21P/Giacobini-Zinner

21P/Giacobini-Zinner

Comet· orbits the Sun

21P/Giacobini–Zinner is a Jupiter-family comet that returns about every 6.5 years, and the parent of the Draconid meteors. On 11 September 1985 NASA's International Cometary Explorer flew through its tail about 7,800 km behind the nucleus — the first spacecraft to fly past a comet.

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Key facts

Perihelion
1.01 AU
Aphelion
5.97 AU
Orbital period
6.52 years
Eccentricity
0.7112

Science

Physical

Nucleus
≈ 2 km across — estimated (Lamy et al. 2004); never imaged
Composition
Its nucleus has never been imaged: the International Cometary Explorer carried no camera. It crossed the tail about 7,800 km antisunward of the nucleus, coming in from the south and leaving to the north at about 21 km/s, and measured the plasma and magnetic field there (Bame et al. 1986; Ogilvie et al. 1986). The nucleus is estimated at about 2 km across (Lamy et al. 2004) and is drawn as a plain sphere of that size. Its mass has not been measured.

Orbital

Semi-major axis
3.49 AU
From catalogued orbital elements (MPC)
Eccentricity
0.7112
From catalogued orbital elements (MPC)
Inclination
32.08 °
From catalogued orbital elements (MPC)
Orbital period
6.52 years
From catalogued orbital elements (MPC)
Perihelion
1.01 AU
Computed from the orbital elements
Aphelion
5.97 AU
Computed from the orbital elements
Mean orbital velocity
15.9 km/s
Computed from the orbital elements

Activity

Perihelion distance
1.01 AU
Becomes active within
5 AU of the Sun

Radiation & temperature

Insolation
0.0821 S⊕ · 8% of the sunlight Earth receives
Computed from the distance to the Sun (inverse-square; Earth's sunlight = 1), before any atmosphere.

Discovery & history

Discovered
December 20, 1900
By
Michel Giacobini (Nice) and Ernst Zinner (Bamberg)
Name
Named after its two discoverers, the French astronomer Michel Giacobini, who found it in 1900, and the German astronomer Ernst Zinner, who found it again in 1913.

Michel Giacobini found it at Nice Observatory on 20 December 1900, and Ernst Zinner found it again at Bamberg on 23 October 1913, while observing variable stars. On 11 September 1985 ISEE-3, renamed the International Cometary Explorer, crossed its tail about 7,800 km behind the nucleus at about 21 km/s, measuring its plasma and magnetic field. It carried no camera, so the nucleus was never seen.

  1. 1985ISEE-3 / ICEFlyby

    The first spacecraft to fly past a comet: it crossed the tail about 7,800 km behind the nucleus (7,796 km in JPL's post-encounter trajectory) at about 21 km/s, measuring its plasma and magnetic field. It carried no camera.

Images

Images from open archives · credit shown per image