Discovery [1] | |
---|---|
Discovered by | R. H. McNaught |
Discovery site | Siding Spring Obs. |
Discovery date | 9 August 1994 |
Designations | |
(7482) 1994 PC1 | |
1994 PC1 | |
Apollo · NEO · PHA [1] [2] | |
Orbital characteristics [1] | |
Epoch 2022-Jan-21 (JD 2459600.5) | |
Uncertainty parameter 0 | |
Observation arc | 47.23 yr (17,251 days) |
Earliest precovery date | 22 September 1974 |
Aphelion | 1.7935 AU |
Perihelion | 0.9042 AU |
1.3488 AU | |
Eccentricity | 0.3297 |
1.56 yr (572 days) | |
337.27° | |
0° 37m 51.6s / day | |
Inclination | 33.479° |
117.88° | |
47.477° | |
Earth MOID | 0.00054 AU (0.21 LD) |
Mars MOID | 0.139 AU (20.8 million km) [2] |
Physical characteristics | |
Mean diameter | 1.052±0.303 km [3] 1.30 km (calculated) [4] |
2.5999 h [5] | |
0.277±0.185 [3] 0.20 (assumed) [4] | |
SMASS = S [1] [4] | |
16.6 [1] [4] ·16.80±0.3 [3] | |
(7482) 1994 PC1 is a stony asteroid, classified as near-Earth object and potentially hazardous asteroid of the Apollo group, approximately 1.1 kilometers in diameter. It was discovered on 9 August 1994, by astronomer Robert McNaught at the Siding Spring Observatory in Coonabarabran, Australia. [2] With an observation arc of 47 years it has a very well known orbit and was observed by Goldstone radar in January 1997. [6] The 2022 approach has been observed every month since August 2021. [2]
1994 PC1 orbits the Sun at a distance of 0.9–1.8 AU once every 1 years and 7 months (572 days). Its orbit has an eccentricity of 0.33 and an inclination of 33° with respect to the ecliptic. [1]
On 17 January 1933, it passed 811,350 km (504,150 mi) from the Moon and then about an hour later made its closest known approach to Earth of 1,125,400 km (699,300 mi). [1] On 18 January 2022, it passed about 1,981,468 km (1,231,227 mi) from Earth. [1]
Date | JPL SBDB nominal geocentric distance | uncertainty region (3-sigma) |
---|---|---|
1933-01-17 | 1125383 km | ± 65 km [lower-alpha 1] |
2022-01-18 | 1981468 km | ± 47 km [7] |
2105-01-18 | 2328125 km | ± 1069 km [8] |
In the SMASS classification, 1994 PC1 is a common stony S-type asteroid. [1] [4]
In 1998, a rotational lightcurve of 1994 PC1 was obtained from photometric observations by Petr Pravec. Lightcurve analysis gave a well-defined rotation period of 2.5999 hours with a brightness amplitude of 0.29 magnitude ( U=3 ). [5]
According to the survey carried out by the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer, 1994 PC1 measures 1.052 kilometers in diameter and its surface has an albedo of 0.277. [3] The Collaborative Asteroid Lightcurve Link assumes an albedo of 0.20 and calculates a diameter of 1.30 kilometers based on an absolute magnitude of 16.8. [4]
At 18 January 2022 21:51 UTC, 1994 PC1 passed 5.15 lunar distances from Earth [1] and had a 3-sigma uncertainty region of less than ± 50 km. [7] It peaked at an apparent magnitude of about 10 [9] placing it just outside the reach of common 7×50 binoculars. The nearly Full moon being about 100 degrees from the asteroid during closest approach may have made it more difficult to observe with smaller telescopes.
