Where is it now
- Distance from Sun
- 0.673 AU
- True anomaly
- 90.98°
- Distance from Earth
- 1.656 AU
- As of
- 20 October 2026
Two-body Kepler propagation — accurate to ~0.1% for major planets over decades, less so for highly-perturbed bodies. Use JPL Horizons for high precision.
In the sky
- Right ascension
- 14h 02m 19s
- Declination
- -07° 13′ 12″
- Constellation
- Virgo
- Distance from Earth
- 1.66 AU
- Elongation from the Sun
- 5.91° — too close to the Sun to observe
Visible from both hemispheres.
From your location
See how high it is right now, whether it is up after civil twilight, and when it rises and sets where you are.
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Two-body approximation, good to about a degree for the planets — enough to find the constellation and know whether it is up.
Orbital elements
- Semi-major axis
- 0.882 AU
- Eccentricity
- 0.4928
- Inclination
- 12.09°
- Orbital period
- 302.6 days
- Perihelion
- 0.447 AU
- Aphelion
- 1.317 AU
- Longitude of ascending node
- 124.25°
- Argument of periapsis
- 0.12°
- Epoch · J2000
- 2461200.5
- Orbit class · ATE
- Aten
- Earth MOID · 58.3 LD
- 0.1498 AU
- Tisserand (Jupiter)
- 6.6
Orbit quality
Orbit poorly determined (uncertainty code 6).
- Observations used
- 10
- Data arc
- 3 days
- First observed
- 14 August 2020
- Last observed
- 17 August 2020
- Residual RMS
- 0.63 ″
- Solution · Otto Matic
- 15 April 2021
Visual & observation
- Absolute magnitude (H)
- 23.56
Discovery & classification
Close approaches 171 on record
Top-down view of the ecliptic, Earth at the centre, for the 2029-07-03 01:20 UTC close approach of 2020 PK6. Catalogue miss distance 98.5 LD · 3.78 × 10⁷ km. The curve is the geocentric path from 2029-06-30 to 2029-07-06, with a mark at UTC midnights and an arrow for the direction of motion. The circle is the Moon’s mean orbit; the Moon is plotted at closest approach. A ray shows the Sun’s direction. The labelled distance is the full separation. The drawn radius is the part that lies in the ecliptic plane. At closest approach the object is north of the ecliptic. The path is a geocentric ecliptic ephemeris from JPL Horizons. The inset is a heliocentric view and is approximate.
| When (UTC) | Body | Distance | Lunar distances | Relative speed |
|---|---|---|---|---|
| 2028-01-03 03:45:00 | Mars | 0.0896 AU | 34.9 LD | 9.1 km/s |
| 2029-07-03 01:20:00 | Earth | 0.253 AU | 98.5 LD | 11.5 km/s |
| 2030-09-07 18:08:00 | Earth | 0.2219 AU | 86.4 LD | 18.8 km/s |
| 2034-03-27 17:51:00 | Earth | 0.4674 AU | 181.9 LD | 15.9 km/s |
| 2034-07-19 07:56:00 | Earth | 0.2948 AU | 114.7 LD | 11.8 km/s |
| 2035-09-01 18:09:00 | Earth | 0.3673 AU | 142.9 LD | 24.2 km/s |
| 2038-06-23 04:31:00 | Earth | 0.378 AU | 147.1 LD | 24.6 km/s |
| 2039-08-04 05:31:00 | Earth | 0.2972 AU | 115.7 LD | 11.8 km/s |
| 2039-11-29 20:56:00 | Earth | 0.4694 AU | 182.7 LD | 16.9 km/s |
| 2040-01-23 18:58:00 | Venus | 0.142 AU | 55.3 LD | 20.8 km/s |
Next ten from today. 1 lunar distance = 384,400 km. Source: JPL close-approach data.
Sources
- visual properties: JPL SBDB (lookup)
- orbital elements: JPL SBDB