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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 imaginary sphere centered on the Earth that hols the stars.
Celestial Sphere
general star population
radiation dominated universe
H2 Regions
2. When the Sun moves from south to north across the celestial equator (about March 21)
Vernal Equinox
Sunspots
Instability strip
Positive - Converge - Greater than 1
3. 1μm 100 nm
Gamma ray bursts
era of recombination
Big Bang
Electromagnetic Radiation: Visible Light
4. A streak of light in the atmosphere
Supernova (You can be my supernova girl)
meteor
Geocentric
Synodic Day
5. A toroidal or donut-shaped collection of material attracted to a central body like a star or black hole. Dust around an object
Most dense
retrograde motion
quasar
accretion disk
6. Medium bulge - moderately would arms - arms have H2 regions in them and look sort of lumpy
homogeneous
Cosmological Principle
Sb spiral galaxy
Superior planets
7. Sc galaxies where star formation and destruction is so rapid that supernova explosions are mainly responsible for compressing gas to create new stars.
self-propagating star formation
direct motion
meteor shower
retrograde motion
8. In Ptolemy's geocentric solar system - the small circle on which a planet moved.
Cepheid Variable
Objective Lens
epicycle
Stephen-Boltzman Law
9. Venus (retrograde)
Supernova (You can be my supernova girl)
shape and color of ELLIPTICAL galaxies
slowest rotation
isotropic
10. The location around an atom where an electron resides.
Convection
Energy Level
Sc spiral galaxy
Ganymede (Jupiter)
11. Cold aggregates of gas - large and contain a huge amount of matter - so cold that molecules stick together to form molecules.
Sidereal Day
molecular clouds
Ecliptic
meteor shower
12. The oldest grouping of stars - found in the galaxy halo
Globular Cluster
High Velocity Stars
cosmological red shift
quarks
13. The rock that makes up the lunar highlands
Blackbody
Supernova (You can be my supernova girl)
anorthosite
Pulsar
14. The most mass a white dwarf can have before collapsing to a neutron star
Inverse Square Law
Chandrasekhar Limit
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.
general star population
15. A particle of light.
Bulge
Refractor
Photon
cosmic singularity
16. Jupiter - Saturn - Uranus - Neptune
general star population
cosmic singularity
neutrino
Jovian Planets
17. In an OPEN UNIVERSE - the curvature of space-time is ____ - Parallel beams will converge/diverge/remain parallel (circle one). The density parameter - Ω0 - is____.
Negative - Diverge - Less than 1
Emission Spectrum
MOONS: thickest atmosphere
Shepherd satellite
18. 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
Reflector
Grand design spirals
Cepheid variables
E=mc2
19. Dying large-mass stars lose their outer layers in a violent explosion creating large - chaotic remnants. these brighten like nova but are so much brighter and only occur ONCE PER STAR
Light Pollution
Red Giant
cosmological principle
supernova
20. 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)
Parallax
Black Hole
Pixel
general star population
21. Ganymede and Titan
slowest rotation
quasar
least dense
MOONS: larger than mercury
22. A small round distribution of gas surrounding a dying star
tectonics of Venus
Planetary Nebula
Electromagnetic Radiation
tectonics of Mars
23. Form honeycomb like patterns surrounding empty or nearly empty voids.
Thermonuclear Fusion
Coronal Loop
tectonics of Earth
superclusters
24. When material is heated and moves taking the heat energy with it
greehouse effects
Convection
Cassegrain Focus
Winter Solstice
25. Relativity predicts that nothing can travel faster than the speed of light in a vacuum - How can it move slower?
Main Sequence
If it is in a denser medium - such as glass - it will move slower
Limb darkening
Annular Eclipse
26. The 'edge' of the universe. Light beyond this has not reached us yet.
aphelion
partile horizon
synchronous rotation
solar nebula
27. The faint glow of light left over from the Big Bang. cosmic microwave background are the photons that remain after the big bang that have not turned into matter.
CMB
Continuous Spectrum
zone
Bulge
28. 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.
Electromagnetic Radiation
tectonics of Venus
The Big Bang Theory
Jovian Planets
29. Poitns of gravitational stability in the orbit of a planet
Light Curve
tectonics of Mars
Magnification
Lagrangian Razor
30. 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
Light-Year
reflection star clusters
Hipparchus
Metals
31. 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.
We don't know. It might be but does not have to be.
Grand design spirals
Thermal Equilibrium
era of recombination
32. The crust of a meteorite caused by its entry into Earth's atmosphere
Olber's paradox
fusion crust
tectonics of Venus
The Local Group
33. The equation that describes how matter equates with energy
Chandrasekhar Limit
neutrino
Cassegrain Focus
E=mc2
34. A star fusing hydrogen to helium in it's core
Particle Horizon
accretion
Main Sequence Stars
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.
35. Jupiter
widmanstatten pattern
density parameter
Gamma ray bursts
most moons
36. Titan
Supernova (You can be my supernova girl)
MOONS: thickest atmosphere
E=mc2
Parallax
37. A younger cluster of stars - found in the galaxy disk
Open Cluster
Photon
Neutron Star
most moons
38. 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
reflection star clusters
Make up of the terrestrial planets
3 reasons we orbit satellites to observe universe
Pulsar
39. Places in the asteroid belt - caused by resonance with Jupiter - where there are no asteroids
Sidereal Day
Energy Level
fusion crust
Kirkwood gaps
40. The oldest part of the Milky Way
acceleration
Halo
Steady State Theory (Leads to Olber's Paradox)
Electromagnetic Radiation: Ultraviolet Light
41. 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
Degeneracy
Ammonia - methane - and water
Coronal Loop
42. A huge sphere of tenuous gas surrounding the nucleus of a comet
Photosphere
coma
epicycle
Light Pollution
43. 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)
Umbra
general star population
difference between maria and highlands of the moon.
Color Index
44. A crystalline patter found in iron meteorites
shape and color of SPIRAL galaxies
Superior planets
widmanstatten pattern
CMB
45. Earth
Grand design spirals
Rich vs poor clusters
Most dense
Electromagnetic Radiation: Microwave
46. An entity that is likely in the nucleus of most - if not all - galaxies.
Granules
Synodic Day
supermassive black hole
Superior planets
47. When massive objects bend space and time enough to create multiple images of an object located behind them
Gravitational Lens
Perihelion
Heliocentric
differential rotation
48. The rotation period of the Earth measured relative to the Sun.
Shepherd satellite
terrestrial planet
Synodic Day
radiant
49. The assumption that the universe is isotropic (same in all directions) and homogeneous (Same everywhere throughout)
cosmological principle
Coldest surface
chondrite
OB Associations
50. The displacement of spectral lines to redder colors caused by the expansion of the universe.
deferent
aurora
Big Bang
cosmological red shift