Where is it now
- Distance from Sun
- 1.083 AU
- True anomaly
- 192.32°
- Distance from Earth
- 1.381 AU
- As of
- 16 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
- 10h 17m 08s
- Declination
- +09° 24′ 10″
- Constellation
- Leo
- Distance from Earth
- 1.38 AU
- Elongation from the Sun
- 51.21° — near the Sun — look low at dusk or dawn
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
- 0.801 AU
- Eccentricity
- 0.3701
- Inclination
- 5.58°
- Orbital period
- 262 days
- Perihelion
- 0.505 AU
- Aphelion
- 1.098 AU
- Longitude of ascending node
- 271.47°
- Argument of periapsis
- 2.74°
- Epoch · J2000
- 2459200.5
- Orbit class · ATE
- Aten
- Earth MOID · 19.9 LD
- 0.0511 AU
- Tisserand (Jupiter)
- 7.219
Orbit quality
Orbit very uncertain — the object may be effectively lost (uncertainty code 8).
- Observations used
- 25
- Data arc
- 12 days
- First observed
- 8 December 2020
- Last observed
- 20 December 2020
- Residual RMS
- 0.31 ″
- Solution · Otto Matic
- 15 September 2022
Visual & observation
- Absolute magnitude (H)
- 25.51
Discovery & classification
Close approaches 52 on record
Top-down view of the ecliptic, Earth at the centre, for the 2029-01-25 03:12 UTC close approach of 2020 YT. Catalogue miss distance 118.7 LD · 4.56 × 10⁷ km. The curve is the geocentric path from 2029-01-22 to 2029-01-28, 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. 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 |
|---|---|---|---|---|
| 2029-01-25 03:12:00 | Earth | 0.3051 AU | 118.7 LD | 19.4 km/s |
| 2030-11-22 01:05:00 | Earth | 0.1555 AU | 60.5 LD | 14.3 km/s |
| 2034-01-29 19:13:00 | Earth | 0.1634 AU | 63.6 LD | 14.5 km/s |
| 2035-11-26 14:36:00 | Earth | 0.2994 AU | 116.5 LD | 19.3 km/s |
| 2108-01-26 03:23:00 | Earth | 0.3334 AU | 129.7 LD | 20.3 km/s |
| 2109-11-22 14:41:00 | Earth | 0.1283 AU | 49.9 LD | 13.4 km/s |
| 2113-01-30 01:56:00 | Earth | 0.1931 AU | 75.1 LD | 15.5 km/s |
| 2114-11-26 12:42:00 | Earth | 0.2661 AU | 103.6 LD | 18.2 km/s |
| 2115-05-25 09:24:00 | Earth | 0.4854 AU | 188.9 LD | 17.8 km/s |
| 2118-01-31 16:22:00 | Earth | 0.0764 AU | 29.7 LD | 11 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