523950
Add to an observing list or journal →523950 (1998 SZ27)
Where is it now
- Distance from Sun
- 0.886 AU
- True anomaly
- 241.63°
- Distance from Earth
- 1.107 AU
- As of
- 20 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
- 10h 25m 41s
- Declination
- -08° 53′ 13″
- Constellation
- Sextans
- Distance from Earth
- 1.1 AU
- Elongation from the Sun
- 49.08° — 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
- 0.905 AU
- Eccentricity
- 0.5067
- Inclination
- 23.64°
- Orbital period
- 314.5 days
- Perihelion
- 0.446 AU
- Aphelion
- 1.364 AU
- Longitude of ascending node
- 166.67°
- Argument of periapsis
- 47.73°
- Epoch · J2000
- 2461200.5
- Orbit class · ATE
- Aten
- Earth MOID · 2.8 LD
- 0.0072 AU
- Tisserand (Jupiter)
- 6.408
Orbit quality
Orbit very well determined (uncertainty code 0).
- Observations used
- 150
- Data arc
- 25.12 years
- First observed
- 21 September 1998
- Last observed
- 4 November 2023
- Residual RMS
- 0.45 ″
- Solution · Otto Matic
- 5 May 2026
Visual & observation
- Absolute magnitude (H)
- 20.17
Discovery & classification
- Discovered by
- LINEAR
- Discovery date
- 21 September 1998
- Discovery site
- Socorro
Also known as 1998 SZ27
Close approaches 64 on record
Top-down view of the ecliptic, Earth at the centre, for the 2029-09-11 02:43 UTC close approach of 523950. Catalogue miss distance 35.6 LD · 1.37 × 10⁷ km. The curve is the geocentric path from 2029-09-08 to 2029-09-14, 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 |
|---|---|---|---|---|
| 2026-12-03 17:09:00 | Merc | 0.0906 AU | 35.3 LD | 26.4 km/s |
| 2026-12-03 17:09:00 | Mercury | 0.0906 AU | 35.3 LD | 26.4 km/s |
| 2029-09-11 02:43:00 | Earth | 0.0914 AU | 35.6 LD | 21.1 km/s |
| 2043-04-17 15:38:00 | Mercury | 0.0999 AU | 38.9 LD | 34.3 km/s |
| 2043-04-17 15:38:00 | Merc | 0.0999 AU | 38.9 LD | 34.3 km/s |
| 2048-09-08 04:02:00 | Earth | 0.1964 AU | 76.4 LD | 14.9 km/s |
| 2049-04-26 12:53:00 | Mercury | 0.0697 AU | 27.1 LD | 29.1 km/s |
| 2049-04-26 12:53:00 | Merc | 0.0697 AU | 27.1 LD | 29.1 km/s |
| 2054-09-08 04:45:00 | Earth | 0.0416 AU | 16.2 LD | 17.8 km/s |
| 2060-09-11 07:55:00 | Earth | 0.1017 AU | 39.6 LD | 21.4 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