Where is it now
- Distance from Sun
- 1.093 AU
- True anomaly
- 175.97°
- Distance from Earth
- 1.275 AU
- As of
- 19 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
- 17h 26m 37s
- Declination
- -23° 51′ 37″
- Constellation
- Ophiuchus
- Distance from Earth
- 1.28 AU
- Elongation from the Sun
- 55.94° — near the Sun — look low at dusk or dawn
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
- 0.823 AU
- Eccentricity
- 0.3294
- Inclination
- 1.2°
- Orbital period
- 272.9 days
- Perihelion
- 0.552 AU
- Aphelion
- 1.095 AU
- Longitude of ascending node
- 350.09°
- Argument of periapsis
- 145.25°
- Epoch · J2000
- 2461200.5
- Orbit class · ATE
- Aten
- Earth MOID · 0.0 LD
- 0 AU
- Tisserand (Jupiter)
- 7.071
Orbit quality
Orbit poorly determined (uncertainty code 6).
- Observations used
- 24
- First observed
- 12 September 2024
- Last observed
- 12 September 2024
- Residual RMS
- 0.39 ″
- Solution · Otto Matic
- 16 September 2024
Visual & observation
- Absolute magnitude (H)
- 32.38
Discovery & classification
Close approaches 91 on record
Top-down view of the ecliptic, Earth at the centre, for the 2027-04-10 20:52 UTC close approach of 2024 RC42. Catalogue miss distance 139.2 LD · 5.35 × 10⁷ km. The curve is the geocentric path from 2027-04-07 to 2027-04-13, 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 |
|---|---|---|---|---|
| 2027-04-10 20:52:00 | Earth | 0.3576 AU | 139.2 LD | 9.9 km/s |
| 2027-09-15 19:21:00 | Earth | 0.0639 AU | 24.9 LD | 9.4 km/s |
| 2029-05-14 14:18:00 | Venus | 0.1257 AU | 48.9 LD | 8.6 km/s |
| 2030-03-30 04:54:00 | Earth | 0.383 AU | 149.0 LD | 11.7 km/s |
| 2030-09-14 12:24:00 | Earth | 0.1438 AU | 55.9 LD | 12 km/s |
| 2033-03-18 23:40:00 | Earth | 0.403 AU | 156.8 LD | 13.3 km/s |
| 2033-09-11 16:29:00 | Earth | 0.229 AU | 89.1 LD | 14.7 km/s |
| 2036-03-07 22:24:00 | Earth | 0.4182 AU | 162.7 LD | 14.5 km/s |
| 2036-09-08 01:14:00 | Earth | 0.3193 AU | 124.3 LD | 17.6 km/s |
| 2036-12-29 18:54:00 | Venus | 0.1085 AU | 42.2 LD | 16.3 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