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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. A term referring to Jupiter-like planets
quasar
belt
jovian
homogeneous
2. The final end state of a high mass star. .An entity for which gravity has completely overwhelmed all other forces of nature.
mare basalt
least dense
Black Hole
Synodic Day
3. 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.
Light Curve
acceleration
H2 Regions
Cosmological Principle
4. Why do Galaxies move very rapidly in the interiors of the dense clusters?
Dark matter is located at center of clusters - pulling the cluster members into faster orbits--dark matter gravity keeps objects in galxies bound.
Horizontal Branch Star
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.
Cosmic Microwave Background (CMB)
5. The shadow behind the Earth or Moon where the Sun is partially obscured.
Cosmic Microwave Background (CMB)
Nova
Penumbra
greehouse effects
6. A change in the wavelength of light caused by a motion between the observer and light (or wave) source (blue shift if getting closer - red shift if moving away)
Red Giant
Total Eclipse
Doppler Shift
Ecliptic
7. An efficient - two-dimensional electronic light detector. Common in digital cameras - they revolutionized astronomical imaging
mare basalt
Resolving Power
jovian
CCD
8. Hot cells of gas that rise and fall in the hotosphere
If it is in a denser medium - such as glass - it will move slower
Seeing
Granules
Cassegrain Focus
9. Mercury
greehouse effects
thinnest atmosphere
Energy Level
Blackbody
10. In a CLOSED UNIVERSE - the curvature of space-time is _________. Parallel beams will converge/diverge/remain parallel (circle one). The density parameter - Ω0 - is _____.
nova
Positive - Converge - Greater than 1
Clouds of sufuric acid (very inhospitable and brightest object in the sky) - process called greenhouse affect traps radiation making it 900 degrees at times - spins with retrograde rotation (sun rises in west) and takes 58.4 days for it to set. Thick
zone
11. An object that may remain after a star explodes
Ionization
Neutron Star
Secondary Mirror
condensation temperature
12. The larger bodies that formed early in teh solar nebula that were chemically differentiated
planetesimal
Gamma ray bursts
Convection
Sunspots
13. A point in the sky where meteors appear to come from during a shower
fusion crust
radiant
Radio Galaxy
slowest rotation
14. Ganymede
MOONS: largest size
bulge
Radiative Diffusion
High Velocity Stars
15. The philosophical stand that says a simpler explanation is more likely to be correct than a complicated one.
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16. The force of attraction between any two objects having mass
Continuous Spectrum
gravity
meteor shower
Quasar
17. In Ptolemy's geocentric solar system - the small circle on which a planet moved.
E=mc2
epicycle
Asymptotic giant Branch Star
Main Sequence Stars
18. A small and dim but hot star.
Blackbody
fusion crust
accretion disk
White Dwarf
19. The era when the ratio of matter to energy greatly favored matter. (verses radiation dominated universe where it was opaque. Matter is now dominated by gravity not photons)
Dark matter is located at center of clusters - pulling the cluster members into faster orbits--dark matter gravity keeps objects in galxies bound.
matter dominated universe
acceleration
fastest rotation
20. A long-lived high-pressure bulge in Jupiter's southern hemisphere
tectonics of Earth
Galilean satellite
Celestial Equator
great red spot
21. The study of the universe as a whole.
A family of radiant energy- includes light
cosmology
greehouse effects
molecular clouds
22. A prominence seen against the disk of the sun
Sidereal Day
Filament
shape and color of ELLIPTICAL galaxies
standard candle
23. Then the Sun moves from north to south across the celestial equator (about September 23)
Reflector
Autumnal Equinox
Vernal Equinox
Oort Cloud
24. The state of having a balance between inward and outard pressures in a gas--the inward force from gravity is balanced by the outward force from heat.
