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        "description": "===============\nWhatsObservable\n===============\n\nWhatsObservable is used for determining which minor planets (and comets) \nare observable at a given time from a given location on Earth.  \n\nWhatsObservable determines the locations of objects using the routines\nof [PyEphem](http://rhodesmill.org/pyephem/) and the\n[Minor Planet Center's Orbit Database](http://www.minorplanetcenter.net/iau/MPCORB/MPCORB.DAT).\n*Note that at least for the time being the user must download this file \nseparately and WhatsObservable will find it on disk.*\n\nThe intent is to replicate the functionality available at the [JPL Solar System\nDynamics Small Body Whats Observable web page](http://ssd.jpl.nasa.gov/sbwobs.cgi).\nThe motivation for writing WhatsObservable was to provide this capability when\noffline and in an easily scriptable manner.  \n\nNOTE: The precision of PyEphem with the MPC Orbit Database is good, especially for\ndates near the orbital epoch, but is not nearly as good as what is available \ndirectly from the [JPL Horizons System](http://ssd.jpl.nasa.gov/?horizons).  Even\nnear the orbital epoch errors of a few arcseconds are not uncommon.  Use this\ntool at your own risk and if precision matters, refer back directly to the\n[JPL Horizons System](http://ssd.jpl.nasa.gov/?horizons).\n\nA typical usage is:\n\n    import datetime\n    from whatsobservable import minorplanets\n\n    objects = minorplanets(datetime.datetime(2013, 9, 1, 10, 0), \n                           568,   # 568 is the observatory code for Mauna Kea\n                           max_objects=5, max_magnitude=12., max_zenithdistance_deg=60.0)\n    print objects\n\nNote that the return is a pandas.DataFrame\n\n===============\n\nOriginally written 2013-09-07 by Henry Roe (hroe@hroe.me)",
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