How bright a star is how it is burning its gases and the color depends on WHAT gasses it is burning, the sun is red because it is seperating hydrogen atoms apart and creating helium atoms which have two orbiting particles. and in doing so it creates enormous amount of heat that is why the sun is both hot and red and bright.
Venus is close to the Sun, and it has a thick cloud cover. That accounts for its relative brightness.
Close to absolute zero.
Venus has a surface temperature close to this.Venus has a surface temperature close to this.Venus has a surface temperature close to this.Venus has a surface temperature close to this.
If the sun will be close to earth, earth's temperature will increase. It will be too hot.
Yes, tulips typically open during the day and close at night. This behavior is known as nyctinasty, which is a natural response to changes in light and temperature. Tulips usually open in the morning and close in the evening to protect their flowers and conserve energy.
how are temperature the amount of heat transferred and change in in temperature of related
how are temperature the amount of heat transferred and change in in temperature of related
No. The stars are not only not the same brightness, they are not the same distance from us - they just "appear" to be as part of the optical illusion of earthbound astronomy. They are all of varying brightness, though fairly close in brightness overall.
Venus is close to the Sun, and it has a thick cloud cover. That accounts for its relative brightness.
Distance and intervenng or close celestial bodies
Distance and intervenng or close celestial bodies
Distance and intervenng or close celestial bodies
Distance and intervenng or close celestial bodies
Information on millions of stars shows that there is a relationship between temperature and brightness. Surface temperature is measured in degrees C and brightness is measured in absolute magnitude (the star's brightness at a standard distance). If all the stars are plotted on a graph of temperature against absolute magnitude, called a Hertzsprung-Russell diagram, very many of them lie close to a straight line that is called the Main Sequence. There are some stars that do not lie on the Main Sequence, notably the red giants that are very bright despite having a relatively low temperature. The Sun is right in the middle of the Main Sequence showing it is an average star in the middle of its life and very stable.
Distance and intervenng or close celestial bodies
Information on millions of stars shows that there is a relationship between temperature and brightness. Surface temperature is measured in degrees C and brightness is measured in absolute magnitude (the star's brightness at a standard distance). If all the stars are plotted on a graph of temperature against absolute magnitude, called a Hertzsprung-Russell diagram, very many of them lie close to a straight line that is called the Main Sequence. There are some stars that do not lie on the Main Sequence, notably the red giants that are very bright despite having a relatively low temperature. The Sun is right in the middle of the Main Sequence showing it is an average star in the middle of its life and very stable.
Information on millions of stars shows that there is a relationship between temperature and brightness. Surface temperature is measured in degrees C and brightness is measured in absolute magnitude (the star's brightness at a standard distance). If all the stars are plotted on a graph of temperature against absolute magnitude, called a Hertzsprung-Russell diagram, very many of them lie close to a straight line that is called the Main Sequence. There are some stars that do not lie on the Main Sequence, notably the red giants that are very bright despite having a relatively low temperature. The Sun is right in the middle of the Main Sequence showing it is an average star in the middle of its life and very stable.