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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 push or a pull
mare basalt
Penumbra
comet
force
2. Largest moon in solar system - two differenet types of terrain - darker terrain is older - NOT ACTIVE SURFACE
Thermonuclear Fusion
300000 KM/sec
Ganymede (Jupiter)
Planck time
3. Orbit in Jupiters orbit
differential rotation
Nowhere visible to us. If there are higher dimension then the center would be visible to someone who lives in one. If there are no higher dimensions then the center does not exist.
great red spot
Trojan asteroids
4. A phenomenon seen when the Earth passes through the orbit of a burned out comet
condensation temperature
Celestial Sphere
E=mc2
meteor shower
5. A representation of the changes in color and brightness of an evolving protostar.
Spectral Lines
Hyashi track
Parallax
zone
6. 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
Kuiper belt
Nebula
Gamma ray bursts
partile horizon
7. Highlands: rocks are made of lighter anorthosite (similar to old earth rocks) Maria: rocks made of heavy mare basalt (volcanic rock) everywhere else is loose regolith created by meteoric impact.
Synchrotron Rotation
Black Hole
Population 1 vs Population 2 stars
difference between maria and highlands of the moon.
8. Why do Galaxies move very rapidly in the interiors of the dense clusters?
Trojan asteroids
Molecular Clouds
Dark matter is located at center of clusters - pulling the cluster members into faster orbits--dark matter gravity keeps objects in galxies bound.
Oort Cloud
9. 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:
mass
Hipparchus
quasar
Drake equation
10. 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)
blazar
matter dominated universe
Extrasolar Planet
chemical differentiation
11. An evolved star - past the helium flash that is burning helium to carbon in it's cores
Celestial Equator
Horizontal Branch Star
Sunspot cycle
Neutron Star
12. Sa - Sb galaxies where two magnificent arms wind their way from nucleus out in a symmetrical manner.
Grand design spirals
H2 Regions
Chromosphere
tectonics of Earth
13. The apparent path of the Sun through the stars on the celestial sphere.
direct motion
Electron
Thermonuclear Fusion
Ecliptic
14. Form honeycomb like patterns surrounding empty or nearly empty voids.
shape and color of ELLIPTICAL galaxies
Photon
superclusters
anorthosite
15. A subatomic particle with a negative charge. It creates light.
Cepheid variables
Electron
Absorption Spectrum
Ionization
16. 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)
Corona
The Big Bang Theory resolves Olber's Paradox
Thermal Equilibrium
general star population
17. 1 mm 1μm
A family of radiant energy- includes light
Electromagnetic Radiation: Infrared
Nowhere visible to us. If there are higher dimension then the center would be visible to someone who lives in one. If there are no higher dimensions then the center does not exist.
comet
18. 100 nm 10 nm
Electromagnetic Radiation: Ultraviolet Light
asteroid
Gravitational Lens
great red spot
19. The force of attraction between any two objects having mass
Make up of the jovian planets
Planck time
gravity
great dark spots
20. A highly variable galaxy nucleus of which BL Lac is one. Their light is highly energetic and their spectra are featureless. (face on)
