Sidereal time on any date
- Builds on
- Sections 1.3, 2.1, 2.3 and 2.4
- Reading time
- 35 min
- Exercises
- 4
- Olympiad problems
- 2
At 22:00 on 15 January in Ankara, Aldebaran crossed the meridian a quarter of an hour earlier, high in the south, and Sirius will cross it at 23:54. Both facts follow from one number, the local sidereal time, which at that moment was 4h 52m. In Section 1.3 we met sidereal time as the right ascension of whatever is on the meridian, and a star's hour angle as the sidereal time minus its right ascension. In this section we find the sidereal time for any place, date and time, which is the first step of almost every problem that links the sky to a clock.
2.5.1Sidereal time from the Sun
At 12:00 apparent solar time on the day of the March equinox, what is the local sidereal time?
The Sun has a right ascension and an hour angle like any star, so (1.10) applies to it. Its hour angle is the apparent solar time minus 12 hours, by (2.3). Putting the two together gives the sidereal time from the Sun.
| local sidereal time | |
| apparent solar time | |
| right ascension of the Sun |
For a quick estimate, the sidereal time is about 0h at 12:00 on 21 March and runs 3 min 56.6 s ahead of solar time each day. The estimate can be out by several minutes, because the equation of time and the uneven motion of the Sun in right ascension are ignored, but it is often enough to tell which part of the sky is up.
| Local sidereal time | |
|---|---|
| Bright star nearest the meridian | |
| Hour angle of the Sun |
Estimate the local sidereal time at 21:00 local mean time on 21 May.
At 12:00 on 21 March the sidereal time is about 0h. Sixty-one days later, at the same time, it is later by
Nine hours of solar time are
2.5.2Sidereal time from the date
For accurate work we start from the sidereal time at Greenwich, the Greenwich mean sidereal time, written GMST, and add the longitude. Problems usually give GMST at 0h UT on some reference date, such as 1 January of the year. From there it grows by 3 min 56.56 s for each whole day, by (2.2), and on the day itself by 1.002738 hours for each hour of universal time.
| Greenwich mean sidereal time at 0h UT on the reference date | |
| number of whole days from the reference date to the day in question | |
| 1.002738, the number of sidereal hours in an hour of universal time | |
| longitude, positive east |
Without a reference date, the Julian date of Section 2.4 gives GMST directly. Between noon UT on 1 January 2000 and any moment there are
| days since J2000.0, |
Find the local sidereal time in Hanoi (105.85° E, UT+7) at 21:00 on 28 September 2026.
From Example 2.8, 0h UT on 28 September 2026 is
and taking away
At 22:00 on 15 January the local sidereal time in Ankara is 4h 52m. Sirius has right ascension 6h 46m. How many hours east of the meridian is Sirius?
- Sidereal time runs faster than solar time. An interval of universal time must be multiplied by 1.002738 before it is added to a sidereal time, which adds about 10 seconds for every hour.
- GMST is the sidereal time at Greenwich. The local sidereal time needs the longitude added, east positive, at one hour for every 15°.
- Days are counted from 0h UT on the reference date to 0h UT on the day in question. In a leap year February has 29 days, and forgetting it puts the answer 3 min 56 s out.
- A sidereal time larger than 24h, or negative, is fine in the middle of a calculation, but the answer should be brought back between 0h and 24h.
- 2.5.1
Use (2.12) to find GMST at 0h UT on 1 January 2026, which is JD 2 461 041.5.
hoursHere
andwhich after taking away whole multiples of 24 h is 6.71 h, or 6h 42.6m.
- 2.5.2
At 0h UT on 1 January 2017 the Greenwich mean sidereal time was 6h 43m. What was it at 0h UT on 1 March 2017?
hours2017 was not a leap year, so 1 March is 59 days after 1 January. By (2.11),
which is 10.59 h.
- 2.5.3
Roughly what is the local sidereal time at midnight, apparent solar time, at the September equinox?
The answer is (a). At the September equinox the Sun's right ascension is 12h, and at midnight the apparent solar time is 24h, so by (2.10) the sidereal time is , which is 0h. - 2.5.4
Find the local sidereal time in Ankara (32.86° E, UT+3) at 22:00 on 15 January 2026, given that GMST at 0h UT on 1 January 2026 was 6h 42.6m.
hoursAt 22:00 in Ankara the universal time is 19:00. From 1 to 15 January is 14 days, so GMST at 0h UT on 15 January is . In 19 hours it grows by , giving GMST = 26h 40.9m, which is 2h 40.9m. Adding the longitude, h = 2h 11.4m, gives LST = 4h 52.3m, which is 4.87 h.
2018Sidereal time zero twice in a day10 points
Adapted from IOAA 2018 (Beijing), theory problem 5. We have restated it in our own words and kept the original data. The solution was last checked on 17 October 2026.
On one particular day of each year, the Greenwich mean sidereal time is 00:00:00 twice. (a) Roughly what is the right ascension of the Sun on that day? (b) Estimate the date of this day in 2018, given that GMST was 6.706 h at 0h UT on 1 January 2018 (JD 2 458 119.5).
- (a) Sidereal time 0h comes round once every sidereal day, which is shorter than a solar day, so it can fall twice on one date only if the first time is within 3 min 56 s after midnight. GMST is then about 0h at midnight UT, when the meridian of Greenwich points away from the Sun. So the meridian at midnight has right ascension 0h, the Sun is opposite it, at right ascension 12h, and the date is near the September equinox.
- (b) GMST at 0h UT grows by
h a day. It reaches 24 h after days. - After 263 days, at 0h UT on 21 September 2018, GMST is
h, or 23h 59m 16s. It reaches 0h 44 s later, at 00:00:44 UT, and again one sidereal day later, at 23:56:48 UT, both on 21 September.
Answer(a) The Sun is near the September equinox, at a right ascension of about 12h. (b) It happens on 21 September 2018. The official solution states 18h in part (a), which does not fit its own reasoning about the September equinox, where the Sun's right ascension is 12h.
2020The sky above Chiayi6 points
Adapted from the 2020 Global e-Competition on Astronomy and Astrophysics (Estonia, online), held in place of the IOAA that year, theory problem 7, part (a). We have restated it in our own words and kept the original data. The solution was last checked on 17 October 2026.
An observer in Chiayi, Chinese Taipei (23.5° N, 120.4° E, UT+8) watched meteors at 21:00 local time on 25 September 2020. Find the local sidereal time of the observation. The Greenwich sidereal time at 0h UT on 1 January 2020 was 6h 40m 30s.
-
21:00 at UT+8 is 13:00 UT. From 1 January to 25 September 2020 is
days. -
By (2.11), in 268 days GMST grows by
. Here the daily gain, , has one more figure than in the result, because over 268 days that figure is worth a second. In 13 hours of universal time GMST grows by . So GMST iswhich is 13h 19m 15s.
-
The longitude 120.4° E is 8h 01m 36s, so LST = 21h 20m 51s.
AnswerThe local sidereal time was 21h 20m 51s. The official solution rounds the 268 days of growth down to 17h 36m 36s and gets 21h 20m 50s.