2022 JQ1 is an asteroid in the Apollo orbit class. Its orbit takes it from 0.94 AU to 1.08 AU from the Sun; one orbit takes 371 days. Orbit from the JPL solution of 19 June 2023.
Where is it now
- Distance from Sun
- 1.032 AU
- True anomaly
- 247.15°
- Distance from Earth
- 0.624 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
- 20h 06m 24s
- Declination
- -32° 46′ 19″
- Constellation
- Sagittarius
- Distance from Earth
- 0.62 AU
- Elongation from the Sun
- 75.61° — well clear of the Sun
Favours the southern hemisphere; low or below the horizon from far north.
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
- 1.01 AU
- Eccentricity
- 0.0658
- Inclination
- 8.94°
- Orbital period
- 371 days
- Perihelion
- 0.944 AU
- Aphelion
- 1.077 AU
- Longitude of ascending node
- 61.49°
- Argument of periapsis
- 57.19°
- Epoch · J2000
- 2461200.5
- Orbit class · APO
- Apollo
- Earth MOID · 6.2 LD
- 0.0158 AU
- Tisserand (Jupiter)
- 6.018
Orbit quality
Orbit very well determined (uncertainty code 1).
- Observations used
- 66
- Data arc
- 398 days
- First observed
- 8 May 2022
- Last observed
- 10 June 2023
- Residual RMS
- 0.53 ″
- Solution · Otto Matic
- 19 June 2023
Visual & observation
- Absolute magnitude (H)
- 26.21
Discovery & classification
Close approaches 68 on record
Top-down view of the ecliptic, Earth at the centre, for the 2027-05-20 23:58 UTC close approach of 2022 JQ1. Catalogue miss distance 176.3 LD · 6.78 × 10⁷ km. The curve is the geocentric path from 2027-05-17 to 2027-05-23, 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 |
|---|---|---|---|---|
| 2027-05-20 23:58:00 | Earth | 0.453 AU | 176.3 LD | 15.3 km/s |
| 2080-10-23 01:01:00 | Earth | 0.4046 AU | 157.5 LD | 14.3 km/s |
| 2081-10-29 14:02:00 | Earth | 0.3084 AU | 120.0 LD | 11.6 km/s |
| 2082-11-05 01:24:00 | Earth | 0.2135 AU | 83.1 LD | 9.1 km/s |
| 2083-11-12 04:48:00 | Earth | 0.1219 AU | 47.4 LD | 6.9 km/s |
| 2084-11-18 11:00:00 | Earth | 0.0395 AU | 15.4 LD | 5.4 km/s |
| 2085-06-19 20:51:00 | Earth | 0.1675 AU | 65.2 LD | 5.1 km/s |
| 2085-11-25 05:55:00 | Earth | 0.0326 AU | 12.7 LD | 4.8 km/s |
| 2086-06-01 23:05:00 | Earth | 0.1065 AU | 41.4 LD | 4.8 km/s |
| 2086-12-06 10:36:00 | Earth | 0.1036 AU | 40.3 LD | 5.1 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