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FUSE
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Mission Status Report
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Mission Status Report #51 Star Date: November 1, 2001
FUSE Science Moves to the Forefront!
Caption: The space between stars is not entirely empty! In many regions, clouds of gas and dust
lurk nearly undetected. Where such clouds of gas and dust are located near hot, young stars, such
as in this picture of NGC 6559, the gas glows or the dust can be seen as dark lanes against
a brighter background. FUSE can detect such material even if it is invisible in such a picture
by looking for absorption from this material in the far-ultraviolet light spectrum.
Such indirect studies of hot and cold material in the Interstellar Medium" is a major part
of what the FUSE satellite does. (Photo courtesy of Robert Gendler. See
Astronomy Picture of the Day for
October 23, 2001.)
(Click image above to see larger version.)
Hello World,
All continues to go extremely well on the FUSE project. All systems are nominal, including the
spacecraft, science instrument, and ground systems performance. As FUSE continues operations
during the primary scientific mission, over three-quarters of a million seconds of on-target
observing time is being obtained each month. These data are processed at Johns Hopkins and
then archived at the Multi-Mission Archive at
Space Telescope (MAST), where the data can be
downloaded by astronomers from all over the world.
The wheels of science sometimes grind slowly. The data sets produced by FUSE are themselves
quite complex to work with, and interpretting what these data mean can also be challenging.
We are please by the results coming out so far (see
this reference list of
2001 Publications to date), and there are many more on the way, but these are literally
the tip of the iceberg! There is so much more to come!
During the week of October 22, 2001, the FUSE Science Team met in Baltimore. (This is the
so-called "Principal Investigator" science team--the group of scientists who proposed the
FUSE mission to NASA. Averaged over the three years of the primary science mission, this
team of scientists receives about 43% of the observing time, much of which has already been
performed.) Each project leader reported on the results from their project area, and the results
were truly impressive! From active galaxies to cool stars to hot stars to various programs
on understanding cold and hot gas in interstellar space, it is clear that the FUSE mission
is providing bold new insights into the universe around us. But it will take time for these
results to make their way out into the professional literature.
And this is only a fraction of the total FUSE effort! Over 50% of the time with FUSE is used
to observe targets for Guest Investigators--scientists from the astronomical community selected
by NASA to use the capabilities of FUSE for their own science projects. Since many of these
people are university and college professors and the like, they also have limited time to pursue
their research interests and get their results into publications. Many of these results are
discussed first at meetings such as hosted bi-annually by the American Astronomical Society.
To help get the word out about FUSE science results, the FUSE project is holding a FUSE
Science Workshop on the Johns Hopkins campus March 20-22, 2002. This will be an opportunity for
anyone working on FUSE-related science projects to come together, present their results, and
discuss them with other scientists who may work in a similar or completely different field.
This kind of cross-fertilization is common in astronomy and often results in new insights
either about the data themselves or the interpretation of them. We encourage all FUSE
scientists to consider attending this important meeting. (Watch the FUSE home page for details!)
Elsewhere on the project, plans are well underway for "Cycle 3", or the third year of science
operations, which begins officially on Dec. 1, 2001. NASA has recently announced the results
of the latest round of proposal requests, and revised inputs to support those observations are
being processed into the planning system. As long as our satellite remains healthy, we will
continue to reap the benefits of this astronomical workhorse in orbit.
Reported by: Bill Blair, Chief of Observatory Operations
Peruse Previous Status Reports, or
Return to the FUSE home page.
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