| .TH ASTRO 1 |
| .SH NAME |
| astro \- print astronomical information |
| .SH SYNOPSIS |
| .B astro |
| [ |
| .B -dlpsatokm |
| ] |
| [ |
| .B -c |
| n |
| ] |
| [ |
| .B -C |
| d |
| ] |
| [ |
| .B -e |
| .I obj1 |
| .I obj2 |
| ] |
| .SH DESCRIPTION |
| .I Astro |
| reports upcoming celestial events, by default for 24 hours starting now. |
| The options are: |
| .TP |
| .B d |
| Read the starting date. |
| A prompt gives the input |
| format. |
| .TP |
| .B l |
| Read the north latitude, west longitude, and elevation of the observation point. |
| A prompt gives the input format. |
| If |
| .B l |
| is missing, the initial position is read from the file |
| .BR \*9/sky/here . |
| .TP |
| .B c |
| Report for |
| .I n |
| (default 1) successive days. |
| .TP |
| .B C |
| Used with |
| .BR -c , |
| set the interval to |
| .B d |
| days (or fractions of days). |
| .TP |
| .B e |
| Report distance between the centers of |
| objects, in arc seconds, during eclipses or occultations involving |
| .I obj1 |
| and |
| .IR obj2 . |
| .TP |
| .B p |
| Print the positions of objects at the |
| given time rather than searching for interesting |
| conjunctions. |
| For each, the name is followed by |
| the right ascension (hours, minutes, seconds), |
| declination (degrees, minutes, seconds), |
| azimuth (degrees), |
| elevation (degrees), |
| and semidiameter (arc seconds). |
| For the sun and moon, the magnitude is also printed. |
| The first line of output presents the date and time, |
| sidereal time, and the latitude, longitude, and elevation. |
| .TP |
| .B s |
| Print output in English words suitable for speech synthesizers. |
| .TP |
| .B a |
| Include a list of artificial earth satellites for interesting events. |
| (There are no orbital elements for the satellites, so this option |
| is not usable.) |
| .TP |
| .B t |
| Read |
| ΔT |
| from standard input. |
| ΔT |
| is the difference between ephemeris and |
| universal time (seconds) due to the slowing of the earth's rotation. |
| ΔT |
| is normally calculated from an empirical formula. |
| This option is needed only for very accurate timing of |
| occultations, eclipses, etc. |
| .TP |
| .B o |
| Search for stellar occultations. |
| .TP |
| .B k |
| Print times in local time (`kitchen clock') |
| as described in the |
| .B timezone |
| environment variable. |
| .TP |
| .B m |
| Includes a single comet in the list of objects. |
| This is modified (in the source) to refer to an approaching comet |
| but in steady state |
| usually refers to the last interesting comet (currently Hale-Bopp, C/1995 O1). |
| .SH FILES |
| .TP |
| .B \*9/sky/estartab |
| ecliptic star data |
| .TP |
| .B \*9/sky/here |
| default latitude (N), longitude (W), and elevation (meters) |
| .SH SOURCE |
| .B \*9/src/cmd/astro |
| .SH SEE ALSO |
| .IR scat (1) |
| .SH BUGS |
| The |
| .B k |
| option reverts to GMT outside of 1970-2036. |