A Star That Is Cool and Very Luminous Must Have

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A very great distance e. C a very small mass.


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Dwarf stars can have the same temperatures of main sequence stars.

. For a red giant have a red light inside a 5-inch globe. A star that is cool and very luminous must have a a very low velocity b a very small mass c a very small radius d a very large radius e a very great distance 12. A star that is cool and very luminous must have a a very great distance.

A cool but very luminous star must have ________. Star betelguese in Orion is 10000 more luminous than the Sun yet its surface temperature is about half that of the sun which implies that the suns radius is much smaller than the radius of betelguese. Classification of Stars-Stars not in the Main Sequence Some stars are relatively cool but very luminous They must have very large radii to give off so much energy They are the Giantsand Supergiants Other stars are hot but very dim They must have very small radii to give off so little energy They are the White Dwarfs OLLI Winter 2021 11.

The surface temperature of Rigel is about 12000 K and the surface temperature of Betelgeuse is about 3000 K. What is its distance. Wrap crumpled tissue paper around the outside of the globe.

D a very large radius. They are relatively cool but very luminous. Click again to see term.

Which of the following stars has the hottest surface. The universe became transparent to radiation once atoms formed and photons became decoupled from matter. For a steady star have a yellow light inside a 2-inch globe.

Evidence that life on Earth is very ancient comes from fossil algae in rocks more than 3 billion years This problem has been solved. A star that is cool and very luminous must have a low recessional velocity. Tap card to see definition.

C a very small radius. The hotter a star gets the more energy it emits. A star has a parallax of 004 arc seconds.

A star that is cool and very luminous must have a a very great distance. A few nearby stars are more luminous than the Sun but. C a very small mass.

Cooler less luminous main sequence stars have A higher masses. A very large radius b. Other stars are hot but very dim.

Stars Rigel and Betelgeuse in Orion have nearly equal luminosity of about 120000 solar luminosity. B a very small mass. B a very large radius.

A a very large radius. This is a list of stars arranged by their absolute magnitude their intrinsic stellar luminosityThis cannot be observed directly so instead must be calculated from the apparent magnitude the brightness as seen from Earth the distance to each star and a correction for interstellar extinctionThe entries in the list below are further corrected to provide the bolometric. Two stars U and W have the same radius but.

Solutions for Chapter 13 Problem 5TY. To determine the stars absolute magnitude you need to know the stars a. A star that is cool and very luminous must havea a very large radiusb a very small radiusc a very small massd a.

True Stars on the main sequence have different luminosities because. B a very small radius. A very small mass d.

4 light years B. B a very small radius. Luminosity of Star R2 x T4.

For a newborn star have an orange light inside a 3-inch globe. A star that is cool and very luminous must have. A a very great distance.

C a very small radius. The hottest O and B type stars are usually binary stars while the coolest M type stars are usually single stars. And cool red stars less than 3000 Kelvin at.

C the same masses as hotter stars. Very low velocity 21. D a very low velocity.

A star that is cool and very luminous must have. Rigel has a smaller radius than Betelgeuse. D a very small radius.

C a very small mass. B a very large radius. A a very large radius.

Red Giants are larger in diameter than main sequence stars. D a very small radius. Stars with masses in excess of 50 solar masses are very common.

C a very small mass. C a very small mass. D a very great distance.

A star that is cool and very luminous must have a a very great distance. D a very large radius. For a planetary nebula have a red light inside a 3-inch globe.

Beyond the Main Sequence. Click card to see definition. D a very low velocity.

E a very low velocity. A very large radius. These stars must have tiny radii to give off so little energy.

Stars with masses in excess of 50 solar masses are very common. A star that is cool and very luminous must have a. Suppose you observe a previously unknown star and find its apparent magnitude.

B a very small mass. B a very small radius. A cool but very luminous star must have A a very large radius.

The spectral lines of an approaching star are a blueshifted. If mass is added to a white dwarf star a its radius increases b its radius decreases c its density increases d it may exceed the Chandrasekhar limit and collapse e it may produce novae f all of the above. A a very large radius.

A a very large radius. Hot blue stars over 30000 Kelvin at left. The HR Diagram categorizes stars by surface temperature and luminosity.

These stars must have. A star that is cool and very luminous must have a a very great distance. A very small radius.

All stars in the main sequence have the same temperature. A very small radius c.


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