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Test your basic knowledge |
Cosmology
Start Test
Study First
Subject
:
science
Instructions:
Answer 50 questions in 15 minutes.
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.
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 distance between a lens and its focal plane
density parameter
Focal Length
semimajor axis
greehouse effects
2. 10 cm -> 1 mm
Gamma ray bursts
condensation temperature
Electromagnetic Radiation: Microwave
Convection
3. The shadow behind the Earth or Moon where the Sun is partially obscured.
Heliocentric
Penumbra
Metals
belt
4. The sinking of denser elements to the center of a young molten planet
chemical differentiation
Black Hole
Open Cluster
scarp
5. Where is the center of the expansion
highlands
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.
Light: travels like a wave - detected like a particle
Synchrotron Rotation
6. The process that powers the sun and hydrogen bombs
Sunspots
resonance
Thermonuclear Fusion
Terrestrial Planets
7. The location in the Milky Way where stars orbit like a solid wheel
accretion
Umbra
Bulge
Secondary Mirror
8. The 11 or 22 period on the sun durin which sunspots increase - decrease - change polarity - increase and decrease again.
Coronal Loop
plate tectonics
Sunspot cycle
anorthosite
9. The temp at which a substance in the vacuum of space solidifies
Photosphere
condensation temperature
Disk
Hydrostatic Equilibrium
10. Is there water on the moon?
Rich Cluster
homogeneous
Dwarf planets
Yes - frozen at the poles- remains protected from the suns rays
11. Ancient stream channels - flood planes - and sedimentary-type rock. Frozen water is found in the polar ice caps and in the soil.
Radio Galaxy
evidence of water on mars
Positive - Converge - Greater than 1
Negative - Diverge - Less than 1
12. VENUS
Sidereal Day
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
OB Associations
Apollo asteroids
13. A quantity measuring the stability of the Earth's atmosphere
zone
meteorite
regolith
Seeing
14. The rotation of a star or planet at different speeds at its equator and poles
differential rotation
Europa (Jupiters moon)
Olber's paradox
Secondary Mirror
15. The final end state of a high mass star. .An entity for which gravity has completely overwhelmed all other forces of nature.
Gravitational Lens
Grand design spirals
Vernal Equinox
Black Hole
16. A measure of how an object resists accelerating when acted upon by a force. It is proportional the amount of matter in an object
Main Sequence
mass
Yes - frozen at the poles- remains protected from the suns rays
Callisto (Jupiter)
17. The equation that describes how matter equates with energy
Hipparchus
Refractor
CNO Cycle
E=mc2
18. The law stating that hotter blackbodies look bluer than cooler blackbodies.
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19. Dying small mass stars lose their outer layers in a relatively gentle way - creating a round or bipolar nebula about the star (round like planets)
Cassegrain Focus
Thickest atmosphere
neutrino
planetary nebula
20. A fusion process in which a carbon atom transmutes to oxygen and back - creating a helium atom in the process
Make up of the jovian planets
CNO Cycle
Meridian
contrast northern lowlands and the southern highlands of mars...
21. The organized effort to find life elsewhere in the universe. (Search for Extra-Terrestrial Intelligence)
Quasar
radiation dominated universe
White Dwarf
SETI
22. A force exerted by reflecting sunlight
radiation pressure
Make up of the terrestrial planets
Superior planets
We don't know. It might be but does not have to be.
23. Radiation (possibly left over from the big bang) that fills the universe. Perfect black body spectrum and tells us a bit aout how galaxies are formed.
Blackbody
Rich vs poor clusters
Cosmic Microwave Background (CMB)
Sunspot cycle
24. The dark - relativley smooth areas on the moon; Latin for sea
Maria
contrast northern lowlands and the southern highlands of mars...
Negative - Diverge - Less than 1
Doppler Shift
25. A measure of the seasonal shifting of a star's position against farther stars or galaxies. The closer the star - the greater is the angular distance it shifts. We use it to find distances to stars that are up to 1000 pc away.
Titus-Bode Law
Electromagnetic Radiation
Neutron Star
Parallax
26. A streak of light in the atmosphere
Light Gathering Power
meteor
superclusters
Rich Cluster
27. The rotation period of the Earth measured relative to the Sun.
Synodic Day
deferent
Parallax
comet
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.
tectonics of Venus
Continuous Spectrum
blazar
Cosmic Microwave Background
29. The mirror that gathers the light in a reflector
standard candle
cosmological red shift
zone
Primary Mirror
30. 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
Electromagnetic Radiation: Microwave
Resolving Power
Supercluster
31. A high-pressure bulge in Neptune's southern hemisphere
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.
great dark spots
Disk
radio galaxy
32. 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
Make up of the terrestrial planets
Gravity only pulls matter back together. Therefore - if gravity is the only force that operates on cosmic scales then the expansion of the universe should decrease with time. The critical density is the value of matter density sufficient to halt the
Extrasolar Planet
33. When a planet lines up with the sun inthe sky
radiation dominated universe
Summer Solstice
conjunction
Light: travels like a wave - detected like a particle
34. Old - pock marked - icy surface - interior is not differentiated - geologically dead - NOT ACTIVE SURFACE
Europa (Jupiters moon)
Synodic Day
Supercluster
Callisto (Jupiter)
35. Matter that reveals itself only through its gravitational attraction
Asymptotic giant Branch Star
Dark Matter
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.
Focal Length
36. A very distant - star-like object with huge - broad emission lines. Probably the nucleus of a distant active galaxy.
Callisto (Jupiter)
quasar
Meridian
A family of radiant energy- includes light
37. The Greek philosopher responsible for making the stellar magnitude scale.
Supernova (You can be my supernova girl)
Thickest atmosphere
Hipparchus
Olber's paradox
38. The dimming of starlight by intervening dust
Prominence
The Big Bang Theory
Electromagnetic Radiation: Microwave
Interstellar Extinction
39. Sc galaxies
Flocculent spirals
radio galaxy
chemical differentiation
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.
40. The process responsible for creating the arms of flocculent spiral galaxies
Ecliptic
Positive - Converge - Greater than 1
chondrite
Self-Propogating Star Formation
41. An element of a highly efficient - two-dimensional electronic light detector
Pixel
Yes - frozen at the poles- remains protected from the suns rays
Globular Cluster
interstellar dust
42. A large - irregularly shaped rocky object orbiting the sun mostly between mars and jupiter. Left-over planetesimals
Magnification
asteroid
Ground State
Atomic Number
43. After stars form they pump light energy into surrounding gas causing it to heat up and glow (H2=ionized hydrogen - H1= neutral hydrogen in molcular couds)
H2 Regions
Maria
MOONS: most geologically active
Electromagnetic Radiation
44. The process of acquiring material
Halo
retrograde motion
Apollo asteroids
accretion
45. A prominence seen against the disk of the sun
Celestial Sphere
thinnest atmosphere
Filament
molecular clouds
46. Light-colored high-pressure bands in Jupiter's atmosphere
zone
Parallax
Dark matter candidates
highlands
47. Largest moon in solar system - two differenet types of terrain - darker terrain is older - NOT ACTIVE SURFACE
Ganymede (Jupiter)
mapping the structure of Milky Way disk
Red Giant Branch Star
Nebula
48. Saturn
least dense
most eccentric orbit
A family of radiant energy- includes light
Eyepiece Lens
49. The particle horizon is the farthest we can see. It exists because the universe had a beginning and thus a definite age. Light from distances farther away from the particle horizon have not had time to reach us yet.
Instability strip
Neutron Star
Photon
Particle Horizon
50. A particle of light
Open Cluster
Photon
Big Crunch
partile horizon
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