(7482) 1994 PC1

Near-Earth asteroid January 2022 From Wikipedia, the free encyclopedia

(7482) 1994 PC1 is a stony asteroid and near-Earth object, currently estimated to be the most potentially hazardous asteroid over the next 1000 years.[6][7] It is in 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.[8]

Quick facts Discovery, Discovered by ...
(7482) 1994 PC1
Orbit with positions Jan 2020
Discovery[1]
Discovered byR. H. McNaught
Discovery siteSiding Spring Obs.
Discovery date9 August 1994
Designations
(7482) 1994 PC1
1994 PC1
Apollo Â· NEO Â· PHA[1][2]
Orbital characteristics[1]
Epoch 2022-Jan-21 (JD 2459600.5)
Uncertainty parameter 0
Observation arc47.23 yr (17,251 days)
Earliest precovery date22 September 1974
Aphelion1.7935 AU
Perihelion0.9042 AU
1.3488 AU
Eccentricity0.3297
1.56 yr (572 days)
337.27°
0° 37m 51.6s / day
Inclination33.479°
117.88°
47.477°
Earth MOID0.00054 AU (0.21 LD)
Mars MOID0.139 AU (20.8 million km)[2]
Physical characteristics
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] Â· 16.80±0.3[3]
Close

Of all the known asteroids larger than 1 km, 1994 PC1 has the largest probability of a "deep close encounter" with Earth over the next 1000 years. It has a close encounter with Earth in 2525, after which the uncertainty of its orbit increases.[6]

Orbit and classification

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]

More information Date, JPL SBDBnominal geocentric distance ...
Close approaches[1]
Date JPL SBDB
nominal geocentric
distance
uncertainty
region
(3-sigma)
1933-01-171125383 km± 65 km[a]
2022-01-181981468 km± 47 km[9]
2105-01-182328125 km± 1069 km[10]
Close

Physical characteristics

In the SMASS classification, 1994 PC1 is a common stony S-type asteroid.[1][4]

Rotation period

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]

Diameter and albedo

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]

2022 flyby

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.[9] It peaked at an apparent magnitude of about 10[11] 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.

More information Date & Time, Approach to ...
2022 Moon/Earth approach
Date & Time Approach
to
Nominal distance
2022-01-18 18:58Moon2085780 km[12]
2022-01-18 21:51Earth1981468 km[1]
Close
Animation of 1994 PC1 - 2022 close approach
  Sun Â·   Earth Â·   1994 PC1
Sky trajectory with daily motion
History of close approaches of large near-Earth objects since 1908 (A)
More information PHA, Date ...
PHA Date Approach distance (lunar dist.) Abs.
mag

(H)
Diameter (C)
(m)
Ref (D)
Nomi-
nal(B)
Mini-
mum
Maxi-
mum
(33342) 1998 WT241908-12-163.5423.5373.54717.9556–1795data
(458732) 2011 MD51918-09-170.9110.9090.91317.9556–1795data
(7482) 1994 PC11933-01-172.9272.9272.92816.8749–1357data
69230 Hermes1937-10-301.9261.9261.92717.5668–2158data
69230 Hermes1942-04-261.6511.6511.65117.5668–2158data
(137108) 1999 AN101946-08-072.4322.4292.43517.9556–1795data
(33342) 1998 WT241956-12-163.5233.5233.52317.9556–1795data
(163243) 2002 FB31961-04-124.9034.9004.90616.41669–1695data
(192642) 1999 RD321969-08-273.6273.6253.63016.31161–3750data
(143651) 2003 QO1041981-05-182.7612.7602.76116.01333–4306data
2017 CH11992-06-054.6913.3916.03717.9556–1795data
(170086) 2002 XR141995-06-244.2594.2594.26018.0531–1714data
(33342) 1998 WT242001-12-164.8594.8594.85917.9556–1795data
4179 Toutatis2004-09-294.0314.0314.03115.32440–2450data
(671294)2014 JO252017-04-194.5734.5734.57317.8582–1879data
(137108) 1999 AN102027-08-071.0141.0101.01917.9556–1795data
(35396) 1997 XF112028-10-262.4172.4172.41816.9881–2845data
(154276) 2002 SY502071-10-303.4153.4123.41817.6714–1406data
(164121) 2003 YT12073-04-294.4094.4094.40916.21167–2267data
(385343) 2002 LV2076-08-044.1844.1834.18516.61011–3266data
(52768) 1998 OR22079-04-164.6114.6114.61215.81462–4721data
(33342) 1998 WT242099-12-184.9194.9194.91917.9556–1795data
(85182) 1991 AQ2130-01-274.1404.1394.14117.11100data
314082 Dryope2186-07-163.7092.9964.78617.5668–2158data
(137126) 1999 CF92192-08-214.9704.9674.97318.0531–1714data
(290772) 2005 VC2198-05-051.9511.7912.13417.6638–2061data
(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
Close

Naming

As of 2022, this minor planet has not been named.[2]

See also

Notes

  1. The 1933 approach is better constrained than the 2105 approach as a result of the 1974, 1977, 1980 precovery images of the asteroid.[2]

References

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