James Miller G3RUH
19xx January is that time of year for the annual pleas, by users of
ancient software, that they've run out of "sidereal time data".
This quantity is not some arcane kludge divined by sorcerers from the
entrails of slide rules, but a simple quantity that describes the
Terrestrial longitude of the Celestial 0 deg longitude at 0000 utc.
Some satellite tracking software needs this for 19xx Jan 0.0. Look at the
following table:
YEAR GHAA(0) deg GMST rev
----------------------------------------
1989 99.636681 0.276769 This means that at the
1990 99.397970 0.276105 beginning of 1989, the
1991 99.159257 0.275442 Celestial 0 deg of longitude
1992 98.920546 0.274779 will be over 99.6 deg Earth
longitude (Mexico City).
1993 99.667481 0.276854 As the Earth rotates it
1994 99.428769 0.276191 moves West at a rate of
1995 99.190057 0.275528 approx. 15 deg/hour.
1996 98.951346 0.274865
1997 99.698282 0.276940
1998 99.459570 0.276277
1999 99.220859 0.275613
2000 98.982147 0.274950
-------------------------------------
There are some obvious rhythms in it. The angular measure (Greenwich Hour
Angle Aries Jan 0.0). is roughly 99 degrees. It decreases by 0.238711
degrees for three years, and then increases by 0.746936 after the fourth,
which you will notice is a leap year. So, you can always get next year's
value from last year's.
Where do -0.238711 and +0.746936 come from? Easy! The Earth rotates
360. 985647367 degrees per day; 360 degrees on its own axis, plus the
little bit (0.9856 deg) because it revolves around the Sun too. So in a
leap year of 366 days it turns through 366 * 360.985647367 = 132120.746936
degrees, which is just 367 revolutions + 0.746936 deg. In a 365 day year
it's 366 rev - 0.238711 deg.
OK, so now you want a formula for all this. Mechanising the rhythm just
described gives:
GHAA(0) = 99.6367 - 0.2387*(YR-1989) + 0.9856*INT((YR-1989)/4) degrees
where GHAA(0) is the Greenwich hour angle for year YR Jan 00, 0000utc, and
YR = is four digits, e.g. 1991, 1992 etc.
Divide this value by 360 if you want it in revolutions.
This is perfectly adequate for satellite work. But perfectionists will
want to account for the fact that the year gets longer as the Earth slows
down. By Astronomical convention, the adopted formula is (Ref 1):
GMST = 24110.54841 + TU*(8640184.812866 + TU*(0.093104 + TU*(-6.2E-6)))
seconds
For degrees, divide by 240, for revolutions divide by 86400.
Tu is the interval of time, (measured in Julian centuries of 36525
days of universal time), elapsed since the epoch 2000 Jan 1.5
i.e TU = (JD - 2451545.0)/36525
GMST is Greenwich Mean Sidereal Time. (Astronomers are historically stuck
with using units of time for longitude. The rest of us are stuck with
degrees. 24 hrs = 360 deg).
Now, this is pretty tedious to evaluate, so I've given a short program to
calculate it instead.
I want to make it clear that modern tracking software doesn't need any of
this mumbo-jumbo. It will have the celestial longitude initialised as 99.6
degrees on 1989 Jan 0.0 and can calculate any future value quite simply
from this.
The writers of software that ask you to put in a value for each
year from the table must have regretted ever since. PLEASE give them a
break - work it out for yourself!
Ref 1: Aoki S., Guinot B., Null G.H., Kinoshita H., McCarthy D.D.,
Seidelmann P.K.; Astron. Astrophysics, 105, 359. 1982
10 T$="B.GHAA(0)": REM GMST of 0000 utc Calculator. Based on
20 REM 1984 Astronomical Almanac Pages B6 & S13.
30 REM
40 REM Version 1.1 Last modified 1985 May 08 by JRM
50 REM
60 REM (C)1991 J R Miller G3RUH
70 REM
80 REM GMST =24110.54841 + TU*(8640184.812866+TU*(0.093104+TU*(-6.2E-6)))
90 REM (seconds).
100 REM
110 REM where Tu is the interval of time, (measured in Julian centuries
120 REM of 36525 days of universal time), elapsed since the epoch
130 REM 2000 Jan 1.5 i.e TU = (JD - 2451545.0)/36525
140 REM
150 FI%=&80F: FF%=&2060F: REM Print formats; ######### #.######
160 :
170 PRINT"Program ";T$;" GHAA for Year yyyy Jan 0.0 (C)1991 G3RUH"
180 PRINT
190 PRINT" YEAR GHAA deg GMST rev"
200 PRINT" -------------------------------------"
210 FOR YR = 1989 TO 2000
220 DD = FND0(YR)-(FND0(2000)+1.5): REM Days since 2000 Jan 1.5
230 TU = DD/36525
240 G1 = TU*(184.812866+TU*(0.093104+TU*(-6.2E-6)))/86400 :REM Small part
250 G2 = TU*100 :REM Big part
260 G3 = 0.2790572733 :REM 24110.54841/86400
270 GMST = G1+G2+G3: GMST = GMST-INT(GMST): GHAA = GMST*360
280 @%=FI%: PRINT YR;: @%=FF%: PRINT GHAA,GMST
290 NEXT
300 STOP
310 DEF FND0(YR) =INT((YR-1)*365.25)
Feedback on these pages to Webmaster. Feedback on the article should be sent to James Miller
Created: 1994 Nov 17 -- Last modified: 2005 Oct 29
