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Summary of Lunar Occultations for 2014

More about occultations.

Introduction

During 2014, there are over 700 lunar occultations potentially observable from East Anglia, although many involve faint stars. The tracks of three grazing lunar occultations cross the region during the year, one within 30 km of Orwell Park Observatory and two within 3 km! No lunar occultations of planets occur in 2014 visible from East Anglia.

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
2014
Time
(UT)
D
R
Lunar
Phase
Sun
Alt (°)
Star
Alt (°)
Mag Star
11 Feb03:58:39D0.87+-3175.226 Gem
11 Feb20:10:09
20:45:29
D
R
0.91+-29
-34
50
52
3.654 Gem, λ Gem
13 Feb20:32:19D0.99+-32385.460 Cnc
14 Feb04:22:38D0.99+-27185.276 Cnc, κ Cnc
07 Mar18:30:09R0.42+-8534.368 Tau, δ3 Tau
13 Mar21:02:48D0.92+-28455.42 Leo, ω Leo
25 Mar04:27:43D0.37--13123.944 Sgr, ρ1 Sgr
04 May20:22:05
20:43:37
D
R
0.29+-8
-11
31
28
3.654 Gem, λ Gem
03 Jun21:45:57
22:45:09
D
R
0.32+-11
-14
15
6
5.42 Leo, ω Leo
15 Jun00:14:56
01:18:10
D
R
0.95--15
-13
17
20
3.944 Sgr, ρ1 Sgr
08 Aug21:01:14
22:05:50
D
R
0.95+-12
-18
19
20
3.944 Sgr, ρ1 Sgr
21 Aug03:47:42D0.17--9245.226 Gem
18 Sep03:27:44
04:31:27
D
R
0.30--19
-10
32
41
3.654 Gem, λ Gem
20 Sep04:21:01
05:08:37
D
R
0.14--12
-5
22
29
5.460 Cnc
05 Nov17:06:42D0.98+-8114.3110 Psc, ο Psc
03 Dec02:48:31D0.87+-4484.3110 Psc, ο Psc
09 Dec06:06:59
07:02:14
D
R
0.92--15
-7
31
22
3.654 Gem, λ Gem

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

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.

In 2014, the phenomenon is evident through the repeated occultations of the stars 54 Gem, 26 Gem and 60 Cnc during the year.

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 12 stars. The large numbers of occultations on 03 May and 28 October are associated with star fields in Gemini and Ophiuchus respectively.
 

Date, No occs Date, No occs Date, No occs Date, No occs
04 Jan, 15 05 Jan, 27 05 Mar, 15 07 Mar, 14
03 Apr, 15 04 Apr, 15 05 Apr, 22 06 Apr, 14
02 May, 15 03 May, 46 (!) 04 May, 26 05 May, 13
28 Oct, 48 (!) 30 Oct, 13 25 Nov, 15 26 Nov, 16
24 Dec, 14 25 Dec, 18 26 Dec, 22 -

Table 2. Nights with more than 12 occultations.
 

Grazing Occultations

The tracks of three grazing occultations cross East Anglia during the year. (Note that two of the tracks pass very close to Orwell Park Observatory.) 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 the closest point on the track, on land. Column five links to a plot of the lunar limb profile visible either (a) from longitude 1.25° E (WGS84) on the track, if this is on land or, if it is not, (b) from the most easterly point on the track on land. 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 the track. (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
2014
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
13 Jan 00:45 S 28 Profile 0.5 S Track Track 0.91+ -58 40 245 4.9 104 Tau
01 Nov 21:41 S 3 Profile 1.0 N Track Track 0.70+ -46 23 216 7.1 Hip 109637
29 Dec 17:39 N 2 Profile 2.0 S Track Track 0.61+ -15 43 157 6.0 88 Psc

Table 3. Grazing lunar occultations.
 


James Appleton