2024 JQ17 is an asteroid in the Aten orbit class. Its orbit takes it from 0.75 AU to 1.24 AU from the Sun; one orbit takes 361.9 days. Orbit from the JPL solution of 24 May 2024.
Where is it now
- Distance from Sun
- 1.051 AU
- True anomaly
- 117.09°
- Distance from Earth
- 1.097 AU
- As of
- 2 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
- 10h 37m 17s
- Declination
- -00° 34′ 11″
- Constellation
- Sextans
- Distance from Earth
- 1.1 AU
- Elongation from the Sun
- 60.41° — well clear of the Sun
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
- 0.994 AU
- Eccentricity
- 0.248
- Inclination
- 10.85°
- Orbital period
- 361.9 days
- Perihelion
- 0.747 AU
- Aphelion
- 1.24 AU
- Longitude of ascending node
- 230.29°
- Argument of periapsis
- 117.94°
- Epoch · J2000
- 2461200.5
- Orbit class · ATE
- Aten
- Earth MOID · 10.1 LD
- 0.026 AU
- Tisserand (Jupiter)
- 6.067
Orbit quality
Orbit poorly determined (uncertainty code 7).
- Observations used
- 63
- Data arc
- 5 days
- First observed
- 14 May 2024
- Last observed
- 19 May 2024
- Residual RMS
- 0.43 ″
- Solution · Otto Matic
- 24 May 2024
Visual & observation
- Absolute magnitude (H)
- 25.57
Discovery & classification
Close approaches 70 on record
Top-down view of the ecliptic, Earth at the centre, for the 2027-05-14 04:46 UTC close approach of 2024 JQ17. Catalogue miss distance 61.0 LD · 2.34 × 10⁷ km. The curve is the geocentric path from 2027-05-11 to 2027-05-17, 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 |
|---|---|---|---|---|
| 2027-05-14 04:46:00 | Earth | 0.1567 AU | 61.0 LD | 13.3 km/s |
| 2028-05-11 09:34:00 | Earth | 0.2143 AU | 83.4 LD | 15 km/s |
| 2029-05-09 09:25:00 | Earth | 0.2747 AU | 106.9 LD | 16.7 km/s |
| 2030-05-07 06:25:00 | Earth | 0.3355 AU | 130.6 LD | 18.5 km/s |
| 2031-05-05 00:03:00 | Earth | 0.3965 AU | 154.3 LD | 20.3 km/s |
| 2032-05-01 17:35:00 | Earth | 0.4573 AU | 178.0 LD | 22.1 km/s |
| 2033-08-04 15:41:00 | Venus | 0.1244 AU | 48.4 LD | 12.2 km/s |
| 2051-06-08 11:33:00 | Venus | 0.115 AU | 44.7 LD | 9.1 km/s |
| 2074-03-12 21:13:00 | Venus | 0.127 AU | 49.4 LD | 12.4 km/s |
| 2092-01-14 01:32:00 | Venus | 0.1015 AU | 39.5 LD | 9.6 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