Astronomy unit 7 practice test

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V

Main-sequence stars are all designated by luminosity class _____.

parsec

a unit of distance equal to 3.0857 × 1013 km

pulsar

A _____ is a neutron star that emits narrow beams of energy as it spins on its axis.

binary star

A _____ is two stars orbiting a common center of gravity.

visual binary

A _____ is when both stars in a system can be seen separately through a telescope.

long-term variable

A red variable is a _____ star that is a red giant or supergiant.

helium

A star leaves the main sequence when it stops fusing hydrogen into _____ in its core.

nova

A(n) _____ is a star that suddenly flares up, then fades after a few weeks or months.

light

Almost everything we know about stars comes to us through careful analysis of the _____ they emit.

iron

Formation of _____ marks the end of a blue star's life because it cannot be fused into another element.

lower right

Stars toward the _____ of the main sequence fuse hydrogen at a slower rate because they have less internal nuclear activity.

hydrogen-helium

The _____ cycle process ends with the production of helium-4.

carbon

The _____ cycle/process begins and ends with the same element.

triple-alpha

The _____ cycle/process only occurs in really hot stars.

Hydrostatic equilibrium

_____ is a term describing fluids at rest.

Apparent magnitude

_____ is how bright a star looks in our sky.

Singularity

_____ is the point where gravity compresses an object to infinite density and to almost no volume.

Absolute magnitude

_____ measures the total energy output of a star.

Bright-line

_____ spectra indicate the presence of specific elements and confirm the heat necessary to vaporize them.

Dark-line

_____ spectra indicate the presence of specific elements because those elements absorb white light.

helium flash

occurs after helium begins to fuse with carbon in the triple-alpha process

Big Scrunch

occurs when a star's iron heart suddenly compresses its mass in tenths of a second from stellar death

Enjar Hertzsprung

plotted the absolute magnitude of individual stars within clusters against their colors

Henry Russell

plotted the absolute magnitude of stars against their spectral classes

giants and supergiants

plotted to the upper right on the H-R diagram

lattice

As a white dwarf cools, the carbon and oxygen ions lock themselves into a crystal _____, or three-dimensional pattern of atoms.

slit

The _____ permits light only from a selected source.

Our Sun is a G2 yellow star of above-average size.

Which of the following sentences best describes our Sun?

Mass

_____ dictates what characteristics a star shows throughout all stages of its activity.

White dwarfs

_____ do not shrink further because their electrons cannot get any closer together.

Pulsars

_____ spin rapidly because they are governed by the spin rate of their original star being concentrated into a drastically shrunken condition.

H-R Diagram

a chart of the absolute magnitudes of stars plotted against their temperatures

isotope

a form of an element having the same number of protons, but having more or fewer than the usual number of neutrons

black hole or neutron star

a form of degenerate matter that can occur after a star explodes

light year

approximately 9,460,000,000,000 km

luminoity

indicated by adding a Roman numeral to the letter and number that designates a star's class

Joseph von Fraunhofer

invented the spectroscope

convection

keeps helium from accumulating in the core of a red dwarf

main-sequence

the center curving line in the H-R diagram

logarithm

the exponent to which a base must be raised to produce a given number


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