• The effective temperature of a body such as a star or planet is the temperature of a black body that would emit the same total amount of electromagnetic...
    16 KB (1,953 words) - 16:53, 9 November 2024
  • Thumbnail for Greenhouse effect
    radiation has an associated effective radiating temperature or effective temperature. Effective temperature is the temperature that a black body (a perfect...
    84 KB (8,967 words) - 06:04, 25 December 2024
  • Thumbnail for Color temperature
    unadjusted temperature, derived from comparison to a black-body radiator. The Sun closely approximates a black-body radiator. The effective temperature, defined...
    32 KB (3,546 words) - 08:23, 26 November 2024
  • Thumbnail for Stefan–Boltzmann law
    the stellar radius and T is the effective temperature. This formula can then be rearranged to calculate the temperature: T = L 4 π R 2 σ 4 {\displaystyle...
    38 KB (5,480 words) - 06:27, 2 December 2024
  • In telecommunications, effective input noise temperature is the source noise temperature in a two-port network or amplifier that will result in the same...
    636 bytes (107 words) - 19:14, 4 September 2024
  • Thumbnail for Black-body radiation
    fraction of its energy as ultraviolet radiation. The Sun, with an effective temperature of approximately 5800 K, is an approximate black body with an emission...
    70 KB (8,800 words) - 06:27, 2 December 2024
  • Thumbnail for Black body
    stars and planets is sometimes characterized in terms of an effective temperature, the temperature of a black body that would emit the same total flux of electromagnetic...
    47 KB (5,217 words) - 03:22, 29 November 2024
  • Thumbnail for List of largest stars
    parameters used in calculations, such as stellar luminosity and effective temperature. Often stellar radii can only be expressed as an average or be within...
    250 KB (10,635 words) - 08:02, 21 December 2024
  • near-surface air temperature and sea surface temperature Surface temperature of a star, often the effective temperature Instrumental temperature record, the...
    740 bytes (138 words) - 01:26, 18 November 2023
  • Thumbnail for Stephenson 2 DFK 1
    with Stephenson 2 blending into its immediate surroundings. An effective temperature of 3,200 K was calculated in a 2012 study by SED integration using...
    21 KB (2,391 words) - 00:57, 26 December 2024
  • Thumbnail for Kelvin
    upon their surface temperature, known as effective temperature. The photosphere of the Sun, for instance, has an effective temperature of 5772 K [1][2][3][4]...
    42 KB (4,561 words) - 07:57, 25 December 2024
  • this concept, such as equivalent blackbody temperature of a planet. The effective radiation emission temperature is a related concept, but focuses on the...
    18 KB (2,279 words) - 23:39, 5 July 2024
  • Thumbnail for G-type main-sequence star
    spectral type G. Such a star has about 0.9 to 1.1 solar masses and an effective temperature between about 5,300 and 6,000 K (5,000 and 5,700 °C; 9,100 and 10...
    12 KB (1,170 words) - 15:02, 23 November 2024
  • Thumbnail for Temperature
    Temperature is a physical quantity that quantitatively expresses the attribute of hotness or coldness. Temperature is measured with a thermometer. It reflects...
    104 KB (12,961 words) - 20:55, 7 December 2024
  • Thumbnail for Thermal comfort
    floor temperatures stay in the range of 19–29 °C (66–84 °F) in spaces where occupants will be wearing lightweight shoes. Standard effective temperature (SET)...
    73 KB (9,373 words) - 06:54, 16 December 2024
  • Thumbnail for Betelgeuse
    fluctuating radial velocity, moderate radius and low variation in effective temperature, as of 2024. Parallax is the apparent change of the position of...
    174 KB (18,528 words) - 03:13, 20 December 2024
  • Thumbnail for VV Cephei
    diffuse star orbiting a hot companion. The effective temperature generally quoted for stars is the temperature of a spherical blackbody that approximates...
    26 KB (2,765 words) - 13:47, 22 December 2024
  • Thumbnail for Hertzsprung–Russell diagram
    magnitudes or luminosities and their stellar classifications or effective temperatures. The diagram was created independently in 1911 by Ejnar Hertzsprung...
    23 KB (2,771 words) - 01:42, 18 July 2024
  • Thumbnail for Gliese 581c
    calculate Gliese 581c's effective temperature, a.k.a. black body temperature, which probably differs from its surface temperature.[citation needed] According...
    38 KB (3,772 words) - 03:01, 15 November 2024
  • 'equivalent temperature" or 'effective temperature' to describe combined effects of convective and radiant heat transfer. In design, operative temperature can...
    4 KB (591 words) - 01:52, 21 August 2022
  • work form, where T 0 {\displaystyle T_{0}} is replaced by some effective temperature. When this is done, it often enlarges the scope of the theorem,...
    22 KB (3,216 words) - 00:20, 13 January 2024
  • Thumbnail for VY Canis Majoris
    maser emission. The effective temperature of this star is uncertain. Some signature changes in its spectrum correspond to temperature variations. Early...
    63 KB (6,874 words) - 08:26, 2 December 2024
  • Thumbnail for Orders of magnitude (temperature)
    Joachim; Pauldrach, A. W. A. (2004). "The Physical Properties and Effective Temperature Scale of O-Type Stars as a Function of Metallicity. I. A Sample...
    46 KB (1,239 words) - 10:54, 10 December 2024
  • Thumbnail for Photosphere
    to have a temperature given by the effective temperature in the Stefan–Boltzmann law. Various stars have photospheres of various temperatures. The Sun...
    9 KB (777 words) - 18:12, 18 August 2024
  • Thumbnail for Star
    Star (section Temperature)
    the star's color index. The temperature is normally given in terms of an effective temperature, which is the temperature of an idealized black body that...
    148 KB (16,436 words) - 08:32, 2 December 2024
  • effective temperature given above, the temperature is used to construct an effective classical model. However, this form of the effective temperature...
    12 KB (2,162 words) - 14:01, 29 February 2024
  • Thumbnail for Luminosity
    measure with any certainty. Since the effective temperature is merely a number that represents the temperature of a black body that would reproduce the...
    24 KB (3,002 words) - 09:29, 25 September 2024
  • Thumbnail for K-type main-sequence star
    E. Mamajek (2022-04-16). "A Modern Mean Dwarf Stellar Color and Effective Temperature Sequence". Retrieved 2022-05-14. Steigerwald, Bill (10 March 2019)...
    13 KB (1,418 words) - 02:38, 16 December 2024
  • Thumbnail for Red supergiant
    Bertrand; Josselin, Eric; Maeder, Andre; Meynet, Georges (2005). "The Effective Temperature Scale of Galactic Red Supergiants: Cool, but Not as Cool as We Thought"...
    34 KB (4,286 words) - 07:41, 14 December 2024
  • Thumbnail for WOH G64
    based on the assumption of an effective temperature of 3,200 K. In 2009, Levesque calculated an effective temperature of 3,400±25 K by spectral fitting...
    21 KB (2,290 words) - 04:15, 9 December 2024