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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. First accurately measured the speed of light in a vacuum
Light Curve
Ole Roemer
Cassegrain Focus
Objective Lens
2. As open clusters age - they push gas away but dust remains this can reflect light giving the cluster a blue-ish color. also called reflection nebula
Planck time
Electromagnetic Radiation: Radio
Doppler Shift
reflection star clusters
3. When one side of a body always faces the planet it revolves around
Emission Spectrum
synchronous rotation
Quasar
supernova
4. Flattened spherical distribution of old stars with some young stars too. 'hub' of Milky way - stars orbit with solid body speeds. Elongated into bar shape
Main Sequence Stars
bulge
chondrite
Cassini division
5. The ratio of the actual density of the universe to the critical density. (actual density divided by the critical density
Roundest orbit
Hydrostatic Equilibrium
density parameter
isotropic
6. Population 1 with higher metals and contain many young stars in star clusters. Distribution of stars is everywhere in disk (arms only have 5% more stars)
synchrotron radiation
Color Index
general star population
Winter Solstice
7. We can infer the absolute magnitude of pulsating variable stars by measuring their pulsation periods. The longer the pulsations - the greater their luminosities. We then again measure their apparent magnitudes - compare it with their absolute magnitu
Cepheid variables
nova
quasar
A family of radiant energy- includes light
8. A particle of light
Annular Eclipse
difference between maria and highlands of the moon.
Photon
Neutron Star
9. The law that syas light energy from a blackbody increases as (temperature^4)
Stephen-Boltzman Law
shape and color of SPIRAL galaxies
Secondary Mirror
open star clusters
10. The process of acquiring material
Cosmic Microwave Background (CMB)
Convection
accretion
Photon
11. The surface of the sun
Oort cloud
Photosphere
Metals
Superior planets
12. A large and bright but cool star.
Light Gathering Power
Red Giant
Galilean satellite
radio lobe
13. A word meaning 'the same in all directions.'
fewest moons
isotropic
regolith
Main Sequence Stars
14. Radiation (possibly left over from the big bang) that fills the universe. Perfect black body spectrum and tells us a bit aout how galaxies are formed.
Red Giant
Cosmic Microwave Background (CMB)
We don't know. It might be but does not have to be.
regolith
15. Electromagnetic Radiation
A family of radiant energy- includes light
direct motion
Molecular Clouds
How is winding dilemma solved?
16. A representation of the changes in color and brightness of an evolving protostar.
Light Pollution
Heliocentric
Hyashi track
radiant
17. A star that is burning hydrogen to helium in a shell surrounding it's core
Continuous Spectrum
Red Giant Branch Star
Sc spiral galaxy
Hubble constant
18. A logarithmically scaled value for the measured brightness of a star.
Apparent Magnitude
shape and color of SPIRAL galaxies
rotation curve=winding dilemma?
evidence of water on mars
19. The act of removing an electron from an atom.
Poor Cluster
Red Giant
Ionization
Colestial Pole
20. The equation that describes how matter equates with energy
Flat - Remain Parallel - Exactly 1
Hipparchus
E=mc2
Cosmic Microwave Background (CMB)
21. The organized effort to find life elsewhere in the universe. (Search for Extra-Terrestrial Intelligence)
Focal Plane
The Big Bang Theory resolves Olber's Paradox
Light Gathering Power
SETI
22. A fusion process in which a carbon atom transmutes to oxygen and back - creating a helium atom in the process
Halo
accretion
Neutron Star
CNO Cycle
23. The surface of the sun
Photosphere
terrestrial planet
Blackbody Curve
highlands
24. Thick rigid crust - no longer has plate tectonics but still has convective hot spots that create earth-like volcanoes except that last for billions of years because of lack of tectonics.
