Fragmented comet 73P/Schwassmann-Wachmann 3: A rare close approach

Physics

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

Scientific paper

We propose to observe 3 fragments of the split Jupiter-family comet 73P/Schwassmann-Wachmann 3 (SW3) during their close approach to Earth in May 2006. The comet broke up in 1995, which suggests that much of the outgassing we see now is from relatively pristine nuclear material. This apparition is unique: We have never before been able to study fresh material from a Jupiter-family comet at such close geocentric distances (< 0.1 AU). We propose narrowband visible and J,H,K near-IR imaging and visible spectroscopic observations that will take full advantage of the close approach to Earth and large change in viewing geometry. Our science goals are: (a) to compare the composition, color, and physical characteristics of the fragments to look for heterogeneity. Formation timescales and radial mixing in the protoplanetary disk could have affected cometary structure and composition. (b) to follow coma morphology of the dust and gas. This lets us derive the rotational states and active areas of the newly liberated fragments and study the photochemical behavior of short-lived coma species. (c) to understand the coupling between the solar wind and the comet's ion tail.

No associations

LandOfFree

Say what you really think

Search LandOfFree.com for scientists and scientific papers. Rate them and share your experience with other people.

Rating

Fragmented comet 73P/Schwassmann-Wachmann 3: A rare close approach does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Fragmented comet 73P/Schwassmann-Wachmann 3: A rare close approach, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Fragmented comet 73P/Schwassmann-Wachmann 3: A rare close approach will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-1722332

  Search
All data on this website is collected from public sources. Our data reflects the most accurate information available at the time of publication.