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Test your basic knowledge |
Cosmology
Start Test
Study First
Subject
:
science
Instructions:
Answer 50 questions in 15 minutes.
If you are not ready to take this test, you can
study here
.
Match each statement with the correct term.
Don't refresh. All questions and answers are randomly picked and ordered every time you load a test.
This is a study tool. The 3 wrong answers for each question are randomly chosen from answers to other questions. So, you might find at times the answers obvious, but you will see it re-enforces your understanding as you take the test each time.
1. The distance between a lens and its focal plane
Kuiper belt
Focal Length
Zenith
Refractor
2. Finding a star's absolute magnitude from it's placement on an HR diagram. After finding the absolute magnitude - we measure the apparent magnitude - for a distance modulus and use this to find the distance. This method is good for finding distances t
Cosmic Microwave Background
fewest moons
Focal Plane
Spectroscopic parallax
3. Sulfurous volcanoes - pools of liquid sulfur - surface resembles cheese pizza ACTIVE SURFACE
rotation curve = dark matter?
Thickest atmosphere
Io (jupiters moon)
Absorption Spectrum
4. When the Sun is farthest south of the celestial equator (About December 22)
difference between maria and highlands of the moon.
Kirchhoff's Law
Winter Solstice
gravity
5. Orbit in Jupiters orbit
Trojan asteroids
Coldest surface
Asymptotic giant Branch Star
Photon
6. A repeated - periodic push or pull capable of summing into a larger push or pull
Hydrostatic Equilibrium
How is winding dilemma solved?
Flat - Flat
resonance
7. A particle of light.
If it is in a denser medium - such as glass - it will move slower
Photon
Radiative Diffusion
difference between maria and highlands of the moon.
8. Jupiter
Drake equation
radiation pressure
Hyashi track
Largest diameter
9. A push or a pull
Maria
force
slowest rotation
Autumnal Equinox
10. A measure of how an object resists accelerating when acted upon by a force. It is proportional the amount of matter in an object
mass
Gravity only pulls matter back together. Therefore - if gravity is the only force that operates on cosmic scales then the expansion of the universe should decrease with time. The critical density is the value of matter density sufficient to halt the
The Local Group
Sidereal Day
11. The projection of the Earth's equator onto the celestial sphere.
Celestial Equator
mass
plate tectonics
molecular clouds
12. If stars have diff orbital periods - than any arms formed by stars will wind into a tight spiral pattern (billion yrs or so)
Void
Geocentric
rotation curve=winding dilemma?
Particle Horizon
13. How is the Hubble Law consistent with an expanding universe?
Black Hole
In an expanding universe all galaxies see all other galaxies that are not gravitationally bound to them receding away. This is what we see in the Hubble Law. We infer that the Hubble law also holds true for all other galaxies.
accretion disk
A family of radiant energy- includes light
14. A fusion process in which protons build together to form helium
Umbra
Photon
acceleration
Proton-proton chain
15. Loops that trace the magnetic field as it erupts from a sunspot area and arches over to an adjacent area. They glow in the light of gas pouring out of corona and falling into photosphere.
Sidereal Day
Autumnal Equinox
Cosmological Principle
Coronal Loop
16. A collection of comets in the plane of the solar system - located beyond the orbit of Pluto
planetesimal
Sidereal Day
Kuiper belt
radiation pressure
17. Dying small mass stars lose their outer layers in a relatively gentle way - creating a round or bipolar nebula about the star (round like planets)
synchronous rotation
Extrasolar Planet
Earth resurfaces itself due to erosion and plate tectonics - while the moon has neither.
planetary nebula
18. The opaque universe that existed for 300000 years after the Big Bang. (photons outnumbered nuclei by 1 billion to one - so less light)
Photon
Void
radiation dominated universe
The Big Bang Theory resolves Olber's Paradox
19. Moon in less than the angular diameter of the Sun.
Annular Eclipse
accretion disk
supermassive black hole
Ecliptic
20. Any change in the speed or direction of an object's motion
Continuous Spectrum
acceleration
superclusters
Cosmic Microwave Background
21. Sudden blasts of gamma radiation from a very distant galaxy caused possibly by a supernova explosion.
supermassive black hole
Gamma ray bursts
planetary nebula
protostar
22. A star that has become a red giant for the second and final time. It is burning helium to carbon in a shell surrounding the core
Flocculent spirals
Sb spiral galaxy
Asymptotic giant Branch Star
Planetary Nebula
23. An important quality of telescopes that increases as the square of the primary mirror or objective lens
fusion crust
Light Gathering Power
Corona
Observations of distant type Ia supernovae indicate that the expansion of the universe is speeding up with time - not slowing down! So there must be a force causing this.
