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  2. Planetary transits and occultations - Wikipedia

    en.wikipedia.org/wiki/Planetary_transits_and...

    In astronomy, planetary transits and occultations occur when a planet passes in front of another object, as seen by an observer.The occulted object may be a distant star, but in rare cases it may be another planet, in which case the event is called a mutual planetary occultation or mutual planetary transit, depending on the relative apparent diameters of the objects.

  3. Astronomical transit - Wikipedia

    en.wikipedia.org/wiki/Astronomical_transit

    The transit method can be used to discover exoplanets. As a planet eclipses/transits its host star it will block a portion of the light from the star. If the planet transits in-between the star and the observer the change in light can be measured to construct a light curve. Light curves are measured with a charge-coupled device. The light curve ...

  4. List of transiting exoplanets - Wikipedia

    en.wikipedia.org/wiki/List_of_transiting_exoplanets

    The first known planet to be discovered with the transit method was OGLE-TR-56b. The first planetary transit observed (by already known exoplanet) was caused by HD 209458 b. The most massive transiting exoplanet is KELT-1b which masses 27.23 M J (making it a brown dwarf) while the least massive is Kepler-42d which masses less than 0.003 M J or ...

  5. Transit of Venus - Wikipedia

    en.wikipedia.org/wiki/Transit_of_Venus

    The last transit not to be part of a pair was in 1396 (the planet passed slightly above the disc of the Sun in 1388); [33] the next one will be in 3089. [citation needed] After 243 years the transits of Venus return. The 1874 transit is a member of the 243-year cycle #1. The 1882 transit is a member of #2.

  6. Transit-timing variation - Wikipedia

    en.wikipedia.org/wiki/Transit-timing_variation

    Transit-timing variation was first convincingly detected for planets Kepler-9b and Kepler-9c [13] and gained popularity by 2012 for confirming exoplanet discoveries. [14] TTV can also be used to indirectly measure the mass of the exoplanets in compact, multiple-planet systems and/or system whose planets are in resonant chains.

  7. Transit of Earth from Mars - Wikipedia

    en.wikipedia.org/wiki/Transit_of_Earth_from_Mars

    Earth and Moon transiting the Sun in 2084, as seen from Mars. Image created using SpaceEngine Earth and Moon from Mars, as photographed by the Mars Global Surveyor. A transit of Earth across the Sun as seen from Mars takes place when the planet Earth passes directly between the Sun and Mars, obscuring a small part of the Sun's disc for an observer on Mars.

  8. Transit of Mercury - Wikipedia

    en.wikipedia.org/wiki/Transit_of_Mercury

    Depending on the chord of the transit and the position of the planet Mercury in its orbit, the maximum length of this event is 7 h 50 m. [2] Transit events are useful for studying the planet and its orbit. Examples of the scientific investigations based on transits of Mercury are: Measuring the scale of the Solar System. [3]

  9. Transit of Mercury from Mars - Wikipedia

    en.wikipedia.org/wiki/Transit_of_Mercury_from_Mars

    The rover Curiosity observed the Mercury transit of June 3, 2014, marking the first time any planetary transit has been observed from a celestial body besides Earth. [ 1 ] March 5, 2024: NASA released images of transits of the moon Deimos , the moon Phobos and the planet Mercury as viewed by the Perseverance rover on the planet Mars.