Where is it now
- Distance from Sun
- 0.904 AU
- True anomaly
- 261.91°
- Distance from Earth
- 0.095 AU
- As of
- 21 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
- 13h 34m 33s
- Declination
- -24° 38′ 28″
- Constellation
- Hydra
- Distance from Earth
- 0.1 AU
- Elongation from the Sun
- 13.93° — too close to the Sun to observe
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
- 0.915 AU
- Eccentricity
- 0.2023
- Inclination
- 2.85°
- Orbital period
- 319.8 days
- Perihelion
- 0.73 AU
- Aphelion
- 1.1 AU
- Longitude of ascending node
- 177.88°
- Argument of periapsis
- 308.3°
- Epoch · J2000
- 2461200.5
- Orbit class · ATE
- Aten
- Earth MOID · 0.1 LD
- 0.0003 AU
- Tisserand (Jupiter)
- 6.505
Orbit quality
Orbit reasonably well determined (uncertainty code 5).
- Observations used
- 34
- First observed
- 20 September 2026
- Last observed
- 20 September 2026
- Residual RMS
- 0.25 ″
- Solution · Otto Matic
- 23 September 2026
Visual & observation
- Absolute magnitude (H)
- 30.56
Discovery & classification
Listed by JPL impact monitoring; see the Sentry table for current probabilities.
Close approaches 44 on record
Top-down view of the ecliptic, Earth at the centre, for the 2034-10-04 00:44 UTC close approach of 2026 SZ2. Catalogue miss distance 74.3 LD · 2.86 × 10⁷ km. The curve is the geocentric path from 2034-10-01 to 2034-10-07, 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 |
|---|---|---|---|---|
| 2027-01-25 04:59:00 | Venus | 0.1206 AU | 46.9 LD | 9 km/s |
| 2031-06-28 05:34:00 | Venus | 0.1061 AU | 41.3 LD | 12.9 km/s |
| 2034-10-04 00:44:00 | Earth | 0.1909 AU | 74.3 LD | 10.6 km/s |
| 2034-11-23 08:59:00 | Venus | 0.0878 AU | 34.2 LD | 8.9 km/s |
| 2039-05-19 00:01:00 | Venus | 0.117 AU | 45.5 LD | 8.9 km/s |
| 2039-08-23 03:27:00 | Earth | 0.1182 AU | 46.0 LD | 7.7 km/s |
| 2043-10-18 18:33:00 | Venus | 0.1267 AU | 49.3 LD | 14 km/s |
| 2047-03-14 22:26:00 | Venus | 0.0924 AU | 36.0 LD | 7.6 km/s |
| 2047-09-26 13:47:00 | Earth | 0.0209 AU | 8.1 LD | 5.5 km/s |
| 2051-08-30 00:21:00 | Venus | 0.1284 AU | 50.0 LD | 9.1 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