Description Usage Arguments Value Author(s) Examples
These functions are used for converting between astronomical and sidereal times.
1 2 3 4 |
x |
an object of class gmt (Greenwich Mean Time), gst (Greenwich Sidereal Time), lst (Local Sidereal Time) or lt (Local Time) |
jday |
Julian Day Number (default for today) |
lambda |
Longitude of observer (default taken from options) |
... |
Additional arguments |
A converted object of appropriate class.
Lukasz Komsta
1 2 3 4 5 |
time
1 9h 33m 37s
2 10h 33m 37s
3 11h 33m 37s
4 12h 33m 37s
5 13h 33m 37s
6 14h 33m 37s
7 15h 33m 37s
8 16h 33m 37s
9 17h 33m 37s
10 18h 33m 37s
time
1 9h 33m 37s
2 10h 33m 37s
3 11h 33m 37s
4 12h 33m 37s
5 13h 33m 37s
6 14h 33m 37s
7 15h 33m 37s
8 16h 33m 37s
9 17h 33m 37s
10 18h 33m 37s
time
1 9h 33m 37s
2 10h 33m 37s
3 11h 33m 37s
4 12h 33m 37s
5 13h 33m 37s
6 14h 33m 37s
7 15h 33m 37s
8 16h 33m 37s
9 17h 33m 37s
10 18h 33m 37s
time
1 7h 26m 24s
2 8h 26m 34s
3 9h 26m 44s
4 10h 26m 54s
5 11h 27m 4s
6 12h 27m 14s
7 13h 27m 23s
8 14h 27m 33s
9 15h 27m 43s
10 16h 27m 53s
Add the following code to your website.
For more information on customizing the embed code, read Embedding Snippets.