director, and is the author of time travel and science fiction novels, and also wrote six books on astronomical topics. Hamilton and Helin were acquainted, as he had interviewed her at an astronomical conference for a cable television show he was producing at the time. The official naming citation was published by the Minor Planet Center on 4 October 2009 (M.P.C. 67215).[4]


    Physical characteristics



    Diameter and albedo


    According to the survey carried out by NASA's Wide-field Infrared Survey Explorer with its subsequent NEOWISE mission, Tomhamilton measures 13.7 kilometers in diameter and its surface has an albedo of 0.215, which indicates that it of a stony rather than of a carbonaceous composition.[3]


    Lightcurve


    As of 2017, no rotational lightcurve of Tomhamilton has been obtained from photometric observations. It rotation period, poles and shape remain unknown.[1][5]


    Books by Hamilton


    Hamilton has also had many astronomical articles in The Constellation, and science fiction in Aphelion, Bewildering Stories (Oct. 30, 2017, "An Arkham Halloween"), and Changingthetimes.com (Nov. 23, 2020, "Moctezuma Succeeds").


    Scholarship


    In 2011, using funds that had come down from his great great grandfather Thomas Oliver Larkin, Hamilton created the Hamilton Planetarium Scholarship Fund to encourage and train students to enter the planetarium field as a career.



    References


    1. "JPL Small-Body Database Browser: 4897 Tomhamilton (1987 QD6)" (2017-06-05 last obs.). Jet Propulsion Laboratory. Retrieved 4 August 2017.
    2. "4897 Tomhamilton (1987 QD6)". Minor Planet Center. Retrieved 26 August 2016.
    3. 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. Retrieved 26 August 2016.
    4. "MPC/MPO/MPS Archive". Minor Planet Center. Retrieved 26 August 2016.
    5. "LCDB Data for (4897) Tomhamilton". Asteroid Lightcurve Database (LCDB). Retrieved 4 August 2017.





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