Transits of Venus Lunar Eclipses Occultation of planets by Moon Solar eclipses during transit Solar System Planetary Transits Mutual Planetary Transits

Transit of Venus

2012 Jun 06

Local Circumstances


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General Information
                           Transiting Planet = Venus
                            Greatest Transit = 2012 Jun 06 01:30:43 TT
                               Gr. Longitude = 157° 13.6' E
                                Gr. Latitude =  22° 49.4' N
                              Transit Series = 7
                               Series Member = 7 of 47
Local Circumstances
                            Longitude =  25° 20' 00" E
                             Latitude =  42° 12' 00" N
                            Elevation = 169m.
                          Temperature = 10°C
                             Pressure = 1010 hPA
                                   ΔT = 67.75s

             Calendar Date and Time     Azi    Alt     PA     Sep     S.D.

Rise         2012-Jun-06 02:43:34.2    57.8°   0.0°  317.3°  606.2"  29.4"
Contact III  2012-Jun-06 04:37:40.7    75.9°  18.9°  291.4°  916.3"  29.4"
Contact IV   2012-Jun-06 04:55:24.6    78.6°  22.1°  289.0°  975.1"  29.4"
Transit of Venus
Explaination of prediction
Greatest Transit        The instant of minimum geocentric angular separation between centers of Venus and Sun,
                        in Terrestrial Time.
Gr. Longitude/Latitude  WGS 84 coordinates of location at which Venus is directly overhead at Greatest Transit.
Transit Series          Transits of Venus, separated by roughly 243 years are said to form transit series.
                        All transits that belong to one such series occur near either planet's ascending or 
                        descending node.
Series Member           Number of consecutive transit from the specified transit series.
Longitude/Latitude      The observer's WGS 84 geographical coordinates. Default: Chirpan, Bulgaria.
Elevation               Elevation of observer with respect to the WGS 84 oblate spheroid, in meters.
Temperature/Pressure    Atmospheric conditions at observer's location. Affect rise/set times and apparent 
                        altitudes of Sun and Venus. Default: 10° C & 1010 hPA.
ΔT                      The estimated arithmetic difference between Terrestrial Time and Universal Time.
Calendar Date and Time  Calendar Date and Time of specific event, in Gregorian calendar and Universal Time, 
                        assuming specified value of ΔT.
Contact I               Apparent discs of Venus and Sun are externally tangent, a.k.a exterior ingress.
Contact II              Apparent discs of Venus and Sun are internally tangent, a.k.a interior ingress.
Contact III             Apparent discs of Venus and Sun are internally tangent, a.k.a interior egress.
Contact IV              Apparent discs of Venus and Sun are externally tangent, a.k.a exterior egress.
Rise/Set                If transit is in progress at rise or set, estimated times of rise or set are 
                        displayed. Affected by Temperature and Pressure settings.
Azi                     Planetary Azimuth at specified time (0 = North; 90 = East; 180 = South; 270 = West).
Alt                     Planetary Altitude at specified time, including refraction (0 = horizon; 90 = zenith).
PA                      Position angle of Venus's center with respect to the center of Sun (0 = North;
                        90 = East; 180 = South; 270 = West).
Sep                     Separation between centers of Sun and Venus, in arcseconds.
S.D.                    Apparent angular semi-diameter of Venus, in arcseconds.
Duration                Time interval between transit's first and fourth contacts.

About Predictions

Local Circumstances Generator makes use of JPL DE421 ephemerides and numerical integration software SOLEX. Geocentric positions of Sun and Venus through one minute intervals were generated, which were then converted to topocentric. Local circumstances were then computed on the assumption of linear motion during these intervals, which should be accurate enough for most purposes. Rise and set times are typically accurate to about a minute, due to impossibility to predict exact atmospheric refraction. Rise and set times are computed for the instant at which center of planetary disc would be at apparent horizon, using Saemundsson's formula for computing refraction near horizon. By default, air temperature of 10 degrees celsius and atmospheric pressure of 1010 hectopascals are assumed. These can be changed over a certain range in order to get more accurate times and see what effect could temperature and air pressure have on apparent positions.


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