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Summary of Lunar Occultations for 2004

More about occultations.

Introduction

During 2004, potentially observable from East Anglia are approximately 600 lunar occultations, although many involve faint stars, and one grazing occultation. No planetary occultations are visible from the region during the year.

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 down to magnitude 5.5, 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
2004
Time
(UT)
D
R
Lunar
Phase
Sun
Alt (°)
Star
Alt (°)
Mag Star
05 Jan20:35:51D0.97+-41555.2125 Tau
14 Jan02:18:59
03:02:11
D
R
0.61--50
-44
26
31
2.7γ Vir, Porrima
31 Jan18:48:05D0.73+-20595.572 Tau
24 Feb18:00:27
18:52:55
D
R
0.19+-6
-14
37
30
4.3ο Psc
02 Mar19:32:56D0.82+-19595.376 Gem, c Gem
23 May21:13:02R0.18+-9235.376 Gem, c Gem
02 Jun22:31:55D1.00+-14114.822 Sco, i Sco
10 Jul02:47:34D0.42--7284.3ο Psc
13 Jul01:34:17
02:28:21
D
R
0.16--13
-9
8
16
4.437 Tau, A1 Tau
05 Oct03:21:58
04:12:20
D
R
0.62--25
-18
60
64
4.6136 Tau
20 Oct19:06:19
19:54:42
D
R
0.48+-22
-29
9
7
4.559 Sgr, b Sgr
20 Nov16:43:57R0.66+-7205.095 Aqr, ψ3 Aqr
23 Nov02:42:04D0.86+-4365.580 Psc, e Psc
18 Dec19:29:57
20:27:10
D
R
0.51+-33
-42
31
27
4.927 Psc
18 Dec21:32:04D0.52+-51205.129 Psc

Table 1. Occultations of stars of magnitude 5.5 or brighter.


In table 1, note in particular the occultation of Porrima on 14 January 2004: the star is a famous double with two identical yellowish components, both of magnitude 3.6, which a large telescope will show as separate prior to the occultation.

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 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 10 or more stars.
 

Date, No occs Date, No occs Date, No occs Date, No occs
26 Jan, 15 24 Feb, 12 25 Feb, 14 24 Mar, 15
25 Mar, 22 27 Mar, 19 28 Mar, 14 24 Apr, 45
25 Apr, 12 26 Apr, 20 22 May, 15 23 May, 12
24 May, 16 18 Nov, 10 15 Dec, 19 16 Dec, 10

Table 2. Nights with 10 or more occultations.
 

Grazing Occultation

The track of one grazing occultation crosses 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
2004
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
25 Jan 18:56 S 21 Profile 0 Track Track 0.18+ -22 17 147 6.1 ZC 3506

Table 3. Grazing lunar occultation.
 


James Appleton