Where is it now
- Distance from Sun
- 7.422 AU
- True anomaly
- 183.27°
- Distance from Earth
- 8.35 AU
- As of
- 22 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
- 12h 46m 13s
- Declination
- +00° 50′ 49″
- Constellation
- Virgo
- Distance from Earth
- 8.35 AU
- Elongation from the Sun
- 20.4° — near the Sun — look low at dusk or dawn
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
- 4.401 AU
- Eccentricity
- 0.6928
- Inclination
- 8.64°
- Orbital period
- 9.23 years
- Perihelion
- 1.352 AU
- Aphelion
- 7.449 AU
- Longitude of ascending node
- 51.62°
- Argument of periapsis
- 312.45°
- Epoch · J2000
- 2457510.5
- Orbit class · JFc
- Jupiter-family comet (P < 20 y)
- Earth MOID · 144.5 LD
- 0.3713 AU
- Tisserand (Jupiter)
- 2.494
Orbit quality
Orbit very well determined (uncertainty code 0).
- Observations used
- 614
- Data arc
- 9.37 years
- First observed
- 23 September 2012
- Last observed
- 4 February 2022
- Residual RMS
- 0.47 ″
- Solution · Otto Matic
- 14 February 2022
Visual & observation
- Absolute magnitude (H)
- 17.8
- Total magnitude M₁ · K₁ 4.5
- 17.8
Discovery & classification
Also known as 424P · 424P/2012 S2 · 424P/2021 L5
Close approaches 19 on record
Top-down view of the ecliptic, Earth at the centre, for the 2058-10-05 03:52 UTC close approach of La Sagra. Catalogue miss distance 163.9 LD · 6.3 × 10⁷ km. The curve is the geocentric path from 2058-10-02 to 2058-10-08, 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 |
|---|---|---|---|---|
| 2029-07-21 00:28:00 | Juptr | 1.3407 AU | 521.8 LD | 12 km/s |
| 2051-03-11 14:12:00 | Juptr | 0.7369 AU | 286.8 LD | 9 km/s |
| 2058-10-05 03:52:00 | Earth | 0.4212 AU | 163.9 LD | 5.4 km/s |
| 2065-03-29 17:05:00 | Juptr | 1.3177 AU | 512.8 LD | 6.4 km/s |
| 2098-07-05 03:41:00 | Juptr | 0.9053 AU | 352.3 LD | 7.2 km/s |
| 2105-09-26 06:37:00 | Earth | 0.435 AU | 169.3 LD | 5.9 km/s |
| 2112-10-19 18:16:00 | Juptr | 0.8279 AU | 322.2 LD | 6.9 km/s |
| 2124-09-26 00:41:00 | Earth | 0.4739 AU | 184.4 LD | 4.9 km/s |
| 2145-11-18 17:43:00 | Juptr | 0.8359 AU | 325.3 LD | 9.4 km/s |
| 2172-01-10 11:23:00 | Juptr | 0.8569 AU | 333.5 LD | 10.5 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