Orwell Astronomical Society (Ipswich)
Summary of Lunar Occultations for 2014
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.
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 Feb | 03:58:39 | D | 0.87+ | -31 | 7 | 5.2 | 26 Gem |
11 Feb | 20:10:09 20:45:29 | D R | 0.91+ | -29 -34 | 50 52 | 3.6 | 54 Gem, λ Gem |
13 Feb | 20:32:19 | D | 0.99+ | -32 | 38 | 5.4 | 60 Cnc |
14 Feb | 04:22:38 | D | 0.99+ | -27 | 18 | 5.2 | 76 Cnc, κ Cnc |
07 Mar | 18:30:09 | R | 0.42+ | -8 | 53 | 4.3 | 68 Tau, δ3 Tau |
13 Mar | 21:02:48 | D | 0.92+ | -28 | 45 | 5.4 | 2 Leo, ω Leo |
25 Mar | 04:27:43 | D | 0.37- | -13 | 12 | 3.9 | 44 Sgr, ρ1 Sgr |
04 May | 20:22:05 20:43:37 | D R | 0.29+ | -8 -11 | 31 28 | 3.6 | 54 Gem, λ Gem |
03 Jun | 21:45:57 22:45:09 | D R | 0.32+ | -11 -14 | 15 6 | 5.4 | 2 Leo, ω Leo |
15 Jun | 00:14:56 01:18:10 | D R | 0.95- | -15 -13 | 17 20 | 3.9 | 44 Sgr, ρ1 Sgr |
08 Aug | 21:01:14 22:05:50 | D R | 0.95+ | -12 -18 | 19 20 | 3.9 | 44 Sgr, ρ1 Sgr |
21 Aug | 03:47:42 | D | 0.17- | -9 | 24 | 5.2 | 26 Gem |
18 Sep | 03:27:44 04:31:27 | D R | 0.30- | -19 -10 | 32 41 | 3.6 | 54 Gem, λ Gem |
20 Sep | 04:21:01 05:08:37 | D R | 0.14- | -12 -5 | 22 29 | 5.4 | 60 Cnc |
05 Nov | 17:06:42 | D | 0.98+ | -8 | 11 | 4.3 | 110 Psc, ο Psc |
03 Dec | 02:48:31 | D | 0.87+ | -44 | 8 | 4.3 | 110 Psc, ο Psc |
09 Dec | 06:06:59 07:02:14 | D R | 0.92- | -15 -7 | 31 22 | 3.6 | 54 Gem, λ Gem |
Table 1. Occultations of stars of magnitude 5.5 or brighter.
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.
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.
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