Hydrostatic Equilibrium
3 reasons we orbit satellites to observe universe
High and low pressure which stretch into bands due to the rapid differential rotation. deeper - darker colors are in the belts and zones are lighter
Eyepiece Lens
25. The shadow behind the Earth or Moon where the Sun is partially obscured.
hottest surface
Penumbra
radio galaxy
Most dense
26. A star that blows itself apart
Pixel
Supernova (You can be my supernova girl)
asteroid
Eyepiece Lens
27. 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.
shape and color of ELLIPTICAL galaxies
tectonics of Mars
Geocentric
Brown dwarf
28. The rock that makes up the lunar highlands
anorthosite
Coldest surface
gravity
Superior planets
29. Electromagnetic Radiation
A family of radiant energy- includes light
Ammonia - methane - and water
critical density
Light-Year
30. Centered on the Earth
Geocentric
Eclipses of the Moons of Jupiter
Stephen-Boltzman Law
Plank's Law
31. Hurricane-like vortex in southern-hemisphere winds to north and south blow in opposite directions which keep it spinning and with no subsurface features like mountians it persists.
zone
aphelion
Jupiters red spot
gravity
32. A long-lived high-pressure bulge in Jupiter's southern hemisphere
Black Hole
Zenith
Blackbody
great red spot
33. The instant of time after the Big Bang when space and time obtained their characteristics. (t=10^-43 sec when gravity freezes out-instant when gravity started existing as a separate force)
How is winding dilemma solved?
Ganymede (Jupiter)
tectonics of Mars
Planck time
34. A quantity measuring the stability of the Earth's atmosphere
Sa spiral galaxy
Light-Year
Seeing
Maria
35. 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
Granules
Asymptotic giant Branch Star
Thickest atmosphere
Resolving Power
36. The study of the universe as a whole.
differential rotation
fusion crust
Liquid metallic hydrogen
cosmology
37. Venus
Roundest orbit
thinnest atmosphere
open star clusters
Negative - Diverge - Less than 1
38. 30AU to 50Au from sun - consists of ancietn premordial objects made of frozen ice and dust-35000 objects or more that are larger than 100 km in diameter and many more smaller than this
Blackbody Curve
Kuiper belt
contrast northern lowlands and the southern highlands of mars...
dark energy
39. Form honeycomb like patterns surrounding empty or nearly empty voids.
Bulge
Disk
superclusters
Celestial Equator
40. Population 1- similar to the sun and 2% of elements are metal - Population 2- formed before gas was metal- only a fraction of mass is metal.
hottest surface
3 reasons we orbit satellites to observe universe
Population 1 vs Population 2 stars
Big Bang
41. Matter that reveals itself only through its gravitational attraction
The Big Bang Theory resolves Olber's Paradox
Dark Matter
Positive - Converge - Greater than 1
Eyepiece Lens
42. A large - irregularly shaped rocky object orbiting the sun mostly between mars and jupiter. Left-over planetesimals
asteroid
Parallax
Electromagnetic Radiation
differential rotation
43. Large nebula consisting of very cold gas and dust
Black Hole
greatest elongation
cosmology
Molecular Clouds
44. What is the universe expanding into?
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: Ultraviolet Light
quarks
Hubble constant
45. An empirical scheme for predictin ghe orbital distances of planets
Largest diameter
Limb darkening
Drake equation
Titus-Bode Law
46. The average distance between the Earth and the Sun (=1.5 x10^8km)
Astronomical Unit
Density Wave
radiant
Inverse Square Law
47. A planet that is closer to the sun than the earth
Flat - Remain Parallel - Exactly 1
Dark Nebula
Parsec
inferior planets
48. 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)
Steady State Theory (Leads to Olber's Paradox)
planetary nebula
superclusters
general star population
49. Milky way galaxy is a member - a small poor cluster-about 30 galaxies
Terrestrial Planets
Hubble constant
The Local Group
300000 KM/sec
50. A location on an H-are Diagram where evolving stars pulsate
Extrasolar Planet
Vernal Equinox
fusion crust
Instability strip