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  2. Methods of detecting exoplanets - Wikipedia

    en.wikipedia.org/.../Methods_of_detecting_exoplanets

    The transit method has also the advantage of detecting planets around stars that are located a few thousand light years away. The most distant planets detected by Sagittarius Window Eclipsing Extrasolar Planet Search are located near the galactic center. However, reliable follow-up observations of these stars are nearly impossible with current ...

  3. 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 ...

  4. Transit-timing variation - Wikipedia

    en.wikipedia.org/wiki/Transit-timing_variation

    Transit-timing variation is a method for detecting exoplanets by observing variations in the timing of a transit. This provides an extremely sensitive method capable of detecting additional planets in the system with masses potentially as small as that of Earth. In tightly packed planetary systems, the gravitational pull of the planets among ...

  5. List of exoplanet search projects - Wikipedia

    en.wikipedia.org/wiki/List_of_exoplanet_search...

    Observe exoplanets using the transit method, study and characterise the planets' chemical composition and thermal structures 4 years RST: 2026 To search for and study exoplanets while studying dark matter. It is expected to find about 2,500 planets. 6 years PLATO: 2026 (Ariane 62) To search for and characterize rocky planets around stars like ...

  6. Sagittarius Window Eclipsing Extrasolar Planet Search

    en.wikipedia.org/wiki/Sagittarius_Window...

    g Extrasolar Planet Search, or SWEEPS, was a 2006 astronomical survey project using the Hubble Space Telescope's Advanced Camera for Surveys - Wide Field Channel to monitor 180,000 stars for seven days to detect extrasolar planets via the transit method.

  7. Next-Generation Transit Survey - Wikipedia

    en.wikipedia.org/wiki/Next-Generation_Transit_Survey

    The Next-Generation Transit Survey (NGTS) is a ground-based robotic search for exoplanets. [1] The facility is located at Paranal Observatory in the Atacama Desert in northern Chile, about 2 km from ESO's Very Large Telescope and 0.5 km from the VISTA Survey Telescope.

  8. XO Project - Wikipedia

    en.wikipedia.org/wiki/XO_Project

    McCullough and his team employed a relatively inexpensive telescope called the XO Telescope, made from commercial equipment, to search for extrasolar planets.The construction of the one-of-a-kind telescope cost $60,000 for the hardware, and much more than that for the associated software. [4]

  9. XO-1b - Wikipedia

    en.wikipedia.org/wiki/XO-1b

    While astronomers had detected more than 180 extrasolar planets, XO-1b is only the tenth planet discovered using the transit method. It is only the second planet found using telephoto lenses. The first, TrES-1, in the constellation Lyra, was reported in 2004. The transit method allows astronomers to determine a planet's size. Secondary transits ...