1221 Amor

1221 Amor /ˈeɪmɔːr/ is an asteroid and near-Earth object on an eccentric orbit, approximately 1 kilometer (0.6 miles) in diameter. It is the namesake of the Amor asteroids, the second-largest subgroup of near-Earth objects. It was discovered by Eugène Delporte at the Uccle Observatory in 1932, the first time that an asteroid was seen to approach Earth so closely.[1] The assumed S-type asteroid is one of few low-numbered asteroids for which no rotation period has been determined.[8] It was assigned the provisional designation 1932 EA1 and named for Cupid, also known as "Amor" in Latin, the Roman equivalent of the Greek god Eros.[4]

1221 Amor
Orbital diagram of Amor (cyan) with Earth, Mars and Jupiter (outermost) on 12 March 1932
Discovery [1][2]
Discovered byE. Delporte
Discovery siteUccle Obs.
Discovery date12 March 1932
Designations
(1221) Amor
Pronunciation/ˈeɪmɔːr/[3]
Named after
Cupid, Roman analogue of Eros [4]
(Classical mythology)
1932 EA1
AdjectivesAmorian /əˈmɔːriən/[7]
Orbital characteristics [6]
Epoch 23 March 2018 (JD 2458200.5)
Uncertainty parameter 0
Observation arc86.50 yr (31,595 d)
Aphelion2.7550 AU
Perihelion1.0832 AU
1.9191 AU
Eccentricity0.4355
2.66 yr (971 d)
102.03°
0° 22m 14.52s / day
Inclination11.879°
171.34°
26.656°
Earth MOID0.1069 AU (41.6 LD)
Physical characteristics
Mean diameter
  • 0.15 (assumed)[6]
  • 0.20 (assumed)[8]
S (assumed)[8]

    Discovery

    On 12 March 1932, Belgian astronomer Eugène Delporte photographed Amor at the Royal Observatory of Belgium in Uccle,[1] as it approached Earth to within 16 million kilometers (about 40 times the distance from Earth to the Moon). This was the first time that an asteroid was seen to approach Earth so closely. The body's observation arc begins with its official discovery observation on 12 March 1932, when it was observed at the Uccle and Heidelberg observatories simultaneously.[1]

    Orbit and classification

    Amor is the namesake of the Amor asteroid, a subgroup of near-Earth asteroids that approach the orbit of Earth from beyond, but do not cross it. Next to the Apollo group, the Amors are the second largest group of near-Earth objects with more than 7,000 known members.[10] As with many members of this group, Amor is also a Mars-crosser, crossing the orbit of the Red Planet at 1.66 AU.[6]

    It orbits the Sun at a distance of 1.08–2.76 AU once every 2 years and 8 months (971 days; semi-major axis of 1.92 AU). Its orbit has a high eccentricity of 0.44 and an inclination of 12° with respect to the ecliptic.[6]

    Close encounters

    Amor has an Earth minimum orbital intersection distance of 0.1069 AU (16,000,000 km) which corresponds to 41.6 lunar distances.[6] In March 1940, it approached Earth to 0.1052 AU (15,700,000 km), its closest approach of all close encounters since 1900. Only in March 2129, it will approach Earth at a similar distance of 0.1082 AU (16,200,000 km).[6]

    Naming

    This minor planet was named after the Roman god of love, Cupid, also known as Amor in Latin, and the Roman equivalent of the Greek god Eros.[4] The near-Earth asteroids 433 Eros and 763 Cupido are also named after the god of love. The official naming citation was mentioned in The Names of the Minor Planets by Paul Herget in 1955 (H 113).[4]

    Physical characteristics

    Amor is an assumed, stony S-type asteroid.[8]

    Rotation period

    As of 2018, no rotational lightcurve of Amor has been obtained from photometric observations. The body's rotation period, pole and shape remain unknown.[6][8]

    Diameter and albedo

    According to Tom Gehrels's publication Hazards due to Comets and Asteroids from 1994 (pp. 540–543), Amor measures 1.0 kilometer in diameter and its surface has an albedo of 0.15.[6] The Collaborative Asteroid Lightcurve Link assumes a standard albedo for stony asteroids of 0.20 and calculates a diameter of 0.857 kilometers based on an absolute magnitude of 17.7.[8]

    gollark: So, enjoy 5ms better latency?
    gollark: Then I moved it nearer the magic wireless box™, and thought I plugged in the cable, but as it turns out made a mistake as it didn't click in properly. So now it is TRULY ethernetted.
    gollark: Initially, it was over WiFi in another room, which I *think* is why the connection dropped out a bit.
    gollark: Yes.
    gollark: I also just now plugged in the ethernet cable on the HNode™, so enjoy better quality of service.

    References
    1. "1221 Amor (1932 EA1)". Minor Planet Center. Retrieved 24 September 2018.
    2. "Asteroid 1221 Amor". Small Bodies Data Ferret. Retrieved 24 September 2018.
    3. "Amor". Dictionary.com Unabridged. Random House.
    4. Schmadel, Lutz D. (2007). "(1221) Amor". Dictionary of Minor Planet Names – (1221) Amor. Springer Berlin Heidelberg. p. 102. doi:10.1007/978-3-540-29925-7_1222. ISBN 978-3-540-00238-3.
    5. "Asteroid (1221) Amor". NEODyS-2, Near-Earth object – Dynamic Site. Retrieved 24 September 2018.
    6. "JPL Small-Body Database Browser: 1221 Amor (1932 EA1)" (2018-09-12 last obs.). Jet Propulsion Laboratory. Retrieved 24 September 2018.
    7. Frederick Palmer (1923) "The Flaming Woman", Collier's, vol. 71, April 14
    8. "LCDB Data for (1221) Amor". Asteroid Lightcurve Database (LCDB). Retrieved 24 September 2018.
    9. Wisniewski, W. Z.; Michalowski, T. M.; Harris, A. W.; McMillan, R. S. (April 1997). "Photometric Observations of 125 Asteroids". Icarus. 126 (2): 395–449. Bibcode:1997Icar..126..395W. doi:10.1006/icar.1996.5665. Retrieved 24 September 2018.
    10. "Discovery Statistics – Cumulative Totals". NASA/JPL CNEOS. 21 September 2018. Retrieved 24 September 2018.
    This article is issued from Wikipedia. The text is licensed under Creative Commons - Attribution - Sharealike. Additional terms may apply for the media files.