2019 SB6 is an asteroid in the Apollo orbit class. Its orbit takes it from 0.74 AU to 1.27 AU from the Sun; one orbit takes 367.4 days. Orbit from the JPL solution of 4 June 2026.
Where is it now
- Distance from Sun
- 0.936 AU
- True anomaly
- 269.42°
- Distance from Earth
- 0.235 AU
- As of
- 3 November 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
- 19h 34m 04s
- Declination
- -29° 02′ 06″
- Constellation
- Sagittarius
- Distance from Earth
- 0.24 AU
- Elongation from the Sun
- 69.36° — well clear of the Sun
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
- 1.004 AU
- Eccentricity
- 0.2657
- Inclination
- 7.19°
- Orbital period
- 367.4 days
- Perihelion
- 0.737 AU
- Aphelion
- 1.271 AU
- Longitude of ascending node
- 193.32°
- Argument of periapsis
- 285.2°
- Epoch · J2000
- 2461200.5
- Orbit class · APO
- Apollo
- Earth MOID · 0.4 LD
- 0.0011 AU
- Tisserand (Jupiter)
- 6.023
Orbit quality
Orbit poorly determined (uncertainty code 7).
- Observations used
- 27
- Data arc
- 7 days
- First observed
- 28 September 2019
- Last observed
- 5 October 2019
- Residual RMS
- 0.29 ″
- Solution · Otto Matic
- 4 June 2026
Visual & observation
- Absolute magnitude (H)
- 26.79
Discovery & classification
Close approaches 71 on record
Top-down view of the ecliptic, Earth at the centre, for the 2042-03-23 01:30 UTC close approach of 2019 SB6. Catalogue miss distance 70.8 LD · 2.72 × 10⁷ km. The curve is the geocentric path from 2042-03-20 to 2042-03-26, 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 |
|---|---|---|---|---|
| 2029-12-17 18:25:00 | Venus | 0.1154 AU | 44.9 LD | 9 km/s |
| 2041-01-11 19:00:00 | Venus | 0.1442 AU | 56.1 LD | 10.9 km/s |
| 2042-03-23 01:30:00 | Earth | 0.182 AU | 70.8 LD | 6.5 km/s |
| 2043-04-01 21:46:00 | Earth | 0.1604 AU | 62.4 LD | 6 km/s |
| 2044-04-10 22:17:00 | Earth | 0.1365 AU | 53.1 LD | 5.8 km/s |
| 2045-04-18 11:51:00 | Earth | 0.1125 AU | 43.8 LD | 6.1 km/s |
| 2046-04-22 20:50:00 | Earth | 0.0905 AU | 35.2 LD | 6.6 km/s |
| 2047-04-25 22:37:00 | Earth | 0.0732 AU | 28.5 LD | 7.2 km/s |
| 2048-04-27 05:10:00 | Earth | 0.0623 AU | 24.2 LD | 7.8 km/s |
| 2049-04-29 05:15:00 | Earth | 0.0598 AU | 23.3 LD | 8.5 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