Changes between Version 24 and Version 25 of WikiStart
- Timestamp:
- Feb 6, 2013, 1:03:07 PM (12 years ago)
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WikiStart
v24 v25 15 15 You may also use the science CCD. It has a field of view of 15' times 15', which corresponds to 1024 times 1024 Pixels with a pixel scale of 0.9". The CCD is cooled to -120 degree Celsius by means of liquid Nitrogen. Parts of the electronic are similar to the one used on Calar Alto, as mentioned above. With just a few minutes exposure the camera reaches objects of 17th magnitude. Thanks to a newly improved tracking it is indeed now possible to integrate for ten minutes or even longer. With this camera students have the opportunity to learn vital observational techniques: how to stear a telescope or a camera, how to plan an observing run, how to monitor the data you get while you get it ... This all makes up a very good preparation for observations with bigger telescopes. And, naturally, we also take some beautiful pictures of known and not so known objects. 16 16 17 [[Image(asteroid_mpia_citation .png, right, margin-left=30, title="Citation of asteroid MPIA", longdesc="Citation of asteroid MPIA")]]17 [[Image(asteroid_mpia_citation_ann.png, right, margin-left=30, title="Citation of asteroid MPIA", longdesc="Citation of asteroid MPIA")]] 18 18 19 19 As the telescope starts to be fully usable, there are many ideas for science projects. For example Roland Jesseit has thought of conducting a survey to find planetary transits before stars of the Milky Way. One should be able to distinguish the signature of such an event from other variable stars quite easily. Christian Wolf has thought of tracking faint asteroids to determine their orbit.