When.com Web Search

Search results

  1. Results From The WOW.Com Content Network
  2. Lightmap - Wikipedia

    en.wikipedia.org/wiki/Lightmap

    They are usually flat, without information about the light's direction, whilst some game engines use multiple lightmaps to provide approximate directional information to combine with normal-maps. Lightmaps may also store separate precalculated components of lighting information for semi-dynamic lighting with shaders, such as ambient-occlusion ...

  3. Spectro-Polarimetric High-Contrast Exoplanet Research

    en.wikipedia.org/wiki/Spectro-Polarimetric_High...

    In addition, SPHERE employs differential imaging to exploit differences between planetary and stellar light in terms of its color or polarization. [5] Other high-contrast imaging systems that are operational include Project 1640 at the Palomar Observatory and the Gemini Planet Imager at the Gemini South Telescope . [ 4 ]

  4. Strömgren sphere - Wikipedia

    en.wikipedia.org/wiki/Strömgren_sphere

    The theory was derived by Bengt Strömgren in 1937 and later named Strömgren sphere after him. The Rosette Nebula is the most prominent example of this type of emission nebula from the H II-regions .

  5. Sphere mapping - Wikipedia

    en.wikipedia.org/wiki/Sphere_mapping

    The map has been created as above, looking at the sphere along the z-axis. The texture coordinate of the center of the map is (0,0), and the sphere's image has radius 1. We are rendering an image in the same exact situation as the sphere, but the sphere has been replaced with a reflective object.

  6. Hill sphere - Wikipedia

    en.wikipedia.org/wiki/Hill_sphere

    The Hill sphere is a common model for the calculation of a gravitational sphere of influence. It is the most commonly used model to calculate the spatial extent of gravitational influence of an astronomical body ( m ) in which it dominates over the gravitational influence of other bodies, particularly a primary ( M ). [ 1 ]

  7. Gliese 436 b - Wikipedia

    en.wikipedia.org/wiki/Gliese_436_b

    Gliese 436 b / ˈ ɡ l iː z ə / (sometimes called GJ 436 b, [7] formally named Awohali [2]) is a Neptune-sized exoplanet orbiting the red dwarf Gliese 436. [1] It was the first hot Neptune discovered with certainty (in 2007) and was among the smallest-known transiting planets in mass and radius, until the much smaller Kepler exoplanet discoveries began circa 2010.

  8. Spherical coordinate system - Wikipedia

    en.wikipedia.org/wiki/Spherical_coordinate_system

    For example, one sphere that is described in Cartesian coordinates with the equation x 2 + y 2 + z 2 = c 2 can be described in spherical coordinates by the simple equation r = c. (In this system—shown here in the mathematics convention—the sphere is adapted as a unit sphere, where the radius is set to unity and then can generally be ignored ...

  9. Celestial sphere - Wikipedia

    en.wikipedia.org/wiki/Celestial_sphere

    Such globes map the constellations on the outside of a sphere, resulting in a mirror image of the constellations as seen from Earth. The oldest surviving example of such an artifact is the globe of the Farnese Atlas sculpture, a 2nd-century copy of an older ( Hellenistic period , ca. 120 BCE) work.