Storms on Saturn in 1994
Two new storms were observed on Saturn in 1994.
There is an article in the December 1994 issue of Sky & Telescope
about these storms, one of which is near the south pole and
the other is in the equatorial zone. Here are some central
meridian transit times for the equatorial storm.
From: James Lancashire
British Astronomical Association
Cambridge University Astronomical Society
jalan@mail.ast.cam.ac.uk
---------- 1994 October ----------- ---------- 1994 November ----------
Day UT Day UT Day UT Day UT Day UT Day UT
22 22:08 25 22:42 28 23:16 31 23:50 4 0:24 7 0:58
23 8:30 26 9:04 29 9:38 1 10:12 4 10:46 7 11:20
23 18:52 26 19:26 29 20:00 1 20:34 4 21:08 7 21:42
24 5:14 27 5:48 30 6:22 2 6:56 5 7:30 8 8:04
24 15:36 27 16:10 30 16:44 2 17:18 5 17:52 8 18:26
25 1:58 28 2:32 31 3:06 3 3:40 6 4:14 9 4:48
25 12:20 28 12:54 31 13:28 3 14:02 6 14:36 9 15:10
White spot in Saturn's equatorial zone
--------------------------------------
In response to IAU Circular No 6092, I report my observations at the
Observatories, Cambridge, UK, of a transit of a white spot in Saturn's
equatorial zone.
1994 October 13 300mm OG 25mm eyepiece (x216) seeing I/II (Antoniadi)
---------------
Transit (UT)
preceding edge 2013 +- 4
centre 2026 +- 5
following edge 2038 +- 4
1994 October 22 300mm OG 25mm eyepiece (x216) seeing I/II (Antoniadi)
---------------
Transit (UT)
preceding edge 2158 -5 (est)
centre 2208 +- 3
following edge 2222 +- 4
1994 October 23 200mm OG 18mm eyepiece (x156) seeing I/II (Antoniadi)
---------------
Transit (UT)
centre 1855 +- 3
following edge 1912 +- 3
1994 October 25 300mm OG 25mm eyepiece (x216) seeing II/III (Antoniadi)
--------------- but transparency poor
Transit (UT)
centre 2240 +- 4
following edge 2253 +- 3
The transit (of the centre) is as expected from a rotation of 10h22m for
the spot (as opposed to 10h14m of Saturn's equatorial zone (System I))
and is consistent with transits reported on IAUC 6092 and my own of
October 13 & 22. The spot appeared slightly brighter than the brightest
part of the rings, with the rest of the equatorial zone slightly shaded
and the equatorial belts darker than usual. The spot therefore seems to
be a long-lived phenomenon with no significant change over the past tens
of rotations.