24. The fate of the universe if it is closed. The universe expanding as much as possible and then retracting
Enke gap
Pulsar
Geocentric
Big Crunch
25. Electromagnetic Radiation
A family of radiant energy- includes light
radiation pressure
MOONS: largest size
disk
26. Approximate speed of light in a vacuum
300000 KM/sec
resonance
open star clusters
Filament
27. A term referring to Earth-like planets
partile horizon
solar nebula
synchrotron radiation
terrestrial planet
28. The linear correlation between the rate of the expansion of the universe and distance. Says that as galaxies get farther away in space - the speed with which they recede from us increases. So we can measure the amount of recessional velocity and use
quarks
matter dominated universe
Black Hole
Hubble law
29. What do we think the actual fate of the universe will be and why do we think this?
Hipparchus
Observations of distant type Ia supernovae indicate that the expansion of the universe is speeding up with time - not slowing down! So there must be a force causing this.
self-propagating star formation
Shepherd satellite
30. The entity from which the whole universe is postulated to have come from.
cosmic singularity
Eclipses of the Moons of Jupiter
cosmic fireball
Gamma-ray Burst
31. The movement of the Earth's crustal plates riding on top of the mantle.
Grand design spirals
shape and color of SPIRAL galaxies
plate tectonics
Seyfert galaxy
32. A streak of light in the atmosphere
meteor
Disk
Proton-proton chain
Galilean satellite
33. The larger bodies that formed early in teh solar nebula that were chemically differentiated
planetesimal
Oort Cloud
Particle Horizon
Flat - Remain Parallel - Exactly 1
34. Relativity predicts that nothing can travel faster than the speed of light in a vacuum - How can it move slower?
Resolving Power
rotation curve = dark matter?
If it is in a denser medium - such as glass - it will move slower
Open - flat - and closed.
35. The point in its orbit where a planet is farthest from the sun
Electromagnetic Radiation: Microwave
Inverse Square Law
aphelion
Cosmic Microwave Background
36. The name for the only seriously considered theory of the universe.
Particle Horizon
Big Bang
Supernova (You can be my supernova girl)
radio galaxy
37. A spinning neutron star
greatest elongation
Electromagnetic Radiation: Microwave
Pulsar
Hubble law
38. Old - pock marked - icy surface - interior is not differentiated - geologically dead - NOT ACTIVE SURFACE
Seeing
Parallax
Occam's razor
Callisto (Jupiter)
39. Small compact stars called white dwarfs can have material deposited on their surfaces. In time material heats up and explodes in surface nuclear reaction- star brightens - settles - repeats.
Thickest atmosphere
nova
Umbra
rotation curve = dark matter?
40. Extremely round - lots of liquid water - ice rafts on surface ACTIVE SURFACE
Extrasolar Planet
Particle Horizon
Europa (Jupiters moon)
condensation temperature
41. In an OPEN UNIVERSE - the curvature of space-time is ____ - Parallel beams will converge/diverge/remain parallel (circle one). The density parameter - Ω0 - is____.
Electromagnetic Radiation: X-Ray
Negative - Diverge - Less than 1
fastest rotation
Density Wave
42. The layer of the sun just above the photosphere
Chromosphere
Cepheid variables
White Dwarf
direct motion
43. The location of a supermassive black hole
cosmology
3 reasons we orbit satellites to observe universe
Nucleus
greatest elongation
44. A word meaning 'the same everywhere throughout.'
It does not have to expand into anything. It might just be that the 3 dimensions of space are getting bigger. It may also be that our 3 spatial dimensions are expanding into higher dimensions if such things exist.
Electromagnetic Radiation: X-Ray
force
homogeneous
45. The force of attraction between any two objects having mass
radio galaxy
gravity
Black Hole
Electromagnetic Radiation: X-Ray
46. Clouds of low density gas often found glowing faintly on either side of an AGN.
mare basalt
Globular Cluster
radio lobe
Granules
47. The entity responsible for spiral arms in grand-design spiral galaxies
Density Wave
smallest diameter
cosmological principle
Planck time
48. Norhern lowlands- darker in color and have far fewer craters as if an ancient sea or ice field covered them. southern highlands- much higher in density of craters.
contrast northern lowlands and the southern highlands of mars...
Zenith
Instability strip
greehouse effects
49. In Ptolemy's geocentric solar system - the small circle on which a planet moved.
epicycle
thinnest atmosphere
Apollo asteroids
Void
50. A quantity measuring the stability of the Earth's atmosphere
Dark Nebula
mare basalt
Seeing
Seyfert galaxy