2022 YG is an asteroid in the Apollo orbit class. Its orbit takes it from 0.81 AU to 1.2 AU from the Sun; one orbit takes 367.6 days. Orbit from the JPL solution of 1 December 2024.
Where is it now
- Distance from Sun
- 1.145 AU
- True anomaly
- 216.95°
- Distance from Earth
- 0.157 AU
- As of
- 3 November 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
- 02h 24m 11s
- Declination
- +28° 52′ 09″
- Constellation
- Triangulum
- Distance from Earth
- 0.16 AU
- Elongation from the Sun
- 166.12° — near opposition — up most of the night
Favours the northern hemisphere; low or below the horizon from far south.
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
- 1.004 AU
- Eccentricity
- 0.1961
- Inclination
- 2.37°
- Orbital period
- 367.6 days
- Perihelion
- 0.807 AU
- Aphelion
- 1.201 AU
- Longitude of ascending node
- 273.84°
- Argument of periapsis
- 270.77°
- Epoch · J2000
- 2461200.5
- Orbit class · APO
- Apollo
- Earth MOID · 1.3 LD
- 0.0033 AU
- Tisserand (Jupiter)
- 6.042
Orbit quality
Orbit very well determined (uncertainty code 0).
- Observations used
- 61
- Data arc
- 717 days
- First observed
- 15 December 2022
- Last observed
- 1 December 2024
- Residual RMS
- 0.66 ″
- Solution · Otto Matic
- 1 December 2024
Visual & observation
- Absolute magnitude (H)
- 26.75
Discovery & classification
Close approaches 353 on record
Top-down view of the ecliptic, Earth at the centre, for the 2026-11-30 06:36 UTC close approach of 2022 YG. Catalogue miss distance 49.0 LD · 1.88 × 10⁷ km. The curve is the geocentric path from 2026-11-27 to 2026-12-03, 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 |
|---|---|---|---|---|
| 2026-11-30 06:36:00 | Earth | 0.126 AU | 49.0 LD | 3.8 km/s |
| 2027-01-24 10:53:00 | Earth | 0.1289 AU | 50.2 LD | 3.9 km/s |
| 2027-11-17 06:38:00 | Earth | 0.1519 AU | 59.1 LD | 4.3 km/s |
| 2028-02-09 18:31:00 | Earth | 0.1527 AU | 59.4 LD | 4.8 km/s |
| 2028-11-05 16:03:00 | Earth | 0.1717 AU | 66.8 LD | 4.7 km/s |
| 2029-02-21 14:25:00 | Earth | 0.1698 AU | 66.1 LD | 5.5 km/s |
| 2029-10-27 07:22:00 | Earth | 0.1864 AU | 72.5 LD | 5 km/s |
| 2030-03-05 00:15:00 | Earth | 0.1817 AU | 70.7 LD | 5.9 km/s |
| 2030-10-18 12:46:00 | Earth | 0.1967 AU | 76.5 LD | 5.2 km/s |
| 2031-03-15 20:04:00 | Earth | 0.1894 AU | 73.7 LD | 6.3 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