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Summary of Lunar Occultations for 2020

More about occultations.

Introduction

During 2020, there are more than 500 lunar occultations potentially observable from East Anglia, although many involve faint stars. The tracks of four grazing occultations cross the region during the year. No lunar occultations of planets 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 brighter than magnitude 6.0, where circumstances are favourable. The 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
2020
Time
(UT)
D
R
Lunar
Phase
Sun
Alt (°)
Star
Alt (°)
Mag Star
09 Jan17:06:11
17:51:22
D
R
0.99+-9
-16
18
25
2.913 Gem, μ Gem
04 Feb21:41:19D0.77+-44535.3106 Tau
05 Feb23:55:10D0.86+-54465.9ZC 928
06 Feb02:14:15
03:04:34
D
R
0.86+-46
-40
26
18
3.37 Gem, η Gem
07 Feb21:19:28D0.97+-40545.310 Cnc, μ2 Cnc
08 Feb03:53:44D0.98+-32275.8ZC 1250
29 Feb20:47:15
21:50:52
D
R
0.31+-30
-37
26
16
5.6ZC 454
29 Mar19:22:55
20:31:10
D
R
0.24+-10
-19
38
28
3.574 Tau, ε Tau
30 Mar22:50:32
23:26:32
D
R
0.34+-32
-33
17
12
4.9114 Tau
03 May21:29:02
22:16:04
D
R
0.82+-15
-19
44
41
43 Vir, ν Vir
05 May21:06:27D0.96+-13295.780 Vir
15 Aug02:41:41
03:39:56
D
R
0.18--15
-9
20
29
5.83 Gem, PU Gem
13 Sep02:07:49
02:47:45
D
R
0.23--27
-23
18
24
5.9ZC 1161
27 Sep21:14:22D0.85+-31194.539 Cap, ε Cap
30 Sep23:42:42D0.99+-41324.430 Psc, YY Psc
21 Oct18:23:12D0.31+-1582.822 Sgr, λ Sgr
11 Nov05:29:15
06:33:08
D
R
0.21--15
-6
33
40
43 Vir, ν Vir
22 Nov20:52:52D0.56+-45185.769 Aqr, τ1 Aqr
22 Nov22:12:39D0.57+-54104.171 Aqr, τ2 Aqr
29 Nov19:14:20D1.00+-31325.9ZC 593
11 Dec05:14:38
06:17:31
D
R
0.16--23
-14
14
21
5.595 Vir
18 Dec18:33:04D0.20+-2495.737 Cap
21 Dec19:54:43
21:05:44
D
R
0.48+-37
-47
27
19
4.430 Psc, YY Psc
21 Dec22:02:12D0.49+-54134.633 Psc, BC Psc
24 Dec18:16:40D0.75+-21425.664 Cet
24 Dec19:36:13D0.75+-34474.465 Cet, ξ1 Cet
27 Dec21:17:16D0.95+-48575.8HU Tau

Table 1. Occultations of stars brighter than magnitude 6.0.
 

Nights With Many Occultation Events

During the year, the Moon traverses some rich star fields. When this happens, many occultations can occur during a short period. Table 2 lists evenings throughout the year when the Moon occults 10 or more stars. (Figures for early morning events are included with those of the previous evening, if any.) The large numbers of occultations during late April are associated with the passage of the Moon through the rich star fields of Gemini.
 

Date, No occs Date, No occs Date, No occs Date, No occs
27 Feb, 12 03 Mar, 10 29 Mar, 13 30 Mar, 10
01 Apr, 19 26 Apr, 12 27 Apr, 40 28 Apr, 13
27 May, 13 - - -

Table 2. Nights with 10 or more occultations.
 

Grazing Occultations

The tracks of four 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 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
2020
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
14 Feb 01:19 S 15 Profile 2.5 N Track Track 0.70- -49 18 132 6.6 ZC2008
27 Feb 18:37 S 22 Profile 0.3 N Track Track 0.14+ -11 24 243 7.4 H7156
15 Aug 02:43 N 2 Profile 3.0 S Track Track 0.18- -15 20 78 8.2 Tyc 1877-1004-1
07 Nov 02:30 N 5 Profile 1.0 S Track Track 0.65- -41 51 123 6.3 ZC1208

Table 3. Grazing lunar occultations.
 

Note: the graze tracks on 15 August and 07 November pass within a few km of Orwell Park Observatory. Unfortunately, in both cases, the tracks pass to the south, and there is no convenient observing location nearby.


James Appleton