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(7482) 1994 PC1
Near-Earth asteroid January 2022
Near-Earth asteroid January 2022
| Field | Value |
|---|---|
| minorplanet | yes |
| name | |
| background | #FFC2E0 |
| image | 1994-PC1-orbit.png |
| caption | Orbit with positions Jan 2020 |
| discovery_ref | |
| discoverer | R. H. McNaught |
| discovery_site | Siding Spring Obs. |
| discovered | 9 August 1994 |
| mpc_name | (7482) |
| alt_names | |
| named_after | |
| mp_category | ApolloNEOPHA |
| orbit_ref | |
| epoch | 2022-Jan-21 (JD 2459600.5) |
| uncertainty | 0 |
| observation_arc | 47.23 yr (17,251 days) |
| earliest_precovery_date | 22 September 1974 |
| aphelion | 1.7935 AU |
| perihelion | 0.9042 AU |
| semimajor | 1.3488 AU |
| eccentricity | 0.3297 |
| period | 1.56 yr (572 days) |
| mean_anomaly | 337.27° |
| mean_motion | / day |
| inclination | 33.479° |
| asc_node | 117.88° |
| arg_peri | 47.477° |
| moid | 0.00054 AU |
| mars_moid | 0.139 AU |
| mean_diameter | km |
| 1.30 km (calculated) | |
| rotation | h |
| albedo | |
| 0.20 (assumed) | |
| spectral_type | SMASS S |
| abs_magnitude | 16.6 |
1.30 km (calculated) 0.20 (assumed)
**** is a stony asteroid and near-Earth object, currently estimated to be the most potentially hazardous asteroid over the next 1000 years. 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. With an observation arc of 47 years it has a very well known orbit and was observed by Goldstone radar in January 1997.
Of all the known asteroids larger than 1 km, 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.
Orbit and classification
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.
On 17 January 1933, it passed 811350 km from the Moon and then about an hour later made its closest known approach to Earth of 1125400 km. On 18 January 2022, it passed about 1981468 km from Earth.
| Date | JPL SBDB | |
|---|---|---|
| nominal geocentric | ||
| distance | uncertainty | |
| region | ||
| ([3-sigma](3-sigma)) | ||
| 1933-01-17 | ± 65 km | |
| 2022-01-18 | ± 47 km | |
| 2105-01-18 | ± 1069 km |
Physical characteristics
In the SMASS classification, is a common stony S-type asteroid.
Rotation period
In 1998, a rotational lightcurve of 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 ().
Diameter and albedo
According to the survey carried out by the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer, measures 1.052 kilometers in diameter and its surface has an albedo of 0.277. 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.
2022 flyby
At 18 January 2022 21:51 UTC, passed 5.15 lunar distances from Earth and had a 3-sigma uncertainty region of less than ± 50 km. It peaked at an apparent magnitude of about 10 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 | |
| 2022-01-18 21:51 | Earth |

| [[File:1994 PC1 skypath 2022.png | 500px]] |
|---|
Naming
As of 2022, this minor planet has not been named.
Notes
References
References
- Carter, Jamie. (May 29, 2023). "We Are (Probably) Safe From Asteroids For 1,000 Years, Say Scientists".
- (2023-06-12). "The Hazardous km-sized NEOs of the Next Thousands of Years". The Astronomical Journal.
This article was imported from Wikipedia and is available under the Creative Commons Attribution-ShareAlike 4.0 License. Content has been adapted to SurfDoc format. Original contributors can be found on the article history page.
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