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1862 Apollo

Stony asteroid


Stony asteroid

FieldValue
minorplanetyes
name1862 Apollo
symbol24px (astrological)
background#FFC2E0
image1862Apollo (Lightcurve Inversion).png
caption
discovery_ref
discovererK. Reinmuth
discovered24 April 1932
discovery_siteHeidelberg Obs.
mpc_name(1862) Apollo
alt_names1932 HA
pronounced
named_afterApollo
(Greek mythology)
mp_categoryNEOPHA
Venus-crosser
Mars-crosser
Apollo asteroids
orbit_ref
epoch29 December 2009 (JD 2455194.5)
uncertainty0
observation_arc85.32 yr (31162 days)
earliest_precovery_date13 December 1930
aphelion2.2935 AU
perihelion0.64699 AU
semimajor1.4702 AU
eccentricity0.55994
period1.78 yr (651.15 d)
mean_anomaly144.22°
inclination6.3530°
asc_node35.739°
arg_peri285.85°
moid0.0257026 AU
dimensions1.5 km
rotation3.065 h
spectral_typeQ (Tholen, SMASS)
B–V = 0.819
U–B = 0.481
abs_magnitude16.25
albedo0.25
temp_name1Kelvin
min_temp_1171 K
mean_temp_1214 K
max_temp_1322 K
temp_name2Celsius
min_temp_2−102 °C
mean_temp_2−59 °C
max_temp_249 °C
temp_name3Fahrenheit
min_temp_3−151.6 °F
mean_temp_3−74.2 °F
max_temp_3120.2 °F
mean_motion/ day
mean_radius0.75 km
jupiter_moid3.06837 AU
tisserand4.415

(Greek mythology) Venus-crosser Mars-crosser Apollo asteroids B–V = 0.819 U–B = 0.481

1862 Apollo is a stony asteroid, approximately 1.5 kilometers in diameter, classified as a near-Earth object (NEO). It was discovered by German astronomer Karl Reinmuth at Heidelberg Observatory on 24 April 1932, but was lost and not recovered until 1973.

It is the namesake and the first recognized member of the Apollo asteroids, a subgroup of NEOs which are Earth-crossers, that is, they cross the orbit of the Earth when viewed perpendicularly to the ecliptic plane (crossing an orbit is a more general term than actually intersecting it). In addition, since Apollo's orbit is highly eccentric, it crosses the orbits of Venus and Mars and is therefore called a Venus-crosser and Mars-crosser as well.

Although Apollo was the first Apollo asteroid to be discovered, its official IAU-number (1862) is higher than that of some other Apollo asteroids such as 1566 Icarus, because it was a lost asteroid for more than 40 years and other bodies were numbered in the meantime. The analysis of its rotation provided observational evidence of the YORP effect.

It is named after the Greek god Apollo, god of prophecy, music, healing and light, child of Zeus and Leto, after which the minor planets 5731 Zeus and 68 Leto are named.

Satellite

On 4 November 2005, it was announced that an asteroid moon, or satellite of Apollo, had been detected by radar observations from Arecibo Observatory, Puerto Rico, on 19 October – 2 November 2005. The announcement is contained in the International Astronomical Union Circular (IAUC) 8627. The satellite is only 80 m across and orbits Apollo just 3 km away from the asteroid itself. From the surface of Apollo, the satellite would have an angular diameter of about 2.0835 degrees.Calculated from the formula \delta = (206265) d / D arcseconds. (see Angular diameter)

Potentially hazardous object

1862 Apollo is a potentially hazardous asteroid (PHA) because its minimum orbit intersection distance (MOID) is less than 0.05 AU and its diameter is greater than 150 meters. Apollo's Earth MOID is 0.0257 AU. Its orbit is well-determined for the next several hundred years. On 17 May 2075 it will pass 0.0083 AU from Venus.

Notes

References

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References

  1. "Apollo". [[Oxford University Press]].
  2. "Planetary Habitability Calculators". University of Puerto Rico at Arecibo.
  3. "IAU Circular No. 8627". Central Bureau for Astronomical Telegrams.
  4. Johnston, Wm. Robert. (November 16, 2014). "(1862) Apollo". Johnston's Archive.
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