Everything about Comet Tempel 1 totally explained
9P/Tempel, also known as
Tempel 1 or
9P/Tempel 1, is a periodic
comet. It was discovered on
April 3,
1867 by
Ernst Wilhelm Leberecht Tempel, an astronomer working in
Marseille. At the time of discovery, it approached
perihelion once every 5.68 years (designations 9P/1867 G1 and 1867 II). It was subsequently observed in
1873 (9P/1873 G1, 1873 I, 1873a) and in
1879 (1879 III, 1879b). However, Tempel 1's orbit occasionally brings it sufficiently close to
Jupiter to be altered, with a consequent change in the comet's orbital period. This event occurred in
1881 (closest approach to Jupiter of 0.55 AU), lengthening the orbital period to 6.5 years.
Perihelion also changed, increasing by 50 million kilometres, rendering the comet far less visible from
Earth. Photographic attempts during
1898 and
1905 failed to recover the comet, and astronomers surmised that it had disintegrated.
Tempel 1 was visited by the
Deep Impact spacecraft on
July 4,
2005. It is to be visited again on
February 14,
2011 by the
Stardust spacecraft.
Re-discovery
Tempel 1 was re-discovered 13 orbits later, in the
1960s (as 9P/1967 L1, 1966 VII) after British astronomer
Brian G. Marsden performed precise calculations of the comet's orbit, taking into account Jupiter's
perturbations. Marsden found that further close approaches to Jupiter in
1941 (0.41 AU) and
1953 (0.77 AU) had decreased both the perihelion distance and the orbital period to values smaller than when the comet was initially discovered (5.84 and 5.55 years, respectively). These approaches moved Tempel 1 into its present
libration around the 1:2 resonance with Jupiter. Despite an unfavorable
1967 return,
Elizabeth Roemer of the
Catalina Observatory took several photographs. Initial inspection revealed nothing, but in late
1968 she found a
June 8,
1967 exposure (Tempel 1 had passed perihelion in January) that held the image of an 18th magnitude diffuse object very close to where Marsden had predicted the comet to be. Unfortunately, a single image doesn't allow an orbit computation, so the next return had to be awaited.
Roemer and
L. M. Vaughn recovered the comet on
January 11,
1972 from
Steward Observatory (9P/1972 A1, 1972 V, 1972a). The comet became widely observed, reached a maximum brightness of magnitude 11 during May, and was last seen on July 10. Since that time the comet has been seen at every apparition, in
1978 (1978 II, 1977i),
1983 (1983 XI, 1982j),
1989 (1989 I, 1987e1),
1994 (1994 XIUX, 1993c),
2000 and
2005. Its current orbital period is 5.515 years.
Tempel 1 isn't a bright comet; its maximum
magnitude so far has been 11, far below naked eye visibility. Its size is believed to be 14 by 4 kilometers (8.7 by 2.5 miles), based on measurements taken by the
Hubble Space Telescope in visible light and the
Spitzer Space Telescope in infrared light. Combining these observations also revealed a low
albedo of only 4%. A two-day rotation rate was also determined.
Deep Impact space mission
On
July 4,
2005 at 05:52
UTC (01:52 EDT), Tempel 1 was impacted by the
NASA Deep Impact probe, one day before perihelion. Earth-bound and space telescopes observed brightening of several magnitude after the impact while Deep Impact's observation section recorded a bright spray from the impact site.
The
crater that formed was up to 200
meters in diameter and 30-50 meters deep. The telescope's spectrometer instrument detected dust particles finer than human hair, and discovered the presence of
silicates,
carbonates,
smectite, metal sulfides (like fool's gold),
amorphous carbon and
polycyclic aromatic hydrocarbons.
Tempel 1 will be visited again in 2011 by the
Stardust spacecraft as part of its extended mission. This will be the first time that a comet is visited twice and would be an opportunity to better observe the crater that was created by Deep Impact.
Further Information
Get more info on 'Comet Tempel 1'.
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