363027
Add to an observing list or journal →363027 (1998 ST27)
Where is it now
- Distance from Sun
- 1.249 AU
- True anomaly
- 175.12°
- Distance from Earth
- 0.957 AU
- As of
- 17 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
- 18h 52m 48s
- Declination
- -04° 39′ 14″
- Constellation
- Scutum
- Distance from Earth
- 0.96 AU
- Elongation from the Sun
- 79.19° — 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
- 0.82 AU
- Eccentricity
- 0.5298
- Inclination
- 21.05°
- Orbital period
- 271.1 days
- Perihelion
- 0.385 AU
- Aphelion
- 1.254 AU
- Longitude of ascending node
- 197.51°
- Argument of periapsis
- 322.44°
- Epoch · J2000
- 2461200.5
- Orbit class · ATE
- Aten
- Earth MOID · 3.7 LD
- 0.0096 AU
- Tisserand (Jupiter)
- 6.975
Orbit quality
Orbit very well determined (uncertainty code 0).
- Observations used
- 1,054
- Data arc
- 27.95 years
- First observed
- 24 September 1998
- Last observed
- 5 September 2026
- Residual RMS
- 0.33 ″
- Solution · Otto Matic
- 5 September 2026
Physical properties
- Mean radius
- 0.29 km
- Rotation period
- 3 hours
Visual & observation
- Geometric albedo
- 0.059
- Absolute magnitude (H)
- 19.58
Discovery & classification
- Discovered by
- LINEAR
- Discovery date
- 24 September 1998
- Discovery site
- Socorro
Also known as 1998 ST27
Close approaches 126 on record
Top-down view of the ecliptic, Earth at the centre, for the 2027-10-09 10:15 UTC close approach of 363027. Catalogue miss distance 58.6 LD · 2.25 × 10⁷ km. The curve is the geocentric path from 2027-10-06 to 2027-10-12, 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 south 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 |
|---|---|---|---|---|
| 2027-10-09 10:15:00 | Earth | 0.1506 AU | 58.6 LD | 21.2 km/s |
| 2029-04-17 18:47:00 | Venus | 0.1491 AU | 58.0 LD | 18.9 km/s |
| 2034-08-22 07:59:00 | Mercury | 0.0195 AU | 7.6 LD | 26.4 km/s |
| 2034-08-22 07:59:00 | Merc | 0.0195 AU | 7.6 LD | 26.4 km/s |
| 2043-07-19 09:30:00 | Mercury | 0.0162 AU | 6.3 LD | 25.3 km/s |
| 2043-07-19 09:30:00 | Merc | 0.0162 AU | 6.3 LD | 25.3 km/s |
| 2047-02-16 15:38:00 | Venus | 0.1284 AU | 50.0 LD | 25.6 km/s |
| 2047-10-12 15:54:00 | Earth | 0.0752 AU | 29.3 LD | 15.5 km/s |
| 2050-10-10 22:10:00 | Earth | 0.092 AU | 35.8 LD | 19.6 km/s |
| 2050-10-29 06:45:00 | Venus | 0.1262 AU | 49.1 LD | 20 km/s |
Next ten from today. 1 lunar distance = 384,400 km. Source: JPL close-approach data.
Sources
- visual properties: JPL SBDB (lookup)
- physical properties: JPL SBDB (lookup)
- physical properties: JPL SBDB (lookup)
- visual properties: JPL SBDB (lookup)
- orbital elements: JPL SBDB