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2005/01/30 | 地方恒量时[Local Sidereal Time]
类别(¤〖天文〗)
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发表于 20:07
Local sidereal time is the most useful form of
sidereal time
since it gives the
right ascension
of a transiting celestial object at a given location. To compute the current local sidereal time
LST
, consult the current Astronomical Almanac. Look up the "G. Sidereal Time (Apparent)"
GST
at
midnight
(0 h) in the third column corresponding to the current date
universal time
. Let
T
be the current local 24-hour time, and add
hours to convert from local time to
Greenwich mean time
.For U.S. Eastern time zone, this will be
4
hours for EDT and 5 hours for EST. Multiply
by 1.0027379093 (the number of
sidereal days
in a
solar day
).Add the equation of equinoxes if desired (this is only a tenth of a second or so correction). Then subtract the west longitude (or add the east longitude) L of your location converted to hours (hours = degrees/360*24). Now add or subtract 24 hours as needed. Symbolically,
Since we used the "apparent sidereal time," the above number is actually the "local apparent sidereal time," sometimes written
LAST
.
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