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Summary of Lunar Occultations for 2000

More about occultations.

Introduction

During 2000, there are approximately 540 lunar occultations potentially observable from East Anglia, although many involve faint stars. There are two grazing occultations of stars visible from East Anglia. The Moon does not occult any planets during the year as seen from the region.

This article summarises the circumstances of the best occultations during the year. It provides details for the location of Orwell Park Observatory; differences will in general be negligible for locations throughout East Anglia.

Occultations of Bright Stars

Table 1 lists occultation events during the year, of stars brighter than magnitude 5.0, where the circumstances are favourable. These events should be readily visible in small telescopes or binoculars.

The first two columns of the table list the date and time (UT) of the occultation. Column three specifies the phenomenon: "D" denotes a disappearance and "R" a reappearance. The table lists circumstances of D and/or R as dictated by the visibility of each phenomenon (determined by altitude, lunar phase, etc). Column four details the lunar phase (positive waxing and negative waning). Columns five and six give the altitude of the Sun and the star, both in degrees. (A negative solar altitude means that the Sun is below the horizon.) Columns seven and eight provide the star's magnitude and catalogue number.
 

Date
2000
Time
(UT)
D
R
Lunar
Phase
Sun
Alt (°)
Star
Alt (°)
Mag Star
11 Jan18:08:00
18:45:54
D
R
0.22+-18
-24
22
18
4.2ψ1 Aqr
11 Jan18:49:45
19:53:39
D
R
0.22+-24
-34
18
10
4.4ψ2 Aqr
15 Jan21:52:48
22:41:44
D
R
0.64+-50
-55
36
29
4.3μ Cet
11 Feb20:10:06
21:11:28
D
R
0.37+-29
-38
32
23
4.3ξ2 Cet
16 Feb00:20:48D0.82+-51374.1ν Gem
12 Mar22:16:07
23:15:10
D
R
0.45+-36
-40
27
18
4.9104 Tau
13 Mar20:28:09
21:35:39
D
R
0.56+-23
-32
51
42
4.6χ2 Ori
14 Mar19:49:31
21:02:42
D0.67+-18
-28
58
54
4.0ζ Gem
09 Apr22:43:06
23:24:25
D
R
0.31+-28
-30
15
9
4.4χ1 Ori
21 Aug02:29:24
03:37:11
D
R
0.68--18
-11
41
45
4.3ξ2 Cet
13 Nov02:05:40
02:58:21
D
R
0.98--46
-38
52
47
3.8δ1 Tau
01 Dec16:40:27
17:40:09
D
R
0.27+-8
-16
18
16
4.8η Cap
08 Dec17:20:55D0.91+-14254.3μ Cet

Table 1. Occultations of stars brighter than magnitude 5.0.
 

Occultation Seasons

The Moon’s orbit is defined by a range of periodicities, both short and long term. The short term periodicities mean that the Moon’s path through the sky follows a pattern whereby it almost repeats itself every month. The longer term periodicities gradually shift the orbit so that no particular pattern of approximate repetition can last more than a few years. This results in so called "occultation seasons", lasting for months or years, during which particular stars are repeatedly occulted, or repeatedly not occulted. The effect is most pronounced for the four first magnitude stars that the Moon can occult, namely Aldebaran, Spica, Antares and Regulus. We have recently left an occultation season of Aldebaran and are currently in an occultation season lasting until 2007 when none of these stars are occulted.

Nights With Many Occultation Events

During the year, the Moon traverses some rich star fields. When this happens, a large number of occultations can occur during a single evening. Table 2 lists all evenings throughout the year when the Moon occults more than 10 stars; many are associated with the Moon’s passage through rich star fields in Taurus.
 

Date, No occs Date, No occs Date, No occs Date, No occs
11 Jan, 12 12 Jan, 12 13 Jan, 15 10 Feb, 11
11 Feb, 23 12 Feb, 15 09 Mar, 11 10 Mar, 14
11 Mar, 23 12 Mar, 16 13 Mar, 11 08 Apr, 15
09 Apr, 58 10 Apr, 54 12 Apr, 14 06 May, 13
07 May, 37 08 May, 34 09 May, 36 05 Jun, 18
08 Jun, 11 04 Oct, 19 02 Nov, 13 03 Nov, 23
29 Nov, 11 01 Dec, 16 03 Dec, 17 31 Dec, 13

Table 2. Nights with more than 10 occultations.
 

Grazing Occultations

The track of two grazing occultations cross East Anglia during the year. Table 3 summarises the circumstances. Columns one and two give the date and time of the graze and column three specifies the lunar limb involved. Column four indicates the distance between Orwell Park Observatory and point X on the track, on land, where the distance between the two is least; column five links to a plot of the lunar limb profile visible from X. Column six specifies a north or south displacement of the observer's position, relative to the track, based upon inspection of the limb profile, to maximise the chances of witnessing multiple disappearance and reappearance events. Column seven links to an on-line Google Earth plot of the track and column eight links to an off-line image of it. (The plot and image illustrate the nominal track, with no displacement applied.) Column nine details the lunar phase (positive for waxing, negative for waning) and column 10 the altitude of the Sun (a negative solar altitude means that the Sun is below the horizon). Columns 11 and 12 provide the horizontal co-ordinates of the star (azimuth in the order N→E→S→W). Columns 13 and 14 specify the star and its magnitude.
 

Date
2000
Time
(UT)
Limb Dist
OPO
(km)
Limb
Profile
Track
Shift
(km)
Google
Earth
Track
Google
Earth
Image
Lunar
Phase
Sun
Alt
(°)
Star
Alt
(°)
Star
Azi
(°)
Mag Star
30 Jan 04:03 N 40 Profile 0.6 S Track Track 0.33- -33 10 133 6.5 ZC 2280
08 May 21:34 S 24 Profile 0.5 N Track Track 0.29+ -15 23 273 5.1 ZC 1150

Table 3. Grazing lunar occultations.
 


James Appleton