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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. Venus
Thickest atmosphere
molecular clouds
A family of radiant energy- includes light
Stephen-Boltzman Law
2. The process similar to conduction by which energy moves from the solar core to the convective layer
Oort Cloud
Flare
Radiative Diffusion
Globular Cluster
3. 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.
If it is in a denser medium - such as glass - it will move slower
Cosmic Microwave Background (CMB)
nova
AGN
4. The process that powers the sun and hydrogen bombs
Superior planets
Photosphere
Thermonuclear Fusion
cosmic singularity
5. The north-south line passing directly overhead through the zenith.
The Big Bang Theory resolves Olber's Paradox
Meridian
dark matter
cosmic singularity
6. 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
critical density
Brown dwarf
disk
Neutron Star
7. A term referring to the orbital character of stars near the Sun
Eclipses of the Moons of Jupiter
Nova
slowest rotation
Differential Rotation
8. A star without enough mass to begin hydrogen fusion
Electromagnetic Radiation
Brown dwarf
zone
Coldest surface
9. Neptune or uranus
planetesimal
Terrestrial Planets
Coronal Loop
Coldest surface
10. A logarithmically scaled value for the measured brightness of a star.
Positive - Converge - Greater than 1
Limb darkening
Apparent Magnitude
meteor
11. 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.
mapping the structure of Milky Way disk
Radiative Diffusion
chondrite
nova
12. The science of measuring light energy by wavelength.
Spectroscopy
Positive - Converge - Greater than 1
radiation dominated universe
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
13. 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 ________.
Seyfert galaxy
Flat - Flat
Quasar
cosmological red shift
14. A term referring to Earth-like planets
terrestrial planet
Pixel
synchrotron radiation
Nova
15. A star that erratically and explosively brightens and dims
3 reasons we orbit satellites to observe universe
standard candle
Eyepiece Lens
Nova
16. 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)
Rich Cluster
Doppler Shift
H2 Regions
AGN
17. A very low mass particle formed in solar fusion reactions that reacts only weakly with matter
Cassini division
Open - flat - and closed.
neutrino
Globular Cluster
18. The displacement of spectral lines to redder colors caused by the expansion of the universe.
cosmological red shift
Oort Cloud
synchrotron radiation
Synchrotron Rotation
19. Large bulge - tightly wound spiral arms - relatively few h2 regions and are smooth
Penumbra
Triple Alpha rocess
Density Wave
Sa spiral galaxy
20. The rotation period of the Earth measured relative to the Sun.
shape and color of ELLIPTICAL galaxies
Coronal Loop
Synodic Day
Convection
21. An efficient - two-dimensional electronic light detector. Common in digital cameras - they revolutionized astronomical imaging
Heliocentric
Synodic Day
Supernova (You can be my supernova girl)
CCD
22. The name for the only seriously considered theory of the universe.
Refractor
Sc spiral galaxy
Absorption Spectrum
Big Bang
23. Radiation emitted when charged particles spiral rapidly in a magnetic field. come off of jets from black holes.
Photon
Plague
dark matter
synchrotron radiation
24. The light produced when particles from the sun collide with atmospheric molecules
aurora
Emission Spectrum
density
Chromosphere
25. The final end state of a high mass star. .An entity for which gravity has completely overwhelmed all other forces of nature.
Particle Horizon
Black Hole
Spectroscopy
Steady State Theory (Leads to Olber's Paradox)
26. When particles are compressed to an unnatural state where their pressure is not related to their temperature
tectonics of Venus
Degeneracy
Photosphere
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.
27. What causes the zones and belts on jupiter and saturn?
deferent
Penumbra
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
Negative - Diverge - Less than 1
28. In Ptolemy's geocentric solar system - the small circle on which a planet moved.
greatest elongation
protostar
epicycle
CCD
29. All wavelengths of light emitted by a blackbody.
Red Giant Branch Star
Celestial Sphere
Blackbody Curve
Parallax
30. The process of acquiring material
accretion
force
Absorption Spectrum
Plague
31. Stars orvits do not define the spiral patterns - instead they are density waves that move at slower speeds (arms are defined by young O and B stars and gas clouds)
Dark Nebula
Electromagnetic Radiation
How is winding dilemma solved?
Electron
32. The fate of the universe if it is closed. The universe expanding as much as possible and then retracting
Gravitational Lens
Kirchhoff's Law
Big Crunch
condensation temperature
33. A measure of how an object resists accelerating when acted upon by a force. It is proportional the amount of matter in an object
Make up of the jovian planets
comet
mass
Resolving Power
34. When one side of a body always faces the planet it revolves around
Earth resurfaces itself due to erosion and plate tectonics - while the moon has neither.
synchronous rotation
Flare
Flocculent spirals
35. Collections of young - hot stars
superclusters
OB Associations
standard candle
density waves
36. The high- temperatature outer layer of the sun
Light-Year
Self-Propogating Star Formation
Corona
condensation temperature
37. A perfect absorber and radiator of electromagnetic radiation.
Blackbody
High Velocity Stars
Refractor
Sunspots
38. When the Sun moves from south to north across the celestial equator (about March 21)
Main Sequence
density
smallest diameter
Vernal Equinox
39. Radiation given off by electrons accelerating in a magnetic field
Synchrotron Rotation
inferior planets
Most dense
cosmic fireball
40. The gap etween saturn's A and B rings
Total Eclipse
Cassini division
Cepheid Variable
Light: travels like a wave - detected like a particle
41. 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)
Rich Cluster
general star population
Absolute Magnitude
MOONS: larger than mercury
42. A logarithmically scaled value for the measured brightness of a star.
Doppler Shift
accretion
Apparent Magnitude
Black Hole
43. The source of the force that is accelerating the expansion rate of the universe.
dark energy
Geocentric
CMB
isotropic
44. Matter so dense that even light cannot escape its gravity
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.
Black Hole
comet
slowest rotation
45. 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.
cosmological principle
Blackbody
tectonics of Venus
Hubble constant
46. A prominence seen against the disk of the sun
Filament
MOONS: largest size
density
matter dominated universe
47. Places in the asteroid belt - caused by resonance with Jupiter - where there are no asteroids
We don't know. It might be but does not have to be.
retrograde motion
Kirkwood gaps
disk
48. The rate of expansion of the universe.
highlands
Hubble constant
Earth resurfaces itself due to erosion and plate tectonics - while the moon has neither.
Eclipses of the Moons of Jupiter
49. A quantity measuring the stability of the Earth's atmosphere
least dense
least dense
Seeing
Disk
50. A distance measure determined by the shifting of a star against the background sky every 6 months.
HII Region
Granules
greehouse effects
Parsec