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  2. BIRT Project - Wikipedia

    en.wikipedia.org/wiki/BIRT_Project

    Major release as part of Eclipse Kepler Simultaneous Release [13] 4.3.1 September 27, 2013 Maintenance release 4.3.2 February 28, 2014 Maintenance release 4.4.0 June 25, 2014 Major release as part of Eclipse Luna Simultaneous Release [14] 4.4.1 September 26, 2014 Maintenance release 4.4.2 February 27, 2015 Maintenance release 4.5.0 June 24, 2015

  3. Eclipse (software) - Wikipedia

    en.wikipedia.org/wiki/Eclipse_(software)

    Eclipse (software) Eclipse is an integrated development environment (IDE) used in computer programming. [5] It contains a base workspace and an extensible plug-in system for customizing the environment. It is the second-most-popular IDE for Java development, and, until 2016, was the most popular. [6]

  4. Kepler orbit - Wikipedia

    en.wikipedia.org/wiki/Kepler_orbit

    Kepler orbit. An elliptic Kepler orbit with an eccentricity of 0.7, a parabolic Kepler orbit and a hyperbolic Kepler orbit with an eccentricity of 1.3. The distance to the focal point is a function of the polar angle relative to the horizontal line as given by the equation (13) In celestial mechanics, a Kepler orbit (or Keplerian orbit, named ...

  5. Kepler's laws of planetary motion - Wikipedia

    en.wikipedia.org/wiki/Kepler's_laws_of_planetary...

    t. e. In astronomy, Kepler's laws of planetary motion, published by Johannes Kepler between 1609 and 1619, describe the orbits of planets around the Sun. The laws modified the heliocentric theory of Nicolaus Copernicus, replacing its circular orbits and epicycles with elliptical trajectories, and explaining how planetary velocities vary.

  6. List of exoplanet extremes - Wikipedia

    en.wikipedia.org/wiki/List_of_exoplanet_extremes

    Kepler-42: b, c, d: 1 Kepler-42 b, c and d have a semi-major axis of 0.0116, 0.006 and 0.0154 AU, respectively. Kepler-70 b, c and d (all unconfirmed and disputed) have a semi-major axis of only 0.006, 0.0076 and ~0.0065 AU, respectively. Multiplanetary system with largest mean semi-major axis (planets are farthest from their star) TYC 8998-760 ...

  7. Methods of detecting exoplanets - Wikipedia

    en.wikipedia.org/wiki/Methods_of_detecting_exo...

    The transiting planet Kepler-19b shows TTV with an amplitude of five minutes and a period of about 300 days, indicating the presence of a second planet, Kepler-19c, which has a period which is a near-rational multiple of the period of the transiting planet.

  8. Historical models of the Solar System - Wikipedia

    en.wikipedia.org/wiki/Historical_models_of_the...

    Instead Kepler developed a more accurate and consistent model where the Sun is located not in the centre but at one of the two foci of an elliptic orbit. [71] Kepler derived the three laws of planetary motion which changed the model of the Solar System and the orbital path of planets. These three laws of planetary motion are:

  9. Circumbinary planet - Wikipedia

    en.wikipedia.org/wiki/Circumbinary_planet

    On 15 September 2011, astronomers, using data from NASA's Kepler space telescope, announced the first partial-eclipse-based discovery of a circumbinary planet. [ 9 ] [ 10 ] The planet, called Kepler-16b , is about 200 light years from Earth, in the constellation Cygnus, and is believed to be a frozen world of rock and gas, about the mass of Saturn.