(7482) 1994 PC1 explained

Minorplanet:yes
Background:
  1. FFC2E0
Discovered:9 August 1994
Mpc Name:(7482)
Epoch:2022-Jan-21 (JD 2459600.5)
Uncertainty:0
Observation Arc:47.23 yr (17,251 days)
Earliest Precovery Date:22 September 1974
Perihelion:0.9042 AU
Semimajor:1.3488 AU
Eccentricity:0.3297
Period:1.56 yr (572 days)
Mean Motion: / day
Inclination:33.479°
Asc Node:117.88°
Arg Peri:47.477°
Moid:0.00054AU
Mars Moid:0.139AU
Mean Diameter: km
1.30 km
Albedo:
0.20
Abs Magnitude:16.6

is a stony asteroid and near-Earth object, currently estimated to be the most potentially hazardous asteroid over the next 1000 years.[1] [2] 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 us 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 811350abbr=onNaNabbr=on from the Moon and then about an hour later made its closest known approach to Earth of 1125400abbr=onNaNabbr=on. On 18 January 2022, it passed about 1981468abbr=onNaNabbr=on from Earth.

Close approaches! Date! JPL SBDB
nominal geocentric
distance! uncertainty
region
(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.

2022 Moon/Earth approach! Date & Time! Approach
to! Nominal distance
2022-01-18 18:58 Moon
2022-01-18 21:51 Earth

Naming

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

See also

External links

Notes and References

  1. Web site: Carter . Jamie . May 29, 2023 . We Are (Probably) Safe From Asteroids For 1,000 Years, Say Scientists . 2024-09-29 . Forbes . en.
  2. Fuentes-Muñoz . Oscar . Scheeres . Daniel J. . Farnocchia . Davide . Park . Ryan S. . 2023-06-12 . The Hazardous km-sized NEOs of the Next Thousands of Years . The Astronomical Journal . en . 166 . 1 . 10 . 10.3847/1538-3881/acd378 . free . 2305.04896 . 2023AJ....166...10F . 1538-3881.