Quiz 3 Flashcards

(33 cards)

1
Q

Collects first star catalogue, considered the greatest astronomical observer using Babylonian star records and accurate models of the motion of the sun and moon. Developed trigonometry

A

Hipparchus

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2
Q

Assigned magnitude of 1-2 brightest stars (metal plate), and divided visible stars into six magnitude classes

A

Hipparchus making the first determinations of stellar magnitude

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3
Q

System expanded and improved, still the basis of techniques used today

A

Parsons ratio

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4
Q

Observed from earth, negative is brightest

A

Apparent brightness

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5
Q

NGC 224, spiral 2.5m ly away from earth, trillion stars, Milky Way mass. Black hole nuclear 3-5 x 10^7. Moving to MW at 301 km/s. Will collide in 3.75 b years

A

M31 in andromeda

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6
Q

Three parts: disk, nuclear bulge, globular clouds

A

Spiral galaxy

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7
Q

20%, m31, Milky Way, m 33. type of galaxy. Subdivide to barred and regular

A

Spiral galaxy

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8
Q

Type of galaxy, 55%

A

Elliptical

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9
Q

Type of galaxy, 25% Small Magellanic Cloud

A

Irregular

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10
Q

Demonstrated universe was expanding

A

Hubble and humason

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11
Q

Observed the effects of dark matter in galaxy clusters

A

Zwicky

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12
Q

Supply verification of dark tater with galactic rotation curve

A

Vera Rubin and Kent ford

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13
Q

Should decrease as a function of radius but doesn’t

A

Galactic rotation

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14
Q

Additional source of gravity around galaxies that don’t make light. has to be taken into account when determining mass

A

Dark matter

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15
Q

Expanding and accelerating. Led to noble peace prize and the rehabilitation of Einstein’s cosmological constant

A

Universe

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16
Q

Method of categorizing galaxies, elliptical/irregular to spirals. Not evolutionary. Discovered by Hubble

17
Q

Stars and gas orbit in an overall gravitational field, while stars in Ellipticals orbit to maintain shape.

18
Q

Orbit to maintain shape, center has a supermassive black hole. Hot gas

19
Q

Cold gas, supermassive black hole

20
Q

Can help find distances in our galaxy to other galaxies. Bound collections of up to a million stars. Luminous and can be seen at great distances. Medium black hole centers. Very old stars.

A

Globular cluster

21
Q

Uses up hydrogen, shows age

A

Main sequence turn off

22
Q

Used globular clusters to find the size of our galaxy and observed our sun isn’t near the center.

23
Q

Specifies each point on a plane by two coordinates

A

Cartesian coordinate system

24
Q

Distance from the y axis is scaled with the x axis

25
The y coordinate
Ordinate
26
System of gas, dust, stars with their solar systems
Galaxy
27
All points of a moving body moving in the same direction
Translational motion
28
All points of an object circle around an axis
Rotational motion
29
The squares of the orbital periods of the planets are directly proportional to the cubes of the semi major axes of their orbits
Keplers third law
30
Astronomical objects that make up the rungs of the cosmic distance ladder: tool for measuring distances. Made of cepheids
Standard candle
31
Astronomical method for measuring distances to stars. Applied to any main sequence star a spectrum can be recorded for, doesn’t rely on parallax
Spectroscopic parallax
32
First to realize the Milky Way galaxy was larger than believed, took photographs and observed globular clusters, compact spheres composed of many thousands of stars
Harlow Shapley
33
Studied solar eclipses, argued there were galaxies outside the Milky Way. Debated with Shapley over the size of the universe
Heber Curtis