Photometry
molecular clouds
tectonics of Mars
cosmological red shift
25. Mercury
300000 KM/sec
anorthosite
Active Optics
thinnest atmosphere
26. When the Sun is farthest south of the celestial equator (About December 22)
chemical differentiation
Kirchhoff's Law
Lagrangian Razor
Winter Solstice
27. Europa
Degeneracy
2 Reasons Why there are Supermassive Black holes at the center of every Galaxy
reflection star clusters
MOONS: roundest shape
28. Heavier elements such as iron - silicon - magnesium - sulfer - nickel
Plague
Make up of the terrestrial planets
Bulge
cosmic singularity
29. Latin for 'cloud'. A word used to describe the collections of gas and dust in the Milky Way and other galaxies
Nebula
Horizontal Branch Star
matter dominated universe
Ionization
30. Relativity predicts that nothing can travel faster than the speed of light in a vacuum - How can it move slower?
shape and color of SPIRAL galaxies
Refractor
radio galaxy
If it is in a denser medium - such as glass - it will move slower
31. A spherical shell of comets that orbit the sun at a great distance (roughly two light years from the sun)
Vernal Equinox
Nova
Oort cloud
Eclipses of the Moons of Jupiter
32. Distribution of dust (tells us disk is thin) - find distances to O&B stars and H2 regions (arms are sights of star formation and OB stars live and die at location of birth) -Milky way has four arms. Sun is in spur apart from arms.
Proton-proton chain
mapping the structure of Milky Way disk
Synodic Day
Differential Rotation
33. N=are*Fp(Ne)(Fl)(Fi)(Fc)(L) N: number of civilizations possible to communicate with are*: rate solar-like stars are created Fp: fraction of stars with planets Ne: number of planets like ours Fl: fraction of planets with life Fi: intelligent life Fc:
Drake equation
The Big Bang Theory
cosmological red shift
Flat - Flat
34. The force of attraction between any two objects having mass
Continuous Spectrum
gravity
era of recombination
Turn off Point
35. Theory virtually demands that the geometry of the universe be ______. Results of measuring lumps in the cosmic background radiation indicate that the universe geometry is ________.
Electromagnetic Radiation: Infrared
nova
Hyashi track
Flat - Flat
36. An important quality of telescopes that increases as the square of the primary mirror or objective lens
Triple Alpha rocess
Light Gathering Power
Open - flat - and closed.
Focal Plane
37. The distance between a lens and its focal plane
cosmic fireball
Limb darkening
Prominence
Focal Length
38. The science of measuring the apparent magnitudes of stars by imaging them through different filters.
Pulsar
Photometry
nova
anorthosite
39. The cosmological principle is the assumption that the universe is isotropic and homogeneous.The Big Bang assumes it to be a correct principle so that what we observe is exactly like What is too far away to be observed.
Cosmological Principle
Titus-Bode Law
Primary Mirror
Perihelion
40. The time when the universe cooled sufficiently for atoms to exist. radiation dominated= first 300000 years - THEN era of recombination turns into matter dominated for next.
Big Crunch
era of recombination
Occam's razor
Sb spiral galaxy
41. Venus
MOONS: roundest shape
thinnest atmosphere
semimajor axis
Roundest orbit
42. The crust of a meteorite caused by its entry into Earth's atmosphere
Synchrotron Rotation
cosmological principle
Light Curve
fusion crust
43. Extremely round - lots of liquid water - ice rafts on surface ACTIVE SURFACE
rotation curve = dark matter?
hottest surface
Europa (Jupiters moon)
Cepheid variables
44. A word meaning 'the same everywhere throughout.'
Ground State
homogeneous
Electromagnetic Radiation
quasar
45. A subatomic particle with a negative charge. It creates light.
Galilean satellite
MOONS: larger than mercury
Electromagnetic Radiation: Radio
Electron
46. 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
Dark matter is located at center of clusters - pulling the cluster members into faster orbits--dark matter gravity keeps objects in galxies bound.
Sunspots
47. The name for the only seriously considered theory of the universe.
rotation curve = dark matter?
Ganymede (Jupiter)
accretion disk
Big Bang
48. Light-flaky crust - convective currents cause it to wrinkle and bunch (1/5 of surface). uniform cratering suggests lack of weathering and tectonics. volcanoes are flat due to atmospheric pressure.
tectonics of Venus
isotropic
dark energy
Electron
49. A measure of the ability of a telescope to see fine detail
Radio Galaxy
MOONS: largest size
Resolving Power
Penumbra
50. The process similar to conduction by which energy moves from the solar core to the convective layer
quasar
Radiative Diffusion
deferent
Celestial Equator