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Venus transits: history and opportunities for planetary, solar and gravitational physics

The data of 2012 transit of Venus are compared with the ones of 2004. The thickness of the atmosphere of Venus, its aureole and the effect of oblateness and other asphericities in the figure of the Sun are taken into consideration, as well as the black drop effect. A new extrapolation method for the contact times is presented. The next Mercury transit in 2016 will be fully visible from Europe, and the data will be gathered in view of this new method of analysis, to obtain the solar diameter.

preprint2013arXivOpen access
Costantino SigismondiXiaofan WangPatrick RocherEugenio Reis-Neto
astro-ph.IMastro-ph.SR
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Costantino SigismondiXiaofan WangPatrick RocherEugenio Reis-Neto

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