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Comet Hale-Bopp - Still Enormous!

New Images from the New Technology Telescope at La Silla

29 czerwca 1999

One of the most famous comets is Hale-Bopp that passed near the Earth just over two years ago. It now moves out through the solar system, getting fainter with increasing distance. The estimated magnitude is now about 12.5 (visual), i.e. about 400 times fainter than what can be perceived with the unaided eye.

Many observations of this object have been made with ESO telescopes during the past years. In August 1998, Methanol and Hydrogen Cyanide were detected in Hale-Bopp at record distance, cf. eso9810. The emissions from these molecules are now too faint to be measured, but other observations continue.

The most recent image of Comet Hale-Bopp was obtained at ESO on June 18, 1999, with the EMMI instrument at the ESO 3.5-m New Technology Telescope (NTT) at La Silla. This observation was somewhat difficult, as the comet was very low in the sky at the beginning of the twilight.

At that time, Comet Hale-Bopp was located in the southern constellation Dorado (The Goldfish). It was about 1295 million km (8.66 AU) distant from both the Earth and the Sun, i.e. at about as far away as planet Saturn.

The new NTT exposures have been combined to a (false) colour picture. It shows that there was still a substantial cloud of dust - a "coma" - around the comet's icy nucleus, even at this very large distance.

The second photodemonstrates the unusually large size of this coma. At the distance of the comet, the part that is visible in this photo is no less than 1.1 million km across, or nearly 10 times larger than Saturn! No other comets have ever been found to have such a large coma at this large distance [1].

There is now little structure in the coma and no "jets" are seen any more. Much of this coma consists of dust that was ejected from the nucleus when it was closer to the Sun. However, it is likely that dust is still lost from the nucleus into the coma, perhaps as a result of a continuing outflow of certain gases (in particular CO and CO 2 ), albeit at a lower level than before.

The maximum extent of the coma observed around Hale-Bopp when it was near the Earth and the Sun in early 1997, was 2-3 million km, or only a few times more than now; the uncertainty arises from the different observational methods used. Comae of other comets rarely ever become larger than a few hundred thousand kilometres. There is little doubt that the exceptional dimensions of the coma around Hale-Bopp is a direct consequence of its unusually large nucleus. Although it never became possible to measure its size accurately, a variety of observational methods points towards a diameter in the 40 - 70 km range. The nuclei of most other comets are at most a few km across. With its larger surface, more material is released - this provides a natural explanation of the unusual coma of Hale-Bopp .

Some years from now, this nucleus will be completely frozen. Then no more material will escape from the surface and the cloud will gradually disappear. It should then become possible, for the first time, to observe the "naked" nucleus of Hale-Bopp with large telescopes like the NTT and the Very Large Telescope (VLT) at Paranal.

More information is available at the dedicated ESO Hale-Bopp website.

Uwagi

[1] It appears that the largest coma seen before at another distant comet was that observed around Comet Halley after its perihelion passage. From very long exposures obtained at La Silla in April-May 1988, the diameter of its coma was found to be almost 500,000 km at a distance of about 1,300 million km (8.5 AU) from the Sun.

Addition on 5 July 1999: Kindly note that these observations were made with the EMMI multi-mode instrument at the NTT, not with SUSI2 as indicated in the original text of this release.

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