Hale-Bopp is a long-period comet that was discovered in 1995 and that
reached perihelion in Spring, 1997. Because it was much brighter than
comets normally are when it was first discovered outside the orbit of
Jupiter, there was considerable speculation that in the Spring of 1997
Hale-Bopp would be a spectacular sight.
But Comet Brightness is Notoriously Unpredictable
On the other hand, comets that are predicted to be very bright when discovered often do not live up to their advanced billing (here is an associated funny story concerning the comet Kohoutek; a comet that never grew as bright as predicted in 1974). Hale-Bopp did turn out to be a spectacular sight, certainly one of the better comets of recent years.The Orbit of Hale-Bopp
The orbit of Hale-Bopp and its position with respect to the planets of the inner solar system on Dec. 16, 1996, is shown in the following figure.
Comet Hale-Bopp, December
16, 1996
In this image the orbits are drawn to scale, but the sizes of the planet and comet images (and the length and orientation of the comet tail) are not realistic.
At this time the comet was about 2 A.U. from the Sun and about 2.7 A.U. from the Earth. The color blue indicates portions of orbits that are above the plane of the ecliptic and green indicates portions of orbits that are below the plane of the ecliptic. Notice that Hale-Bopp has an orbit that is either parabolic or highly elliptical, and that its orbit is very far out of the plane of the ecliptic.
 The Inner Solar System on April 1, 1997, with Comet Hale-Bopp at perihelion. |
Comet Hale-Bopp
reached perihelion on April 1, 1997, at a distance of 0.91 A.U.
from the Sun and 1.36 A.U. from the Earth.
The image on the left shows the relative positions of objects in the inner solar system on that date. |
Telescopic Observations of Hale-Bopp
The following figure shows the temporal evolution of Comet Hale-Bopp from late 1995 through late 1996, as observed by the Hubble Space Telescope.
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| Hubble Space Telescope Images of Comet Hale-Bopp (1995) |
The left frame shows the comet about 60 hours after a huge outburst of dust; it shows a spiral structure reminescent of a water sprinkler observed from above. The middle frame shows the comet during a more quiescent phase. The right figure shows a more recent image with at least five jets emanating from the nucleus. (Here is an enhanced photograph of at least 7 jets from Hale-Bopp taken at the European Southern Observatory.)
The nucleus of the comet is located at the center of each frame, but most of the light observed is caused by scattered sunlight from the coma of dust emitted from the nucleus.
Information supplied by: http://csep10.phys.utk.edu