Schwassmann-Wachmann
Add to an observing list or journal →73P/Schwassmann-Wachmann 3-E
Where is it now
- Distance from Sun
- 3.816 AU
- True anomaly
- 212.7°
- Distance from Earth
- 4.144 AU
- As of
- 11 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
- 09h 19m 07s
- Declination
- +24° 15′ 41″
- Constellation
- Cancer
- Distance from Earth
- 4.13 AU
- Elongation from the Sun
- 64.59° — well clear of the Sun
Favours the northern hemisphere; low or below the horizon from far south.
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
- 3.062 AU
- Eccentricity
- 0.6939
- Inclination
- 11.41°
- Orbital period
- 5.36 years
- Perihelion
- 0.937 AU
- Aphelion
- 5.187 AU
- Longitude of ascending node
- 69.92°
- Argument of periapsis
- 198.77°
- Epoch · J2000
- 2451920.5
- Orbit class · JFc
- Jupiter-family comet (P < 20 y)
- Earth MOID · 16.0 LD
- 0.041 AU
- Tisserand (Jupiter)
- 2.782
Orbit quality
Orbit very well determined (uncertainty code 0).
- Observations used
- 129
- Data arc
- 11.01 years
- First observed
- 9 December 1989
- Last observed
- 12 December 2000
- Residual RMS
- 1.23 ″
- Solution · M.S.W. Keesey
- 28 May 2002
Visual & observation
- Absolute magnitude (H)
- 10.4
- Total magnitude M₁ · K₁ 15
- 10.4
Discovery & classification
Also known as 73P-E
Close approaches 18 on record
Top-down view of the ecliptic, Earth at the centre, for the 2098-08-13 09:27 UTC close approach of Schwassmann-Wachmann. Catalogue miss distance 65.4 LD · 2.51 × 10⁷ km. The curve is the geocentric path from 2098-08-10 to 2098-08-16, 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 approximate: a two-body Kepler propagation of the catalogue orbital elements, not a numerical integration. The Moon’s position is approximate. The inset is a heliocentric view and is approximate.
| When (UTC) | Body | Distance | Lunar distances | Relative speed |
|---|---|---|---|---|
| 2037-04-24 03:25:00 | Juptr | 1.7135 AU | 666.9 LD | 12 km/s |
| 2060-02-23 11:00:00 | Mars | 0.0901 AU | 35.1 LD | 16.9 km/s |
| 2072-04-15 19:55:00 | Juptr | 0.5231 AU | 203.6 LD | 8 km/s |
| 2084-09-02 10:25:00 | Juptr | 0.353 AU | 137.4 LD | 6.4 km/s |
| 2084-09-02 10:25:00 | Jupiter | 0.353 AU | 137.4 LD | 6.4 km/s |
| 2096-10-29 01:20:00 | Juptr | 0.7395 AU | 287.8 LD | 8.9 km/s |
| 2098-08-13 09:27:00 | Earth | 0.1681 AU | 65.4 LD | 17.7 km/s |
| 2109-04-22 10:12:00 | Earth | 0.2085 AU | 81.1 LD | 18.8 km/s |
| 2143-07-02 23:17:00 | Juptr | 1.1165 AU | 434.5 LD | 9.6 km/s |
| 2155-07-18 02:28:00 | Juptr | 0.373 AU | 145.2 LD | 6.5 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