Dwarf Stars
Moment Magnitudes are considered more accurate than Richter Scale Magnitudes because Moment Magnitudes take into account all seismic energy released during an earthquake. Additionally, Moment Magnitudes are more suitable for measuring larger earthquakes, while Richter Scale Magnitudes are more commonly used for smaller earthquakes.
Absolute magnitude and apparent magnitude are the same because they are both ways on how to measure the brightness of a star. Absolute magnitude is how bright is the star if we will see it in a 32.616 light-years distance while apparent magnitude is the brightness of it that we see on Earth.
One drawback of absolute dating methods is that they can be costly and time-consuming to perform, often requiring specialized equipment and expertise. Additionally, some absolute dating techniques are limited in their applicability to certain types of materials or time ranges.
The moment magnitude scale is used by seismologists to measure the amount of energy released by large earthquakes (those greater than magnitude 8.0). For smaller earthquakes (those with magnitudes less than 7.0 and with epicentres less than 650 km from a seismometer station may be used) the method devised by Richter (the Richter magnitude scale) may be used to estimate the magnitude. The surface wave magnitude scale may be used for earthquakes with magnitudes up to 8.0 (devised by Richter and Gutenberg to extend the utility of the Richter scale.) Richter magnitudes are generally easier to derive than moment magnitudes being based on direct seismometer measurements, whereas the moment magnitude is a more4 fundamental measurement of magnitude being based on the rock mass strength around the fault, the amplitude of fault movement and the cross sectional area of that portion of the fault that moved. However this is more difficult to measure. As such it is common for initial reports to be in Richter magnitudes and more detailed letter magnitudes to be reported as moment magnitudes.
Shallow focus earthquakes occur closer to the Earth's surface (up to 70 km deep) and typically have higher magnitudes due to proximity to the Earth's brittle crust. Deep focus earthquakes occur at depths of 300-700 km within the subducting slab in a subduction zone and are usually associated with more intense pressure and temperature conditions, resulting in unique seismic waves and less damage on the Earth's surface.
dwarf stars -Sydney-
Spica has a surface temperature of 22,400K and an absolute magnitude of -3.55Rigel has a surface temperature of 11,000K and an absolute magnitude of -6.7So the question is incorrect.
Yes, if the matter surrounding one star is more dense than that surrounding the other it would appear to be less bright.
supergiant
According to Wikipedia giants have absolute magnitudes around 0 to -1 while supergiants have absolute magnitudes around -5 so they are 50-100 times brighter (5 magnitudes difference equals 100 times brighter).
The less luminous one is closer to the observer, just as a candle in the same room can seem as bright as a sodium vapor lamp down the street.
If the radius of Betelgeuse varies by 60% within three years, its luminosity will also change proportionally. Since absolute magnitude is related to luminosity, the ratio of the two absolute magnitudes will be the square root of the ratio of the luminosities. So, the ratio of the two absolute magnitudes will be approximately 1.22.
ble
Red giants have typical absolute magnitudes which are 10-15 magnitudes below white dwarfs, which means that the red giants are 10,000-1,000,000 times brighter, after due allowance for distance.
It can be a plus or a miuns - depending on which one of the two had a greater absolute value. Also, it will be nearer to zero than the larger of the two magnitudes.
No. The magnitude of a vector can't be less than any component.
Cassiopeia is a constellation, not a single star, so it does not have a specific absolute magnitude. The stars within the constellation Cassiopeia have a range of absolute magnitudes depending on their distance and luminosity.