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The transit and related science Venus is one of the most intriguing bodies in the Solar System. It is almost the same size as the Earth and apparently has a simil...
Sample pictures from Lowell Observatory (P. Tanga, W. Sheehan, K. Brausch, W. Burke, J. Roberts) Very good transparency, but bad seeing and wind disturbing the ob...
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Main.JenniferP 23 May 2012 In May 15th, scientists from OCA and OBSPM collaboration have given one last press conference at the Observatory of Paris. Starting wit...
The poorly known L type asteroids and the intriguing Barbarians We investigate the poorly known L type asteroids as some of them (known as "Barbarians") are known...
Photometry One of the most important sources of information about asteroid physical parameters is photometry typical kilometer sized asteroids (up to diameters ...
Stellar occultations for asteroid astrometry Motivations The high quality astrometry of Gaia offers unique opportunities for solar system science. Apart from t...
Occultation astrometry major goals The power of Gaia based predictions was demonstrated by the successful observation of a MU69/Arrokoth occultation (New Horizo...
Densities of asteroids: convex shape models and Gaia masses This project focus on the volume determination by scaling the convex shape models in size. To determin...
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Densities of asteroids: convex shape models and Gaia masses This project focus on the volume determination by scaling the convex shape models in size. To determin...
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Why a coronograph? We plan to image Venus when it is close to the solar limb, around the transit event occuring on June 5 6, 2012, when twilight phenomena become ...
Shape determination Orbital parameters are currently known for more than 500 000 asteroids. On the other hand, rotational states and shapes were determined only f...
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Coronagraph placement Venus TEx Coronographs map here The following table indicates the sites, the observer(s) and the associated filters for each of them: 1 ...