accretion disk
blazar
CCD
Hubble law
21. The fusion process that turns three helium nuclei into a carbon nucleus
Ground State
Apollo asteroids
Jovian Planets
Triple Alpha rocess
22. The powdered stone fragments that make up the lunar 'soil'
Prominence
deferent
regolith
blazar
23. The oldest part of the Milky Way
planetary nebula
Halo
Planetary Nebula
Magnification
24. A nearby galaxy with a quasar-like nucleus. closer but less bright than quasars-weaker
Seyfert galaxy
density waves
most moons
radio galaxy
25. The mix of pure photon energy that emerged at the start of the universe.
cosmic fireball
greatest elongation
Flat - Flat
Largest diameter
26. When the Sun moves from south to north across the celestial equator (about March 21)
Seeing
Drake equation
Plague
Vernal Equinox
27. An energetic event taking place in the early universe
Most dense
Nebula
Gamma-ray Burst
Kuiper belt
28. Matter that reveals itself only through its gravitational attraction.
Gamma-ray Burst
Sa spiral galaxy
dark matter
fusion crust
29. A planet that is closer to the sun than the earth
Continuous Spectrum
Electromagnetic Radiation: Ultraviolet Light
Sc spiral galaxy
inferior planets
30. A fusion process in which a carbon atom transmutes to oxygen and back - creating a helium atom in the process
open star clusters
density waves
Drake equation
CNO Cycle
31. A cloud of ionized hydrogen. Formed when young stars heat the surrounding gas
HII Region
Seeing
Electromagnetic Radiation: Radio
accretion disk
32. A large - irregularly shaped rocky object orbiting the sun mostly between mars and jupiter. Left-over planetesimals
asteroid
Penumbra
Turn off Point
Thermonuclear Fusion
33. A bridge of material held in position above the solar surface. They can remain for hours even days
300000 KM/sec
matter dominated universe
Prominence
Terrestrial Planets
34. What causes the zones and belts on jupiter and saturn?
Synchrotron Rotation
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
Light: travels like a wave - detected like a particle
Dark matter is located at center of clusters - pulling the cluster members into faster orbits--dark matter gravity keeps objects in galxies bound.
35. A prominence seen against the disk of the sun
cosmological red shift
comet
Spectroscopic parallax
Filament
36. Flat disk with gas - dust - H2 regions - molecular clouds - dust young stars and remnants of old planetary nebula and supernova remnants. stars spin together with similar velocities called differential rotation
Most dense
most eccentric orbit
disk
Heliocentric
37. Small bulges - loosely wound - massive arms - arms have many H2 regions and look very lumpy
Occam's razor
Focal Length
highlands
Sc spiral galaxy
38. 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
Cassini division
Annular Eclipse
MOONS: larger than mercury
39. A star without enough mass to begin hydrogen fusion
Brown dwarf
Cepheid Variable
Wein's Law
Largest diameter
40. The law that syas light energy from a blackbody increases as (temperature^4)
Europa (Jupiters moon)
Gamma ray bursts
Stephen-Boltzman Law
Energy Level
41. Highlands: rocks are made of lighter anorthosite (similar to old earth rocks) Maria: rocks made of heavy mare basalt (volcanic rock) everywhere else is loose regolith created by meteoric impact.
radio galaxy
AGN
Perihelion
difference between maria and highlands of the moon.
42. When the Moon entirely blocks the Sun.
Total Eclipse
Flat - Remain Parallel - Exactly 1
MOONS: roundest shape
Extrasolar Planet
43. 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
Hubble law
Hydrostatic Equilibrium
mare basalt
Magnification
44. The name for the only seriously considered theory of the universe.
Big Bang
Asymptotic giant Branch Star
Spectroscopic parallax
Void
45. 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)
Biologicla life created the recycling of nitrogen - co2 - and the production of oxygen. Oxygen is heavier so the atmosphere held onto it easier than hydrogen and helium.
Doppler Shift
retrograde motion
rotation curve=winding dilemma?
46. An element of a highly efficient - two-dimensional electronic light detector
Pixel
Steady State Theory (Leads to Olber's Paradox)
MOONS: thickest atmosphere
Spectral Lines
47. Distance from sun to nucleus- 8 kiloparsecs (26000 LY) - diameter of Milky way- 150000 LY - length for sun to orbit once around milky way- 250 million years
aphelion
Milky way Galaxy
accretion disk
Kirchhoff's Law
48. A planet that is farther from the sun than the Earth is
Cassegrain Focus
Energy Level
Superior planets
Red Giant
49. The assumption that the universe is isotropic (same in all directions) and homogeneous (Same everywhere throughout)
Main Sequence Stars
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
cosmological principle
Galilean satellite
50. A change in the appearance of the sun at the edge of the solar disk
Limb darkening
Electromagnetic Radiation: Radio
Spectroscopy
radiation dominated universe