stellar luminosity उदाहरण वाक्य
उदाहरण वाक्य
- Their great stellar luminosities are determined from various spectral features, which are sensitive to surface gravity, such as H? line widths in hot stars or a strong Balmer discontinuity in cooler stars.
- For perspective, the overall range of stellar luminosities runs from dwarfs less than 1 / 10, 000th as luminous as the Sun, to supergiants over 1, 000, 000 times more luminous.
- This led to systematic differences in bolometric corrections scales, which when combined with incorrect assumed absolute bolometric magnitudes for the Sun could lead to systematic errors in estimated stellar luminosities ( and stellar properties calculated which rely on stellar luminosity, such as radii, ages, and so on ).
- This led to systematic differences in bolometric corrections scales, which when combined with incorrect assumed absolute bolometric magnitudes for the Sun could lead to systematic errors in estimated stellar luminosities ( and stellar properties calculated which rely on stellar luminosity, such as radii, ages, and so on ).
- In the current system of stellar classification, stars are grouped according to temperature, with the massive, very young and energetic Class M stars exhibit temperatures less than 3, 500 K . Because luminosity is proportional to temperature to the fourth power, the large variation in stellar temperatures produces an even vaster variation in stellar luminosity.