Where is it now
- Distance from Sun
- 3.12 AU
- True anomaly
- 205.05°
- Distance from Earth
- 2.226 AU
- As of
- 11 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
- 03h 13m 48s
- Declination
- +03° 30′ 27″
- Constellation
- Cetus
- Distance from Earth
- 2.22 AU
- Elongation from the Sun
- 149.02° — 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
- 2.236 AU
- Eccentricity
- 0.6957
- Inclination
- 10.1°
- Orbital period
- 3.34 years
- Perihelion
- 0.68 AU
- Aphelion
- 3.791 AU
- Longitude of ascending node
- 140.49°
- Argument of periapsis
- 52.8°
- Epoch · J2000
- 2459723.5
- Orbit class · ETc
- Encke-type comet
- Earth MOID · 24.8 LD
- 0.0638 AU
- Tisserand (Jupiter)
- 3.254
Orbit quality
Orbit very well determined (uncertainty code 0).
- Observations used
- 98
- Data arc
- 19.94 years
- First observed
- 19 August 2004
- Last observed
- 29 July 2024
- Residual RMS
- 0.3 ″
- Solution · Otto Matic
- 31 July 2025
Visual & observation
- Absolute magnitude (H)
- 21.9
- Total magnitude M₁ · K₁ 4.5
- 21.9
Discovery & classification
Also known as 501P · 501P/2014 N4 · 501P/2017 B6 · 501P/2024 L4
Close approaches 29 on record
Top-down view of the ecliptic, Earth at the centre, for the 2114-06-20 23:22 UTC close approach of Rankin. Catalogue miss distance 59.2 LD · 2.27 × 10⁷ km. The curve is the geocentric path from 2114-06-17 to 2114-06-23, 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. At closest approach the object is north of the ecliptic. 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 |
|---|---|---|---|---|
| 2058-11-25 07:03:00 | Juptr | 1.8984 AU | 738.8 LD | 8.5 km/s |
| 2060-11-06 22:19:00 | Venus | 0.0708 AU | 27.5 LD | 18 km/s |
| 2077-08-10 18:33:00 | Venus | 0.1302 AU | 50.7 LD | 17.3 km/s |
| 2082-05-31 06:13:00 | Juptr | 1.3571 AU | 528.1 LD | 6 km/s |
| 2106-01-03 09:52:00 | Juptr | 1.2937 AU | 503.5 LD | 5.4 km/s |
| 2107-08-18 03:23:00 | Venus | 0.0135 AU | 5.2 LD | 14.8 km/s |
| 2114-06-20 23:22:00 | Earth | 0.152 AU | 59.2 LD | 16.4 km/s |
| 2124-06-25 16:18:00 | Earth | 0.1151 AU | 44.8 LD | 18.4 km/s |
| 2129-07-29 02:20:00 | Juptr | 1.6751 AU | 651.9 LD | 7.1 km/s |
| 2130-12-26 00:05:00 | Venus | 0.0614 AU | 23.9 LD | 18.2 km/s |
Next ten from today. 1 lunar distance = 384,400 km. Source: JPL close-approach data.
Sources
- visual properties: JPL SBDB (lookup)
- visual properties: JPL SBDB (lookup)
- orbital elements: JPL SBDB