The luminosity of a white dwarf star can vary depending on its mass and age, but typically ranges from about 0.001 to 0.1 times the luminosity of the Sun. These stars are small and dense, with surface temperatures ranging from 8,000 to 100,000 Kelvin, which affects their brightness.
Through a comparison of solar luminosity and temperature seen with the H-R diagram. On this diagram, stars sharing the same temperature but different luminosities show measurable differences in radius as well as mass. So if two stars both have the same visible surface temperature but one is more luminous, it has to be larger. This is further explained by Stefan Boltzmann's law,L=(4πR^2 x sigma(constant) x T^4)A Star with the the same surface temperature with larger surface area results in more Luminosity.
The average surface temperature of Mars is about -80 degrees Fahrenheit (-62 degrees Celsius). However, temperatures can vary significantly depending on the season and location on the planet.
The temperature of the sky can vary depending on factors such as location, time of day, and weather conditions. The sky itself does not have a specific temperature, but the air temperature in the sky can range from very cold at high altitudes to warm near the Earth's surface.
The average surface temperature on Mercury is around 700 K (426.85°C). However, temperatures can vary greatly depending on the location and time of day due to Mercury's lack of atmosphere to regulate heat.
The luminosity of a white dwarf star can vary depending on its mass and age, but typically ranges from about 0.001 to 0.1 times the luminosity of the Sun. These stars are small and dense, with surface temperatures ranging from 8,000 to 100,000 Kelvin, which affects their brightness.
No. Main sequence stars vary greatly in both temperature and luminosity. The least massive stars, red dwarfs, can have temperatures as low as 2,300 Kelvin and luminosity as low as 0.015% that of the sun. The most massive stars, which are blue in color can have temperatures as high as 50,000 Kelvin and may be hundreds of thousands times more luminous than the sun.
Aquarius' color is often described as blue or blue-green. Its surface temperature can vary, but it typically ranges from 5,000 to 6,000 degrees Celsius.
Surface temperature refers to the temperature of an object or material on its outermost layer or the immediate area at the interface with the surrounding environment. It can vary greatly based on the type of material, location, and external factors such as sunlight or insulation. Monitoring surface temperatures is important in various fields like engineering, environmental science, and materials processing.
The temperature of an iceberg can vary, but it is typically around -10 to -20 degrees Celsius at the surface.
As the brightness of main sequence stars increases, their temperature also increases. This is because the brightness of a star is directly related to its surface temperature, with hotter stars emitting more energy and appearing brighter. This relationship is described by the Stefan-Boltzmann law.
The stars in the constellation Hercules vary in color from blue to yellow to red, depending on their temperature. The surface temperature of stars in Hercules typically ranges from 3,000 to 30,000 degrees Celsius.
The differences of star temperatures is very great. For example, three of the stars we know well:are Sol (our sun) with a temperature at the photosphere of 5,778° KBetelgeuse (a red dwarf) with a temperature of 3,140–3,641° Kand Bellatrix (a white dwarf) with a temperature of 22,000° K
The average surface temperature of star Beta (β) can vary depending on the specific star that it refers to. Without a specific star identified, it is not possible to provide an accurate average surface temperature for star Beta.
It depends on the tile of the earth's Axis.....i think
it has no atmosphere to smooth out temperatures, and each day and night lasts a fortnight
Through a comparison of solar luminosity and temperature seen with the H-R diagram. On this diagram, stars sharing the same temperature but different luminosities show measurable differences in radius as well as mass. So if two stars both have the same visible surface temperature but one is more luminous, it has to be larger. This is further explained by Stefan Boltzmann's law,L=(4πR^2 x sigma(constant) x T^4)A Star with the the same surface temperature with larger surface area results in more Luminosity.