Referring to the H-R Diagram, how can the sun be described in terms of actual (absolute) magnitude, temperature, color and spectral class?
The sun's absolute magnitude (actual brightness) 4.83, its temperature is 5,778 K, its class is G2, and its color is yellow on the HR diagram.
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The Sun can be described on the H-R Diagram as having an absolute magnitude of about +4.83, a temperature of approximately 5,500 degrees Celsius, a color classified as yellow-white, and a spectral class of G2V.
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The Sun can be described in terms of actual (absolute) magnitude, temperature, color, and spectral class as follows:
- Actual (absolute) magnitude: The Sun has an absolute magnitude of around +4.83.
- Temperature: The surface temperature of the Sun is approximately 5,500 degrees Celsius (9,932 degrees Fahrenheit).
- Color: The color of the Sun, as seen from Earth, appears as a yellow-white due to its surface temperature and composition.
- Spectral class: The Sun is classified as a G-type main-sequence star, often referred to as a yellow dwarf. Its spectral class is G2V, indicating a moderately hot star in the main sequence.
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When evaluating a one-sided limit, you need to be careful when a quantity is approaching zero since its sign is different depending on which way it is approaching zero from. Let us look at some examples.
When evaluating a one-sided limit, you need to be careful when a quantity is approaching zero since its sign is different depending on which way it is approaching zero from. Let us look at some examples.
When evaluating a one-sided limit, you need to be careful when a quantity is approaching zero since its sign is different depending on which way it is approaching zero from. Let us look at some examples.
When evaluating a one-sided limit, you need to be careful when a quantity is approaching zero since its sign is different depending on which way it is approaching zero from. Let us look at some examples.
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