Date & Time | Approach to | Nominal distance |
---|---|---|
2022-01-18 18:58 | Moon | 2085780 km [10] |
2022-01-18 21:51 | Earth | 1981468 km [1] |
PHA | Date | Approach distance (lunar dist.) | Abs. mag ( H ) | Diameter (C) (m) | Ref (D) | ||
---|---|---|---|---|---|---|---|
Nomi- nal(B) | Mini- mum | Maxi- mum | |||||
(33342) 1998 WT24 | 1908-12-16 | 3.542 | 3.537 | 3.547 | 17.9 | 556–1795 | data |
(458732) 2011 MD5 | 1918-09-17 | 0.911 | 0.909 | 0.913 | 17.9 | 556–1795 | data |
(7482) 1994 PC1 | 1933-01-17 | 2.927 | 2.927 | 2.928 | 16.8 | 749–1357 | data |
69230 Hermes | 1937-10-30 | 1.926 | 1.926 | 1.927 | 17.5 | 668–2158 | data |
69230 Hermes | 1942-04-26 | 1.651 | 1.651 | 1.651 | 17.5 | 668–2158 | data |
(137108) 1999 AN10 | 1946-08-07 | 2.432 | 2.429 | 2.435 | 17.9 | 556–1795 | data |
(33342) 1998 WT24 | 1956-12-16 | 3.523 | 3.523 | 3.523 | 17.9 | 556–1795 | data |
(163243) 2002 FB3 | 1961-04-12 | 4.903 | 4.900 | 4.906 | 16.4 | 1669–1695 | data |
(192642) 1999 RD32 | 1969-08-27 | 3.627 | 3.625 | 3.630 | 16.3 | 1161–3750 | data |
(143651) 2003 QO104 | 1981-05-18 | 2.761 | 2.760 | 2.761 | 16.0 | 1333–4306 | data |
2017 CH1 | 1992-06-05 | 4.691 | 3.391 | 6.037 | 17.9 | 556–1795 | data |
(170086) 2002 XR14 | 1995-06-24 | 4.259 | 4.259 | 4.260 | 18.0 | 531–1714 | data |
(33342) 1998 WT24 | 2001-12-16 | 4.859 | 4.859 | 4.859 | 17.9 | 556–1795 | data |
4179 Toutatis | 2004-09-29 | 4.031 | 4.031 | 4.031 | 15.3 | 2440–2450 | data |
2014 JO25 | 2017-04-19 | 4.573 | 4.573 | 4.573 | 17.8 | 582–1879 | data |
(137108) 1999 AN10 | 2027-08-07 | 1.014 | 1.010 | 1.019 | 17.9 | 556–1795 | data |
(35396) 1997 XF11 | 2028-10-26 | 2.417 | 2.417 | 2.418 | 16.9 | 881–2845 | data |
(154276) 2002 SY50 | 2071-10-30 | 3.415 | 3.412 | 3.418 | 17.6 | 714–1406 | data |
(164121) 2003 YT1 | 2073-04-29 | 4.409 | 4.409 | 4.409 | 16.2 | 1167–2267 | data |
(385343) 2002 LV | 2076-08-04 | 4.184 | 4.183 | 4.185 | 16.6 | 1011–3266 | data |
(52768) 1998 OR2 | 2079-04-16 | 4.611 | 4.611 | 4.612 | 15.8 | 1462–4721 | data |
(33342) 1998 WT24 | 2099-12-18 | 4.919 | 4.919 | 4.919 | 17.9 | 556–1795 | data |
(85182) 1991 AQ | 2130-01-27 | 4.140 | 4.139 | 4.141 | 17.1 | 1100 | data |
314082 Dryope | 2186-07-16 | 3.709 | 2.996 | 4.786 | 17.5 | 668–2158 | data |
(137126) 1999 CF9 | 2192-08-21 | 4.970 | 4.967 | 4.973 | 18.0 | 531–1714 | data |
(290772) 2005 VC | 2198-05-05 | 1.951 | 1.791 | 2.134 | 17.6 | 638–2061 | data |
(A) List includes near-Earth approaches of less than 5 lunar distances (LD) of objects with H brighter than 18. (B) Nominal geocentric distance from the Earth's center to the object's center (Earth radius≈0.017 LD). (C) Diameter: estimated, theoretical mean-diameter based on H and albedo range between X and Y. (D) Reference: data source from the JPL SBDB, with AU converted into LD (1 AU≈390 LD) (E) Color codes: unobserved at close approach observed during close approach upcoming approaches |
As of 2022, this minor planet has not been named. [2]
2063 Bacchus, provisional designation 1977 HB, is a stony asteroid and near-Earth object of the Apollo group, approximately 1 kilometer in diameter. The contact binary was discovered on 24 April 1977, by American astronomer Charles Kowal at the Palomar Observatory in California, United States. It was named after Bacchus from Roman mythology.
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8013 Gordonmoore, provisional designation 1990 KA, is an eccentric, stony asteroid and near-Earth object of the Apollo group, approximately 1–2 kilometers in diameter.
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