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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. Galaxies whose nuclei emit jets of materil at high speeds. material comes from supermassive black holes
great red spot
radio galaxy
Electromagnetic Radiation: Radio
shape and color of ELLIPTICAL galaxies
2. A measure of the force of gravity on an object
Seeing
weight
radio galaxy
jovian
3. A point in the sky where meteors appear to come from during a shower
AGN
radiant
solar nebula
coma
4. The movement of the Earth's crustal plates riding on top of the mantle.
Astronomical Unit
Synchrotron Rotation
plate tectonics
Photosphere
5. Mercury - Venus - Earth - Mars
Terrestrial Planets
reflection star clusters
open star clusters
Nebula
6. The imaginary sphere centered on the Earth that hols the stars.
Dark Matter
Celestial Sphere
dark matter
synchrotron radiation
7. The Big Bang says that the universe has not existed forever. It had a distinct beginning about 14 billion years ago called the 'Big Bang'. Therefore light from any object more than 14 billion light years away has not had time to reach us. The other p
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8. Small moons that maintain the shape of rings around Saturn and Uranus
Flare
Rich vs poor clusters
Umbra
Shepherd satellite
9. A continuous spectrum of light missing energy at a few wave lengths.
Flare
Electromagnetic Radiation: Infrared
Absorption Spectrum
quasar
10. 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
Flat - Flat
Titus-Bode Law
Celestial Sphere
11. A push or a pull
Poor Cluster
force
3 reasons we orbit satellites to observe universe
Cosmic Microwave Background
12. An element of a highly efficient - two-dimensional electronic light detector
Pixel
self-propagating star formation
High Velocity Stars
nova
13. 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
scarp
2 Reasons Why there are Supermassive Black holes at the center of every Galaxy
dark energy
14. The force of attraction between any two objects having mass
Bulge
gravity
quasar
radiation dominated universe
15. A telescope that uses mirrors to focus light
Ionization
Reflector
If it is in a denser medium - such as glass - it will move slower
great dark spots
16. A galaxy emitting large amounts of energy at long wavelengths.
synchronous rotation
zone
radio galaxy
Photosphere
17. Cold aggregates of gas - large and contain a huge amount of matter - so cold that molecules stick together to form molecules.
molecular clouds
Coldest surface
radiant
Jupiters red spot
18. The area behind a lens where images are resolved
Focal Plane
Blackbody Curve
cosmological principle
Main Sequence
19. A very distant - star-like object with huge - broad emission lines. Probably the nucleus of a distant active galaxy.
Grand design spirals
quasar
Observations of distant type Ia supernovae indicate that the expansion of the universe is speeding up with time - not slowing down! So there must be a force causing this.
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.
20. Any class of objects with a uniform luminosity used to determine distance.
meteorite
standard candle
Coronal Loop
Refractor
21. 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.
Flocculent spirals
High Velocity Stars
Big Crunch
Coronal Loop
22. 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
Hubble constant
Summer Solstice
disk
Perihelion
23. The state of having a balance between inflowing and outflowing heat-- the temp at every radial point is different but constant
Turn off Point
Thermal Equilibrium
Main Sequence Stars
Penumbra
24. Collections of young - hot stars
OB Associations
Reflector
Dark Nebula
Neutron Star
25. The organization of clusters of galaxies into sheets and strings
Bulge
chemical differentiation
Instability strip
Supercluster
26. Sudden blasts of gamma radiation from a very distant galaxy caused possibly by a supernova explosion.
Cosmic Microwave Background
Hyashi track
Gamma ray bursts
radio galaxy
27. The fate of the universe if it is closed. The universe expanding as much as possible and then retracting
Big Crunch
Winter Solstice
fastest rotation
MOONS: larger than mercury
28. A quantity measuring the stability of the Earth's atmosphere
Rich Cluster
Focal Length
conjunction
Seeing
29. Ganymede and Titan
cosmic singularity
Neutron Star
belt
MOONS: larger than mercury
30. The family of radiant energy that includes light as a subset
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.
Cosmic Microwave Background
density
Electromagnetic Radiation
31. The rotation period of the Earth measured relative to the Sun.
standard candle
most eccentric orbit
Synodic Day
Refractor
32. Saying that the sky should not get dark at night because all lines of sight end on a star meaning that the night sky should be ablaze BUT the big bang - because the universe had a beginning - says that the sky gets dark because out in space - galaxie
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33. Hydrogen and helium (mainly)
meteoriod
Make up of the jovian planets
dark matter
Heliocentric
34. Moon in less than the angular diameter of the Sun.
Annular Eclipse
Quasar
matter dominated universe
accretion
35. The process similar to conduction by which energy moves from the solar core to the convective layer
synchrotron radiation
Kirchhoff's Law
Electromagnetic Radiation: Gamma Ray
Radiative Diffusion
36. The trapping of heat by carbon dioxide or other gases in the Earth's atmosphere.
OB Associations
nova
nova
greehouse effects
37. Places in the asteroid belt - caused by resonance with Jupiter - where there are no asteroids
Kirkwood gaps
HII Region
Particle Horizon
Thickest atmosphere
38. A very low mass particle formed in solar fusion reactions that reacts only weakly with matter
neutrino
MOONS: larger than mercury
meteorite
terrestrial planet
39. Originially thought to be stars emitting radio radiation but are now concluded to be nuclei of distant galaxies (same as radio galaxies aka emit streams of material)
CMB
quasar
Coronal Loop
Absorption Spectrum
40. 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
Electromagnetic Radiation
Annular Eclipse
Thickest atmosphere
41. The science of measuring the apparent magnitudes of stars by imaging them through different filters.
difference between maria and highlands of the moon.
Poor Cluster
Photometry
Focal Plane
42. A very dense - highly populated cluster of galaxies
Trojan asteroids
Rich Cluster
evidence of water on mars
synchronous rotation
43. In what chemical form are jupiters nitrogen - carbon and oxygen?
Ammonia - methane - and water
H-are Diagram
Molecular Clouds
The Local Group
44. 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
Extrasolar Planet
Differential Rotation
disk
Meridian
45. Small moons that maintain the shape of rings around Saturn and Uranus
White Dwarf
Absorption Spectrum
reflection star clusters
Shepherd satellite
46. Disk dust grains are made of all the elements that are not in gaseous form in space which blocks starlight and causes interstellar extinction
Ionization
Vernal Equinox
3 reasons we orbit satellites to observe universe
interstellar dust
47. 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)
Absorption Spectrum
Thermal Equilibrium
Doppler Shift
cosmic fireball
48. The lowest energy of an atom.
Ground State
Cosmic Microwave Background
Colestial Pole
Superior planets
49. The oldest part of the Milky Way
Globular Cluster
Light-Year
molecular clouds
Halo
50. A nearby galaxy with a quasar-like nucleus. closer but less bright than quasars-weaker
Cassegrain Focus
Particle Horizon
Seyfert galaxy
Earth resurfaces itself due to erosion and plate tectonics - while the moon has neither.