Everything about Transit Of Mercury From Venus totally explained
A
transit of Mercury across the Sun as seen from Venus takes place when the planet
Mercury passes directly between the
Sun and
Venus, obscuring a small part of the Sun's disc for an observer on Venus. During a
transit, Mercury can be seen from Venus as a small black disc moving across the face of the Sun. The duration of a central transit is 6.2 hours.
Transits of Mercury from Venus occur in an irregular fashion: sometimes there are several per decade, while on other occasions there are longer gaps. The overall frequency seems to be somewhat greater than the frequency of
transits of Mercury from Earth.
Naturally, no one has ever seen a transit of Mercury from Venus.
The Mercury-Venus
synodic period is 144.5662 days. It can be calculated using the formula 1/(1/P-1/Q), where P is the
orbital period of Mercury (87.968435 days) and Q is the orbital period of Venus (224.695434 days).
The
inclination of Mercury's orbit with respect to Venus's
ecliptic is 4.33°, which is less than its value of 7.00° with respect to Earth's ecliptic.
The transit that occurred on
March 22,
1894 was particularly interesting because on the 21st, when it began, there were also
transits of Venus and
of Mercury visible from Saturn. There was no overlap among the three transits, however.
Past and future transits
Further Information
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