Astronomy Unit 7 Flashcards

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1
Q

(or nuclear bulge) the central (round) part of the Milky Way or a similar galaxy

A

central bulge

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2
Q

nonluminous mass, whose presence can be inferred only because of its gravitational influence on luminous matter; the composition of the dark matter is not known

A

dark matter

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3
Q

the mass in the Milky Way that extends well beyond the boundary of the luminous stars to a
distance of at least 200,000 light-years from the center of the Galaxy; although we deduce its existence from its gravity, the composition of this matter remains a mystery

A

dark matter halo

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4
Q

the idea that different parts of the Galaxy turn at different rates, since the parts
of the Galaxy follow Kepler’s third law: more distant objects take longer to complete one full orbit around the center of the Galaxy

A

differential galactic rotation

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5
Q

the outermost extent of our Galaxy (or another galaxy), containing a sparse distribution of stars and globular clusters in a more or less spherical distribution

A

halo

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6
Q

the band of light encircling the sky, which is due to the many stars and diffuse nebulae lying
near the plane of the Milky Way Galaxy

A

Milky way galaxy

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7
Q

a star containing heavy elements; typically young and found in the disk

A

population I star

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8
Q

a star with very low abundance of heavy elements; found throughout the Galaxy

A

population II star

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9
Q

a spiral-shaped region, characterized by relatively dense interstellar material and young stars, that
is observed in the disks of spiral galaxies

A

spiral arm

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10
Q

the object in the center of most large galaxies that is so massive and compact that light cannot escape from it; the Milky Way’s supermassive black hole contains 4.6 millions of Suns’ worth of mass

A

supermassive black hole

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11
Q

a galaxy whose shape is an ellipse and that contains no conspicuous interstellar material

A

elliptical galaxy

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12
Q

a constant of proportionality in the law relating the velocities of remote galaxies to their
distances

A

hubble constant

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13
Q

a rule that the radial velocities of remove galaxies are proportional to their distances from us

A

Hubble’s law

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14
Q

a galaxy without any clear symmetry or pattern; neither a spiral nor an elliptical galaxy

A

irregular galaxy

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15
Q

the ratio of the total mass of a galaxy to its total luminosity, usually expressed in units of
solar mass and solar luminosity; the mass-to-light ratio gives a rough indication of the types of stars contained within a galaxy and whether or not substantial quantities of dark matter are present

A

mass-to-light ratio

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16
Q

when lines in the spectra are displaced toward longer wavelengths (toward the red end of the visible spectrum)

A

redshift

17
Q

a flattened, rotating galaxy with pinwheel-like arms of interstellar material and young stars,
winding out from its central bulge

A

spiral galaxy