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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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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 instant of time after the Big Bang when space and time obtained their characteristics. (t=10^-43 sec when gravity freezes out-instant when gravity started existing as a separate force)
Planck time
Focal Plane
smallest diameter
open star clusters
2. The Greek philosopher responsible for making the stellar magnitude scale.
If it is in a denser medium - such as glass - it will move slower
Dark Nebula
Hipparchus
We don't know. It might be but does not have to be.
3. A spherical shell of comets that orbit the sun at a great distance (roughly two light years from the sun)
semimajor axis
Oort cloud
most eccentric orbit
Terrestrial Planets
4. A term referring to Earth-like planets
terrestrial planet
Positive - Converge - Greater than 1
Hubble law
Grand design spirals
5. The rotation period of the Earth measured relative to the Sun.
Synodic Day
Black Hole
Nucleus
radiation dominated universe
6. All wavelengths of light emitted by a blackbody.
Filament
Secondary Mirror
CNO Cycle
Blackbody Curve
7. 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)
The Big Bang Theory
mare basalt
radio galaxy
H2 Regions
8. 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)
Electromagnetic Radiation
planetary nebula
Flat - Flat
Electromagnetic Radiation
9. The elementary building blocks from which protons and neutrons are formed.
quarks
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.
Cassini division
Main Sequence
10. The apparent path of the Sun through the stars on the celestial sphere.
Apollo asteroids
tectonics of Mars
Ecliptic
fastest rotation
11. The opaque universe that existed for 300000 years after the Big Bang. (photons outnumbered nuclei by 1 billion to one - so less light)
Flat - Flat
Extrasolar Planet
radiation dominated universe
Spectral Lines
12. The distance a moon can be from a planet before shattering from tidal forces
Celestial Equator
roche limit
Main Sequence
Sb spiral galaxy
13. Sulfurous volcanoes - pools of liquid sulfur - surface resembles cheese pizza ACTIVE SURFACE
Coldest surface
Io (jupiters moon)
Galilean satellite
Positive - Converge - Greater than 1
14. The assumption that the universe is isotropic (same in all directions) and homogeneous (Same everywhere throughout)
dark matter
Trojan asteroids
cosmological principle
Parallax
15. The family of radiant energy that includes light as a subset
E=mc2
OB Associations
2 Reasons Why there are Supermassive Black holes at the center of every Galaxy
Electromagnetic Radiation
16. 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)
interstellar dust
How is winding dilemma solved?
rotation curve=winding dilemma?
CCD
17. The science of measuring the apparent magnitudes of stars by imaging them through different filters.
Photometry
Penumbra
Make up of the jovian planets
Ole Roemer
18. 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)
Refractor
Occam's razor
Doppler Shift
radiant
19. Is there water on the moon?
Gravitational Lens
density
aphelion
Yes - frozen at the poles- remains protected from the suns rays
20. Large bulge - tightly wound spiral arms - relatively few h2 regions and are smooth
Chromosphere
Sa spiral galaxy
Stephen-Boltzman Law
Nebula
21. A point in the sky where meteors appear to come from during a shower
aurora
radiant
zone
Perihelion
22. The seasonal shifting of a nearby star's position relative to more distant objects.
Parallax
The Local Group
meteor shower
asteroid
23. A plot of star absolute magnitude verses spectral type.
H-are Diagram
Nucleus
radiation pressure
CMB
24. First accurately measured the speed of light in a vacuum
Density Wave
Bulge
Annular Eclipse
Ole Roemer
25. 1-orbit aroudn the sun 2- are in hydrostatic equilibrium and 'mostly round' 3- have not cleared debris around its orbit 4- are not satellites
Meridian
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.
least dense
Dwarf planets
26. The process responsible for creating the arms of flocculent spiral galaxies
Sunspots
open star clusters
Self-Propogating Star Formation
Supernova (You can be my supernova girl)
27. Extremely round - lots of liquid water - ice rafts on surface ACTIVE SURFACE
meteoriod
Europa (Jupiters moon)
Colestial Pole
era of recombination
28. The movement of the Earth's crustal plates riding on top of the mantle.
HII Region
Granules
Meridian
plate tectonics
29. The point in its orbit where a planet is nearest the sun
Secondary Mirror
Filament
Sc spiral galaxy
Perihelion
30. 10 nm 10^2 nm
Jupiters red spot
Electromagnetic Radiation: X-Ray
Hubble constant
Main Sequence Stars
31. 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
disk
contrast northern lowlands and the southern highlands of mars...
Milky way Galaxy
Cosmic Microwave Background
32. Mercury - Venus - Earth - Mars
Terrestrial Planets
Enke gap
H2 Regions
fusion crust
33. The act of removing an electron from an atom.
Apparent Magnitude
Ionization
Ecliptic
highlands
34. Jupiter
Electromagnetic Radiation: Radio
fastest rotation
self-propagating star formation
Electron
35. Formed rapidly - collapsed slower into disk shape - star birth rate is low but lasts longer and ongoing - contain higher mass blue stars.
molecular clouds
shape and color of SPIRAL galaxies
Photosphere
mare basalt
36. The ratio of the actual density of the universe to the critical density. (actual density divided by the critical density
density parameter
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
Cassini division
Nucleus
37. Collections of young - hot stars
Main Sequence
era of recombination
Nova
OB Associations
38. A particle of light
Electromagnetic Radiation: X-Ray
Photon
Cepheid variables
Synchrotron Rotation
39. The oldest part of the Milky Way
2 Reasons Why there are Supermassive Black holes at the center of every Galaxy
Halo
Corona
Nova
40. 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)
planetary nebula
Instability strip
How is winding dilemma solved?
Interstellar Extinction
41. Ganymede
Chandrasekhar Limit
acceleration
Thermonuclear Fusion
MOONS: largest size
42. Star speed at outer edge of galaxy should begin to diminish - but they dont so we guess that this means there is increasing force (aka dark matter)
Photon
rotation curve = dark matter?
Molecular Clouds
If it is in a denser medium - such as glass - it will move slower
43. Half of the longest diameter across an ellipse
Focal Plane
Flare
Nebula
semimajor axis
44. A spinning neutron star
Electromagnetic Radiation: Radio
Pulsar
Enke gap
belt
45. The organized effort to find life elsewhere in the universe. (Search for Extra-Terrestrial Intelligence)
Annular Eclipse
Light Pollution
Cosmological Principle
SETI
46. Formed from slow rotating clouds - collapsed quicker - initial star formation rate is high but died out - older - little rotation - look redder
Make up of the jovian planets
Refractor
shape and color of ELLIPTICAL galaxies
Dwarf planets
47. A planet that is closer to the sun than the earth
Inverse Square Law
inferior planets
Electromagnetic Radiation
greatest elongation
48. Centered on the sun.
Red Giant
Turn off Point
Heliocentric
Inverse Square Law
49. The distance light travels in one year (=9.46x10^12km).
Oort Cloud
Light-Year
Photon
Apparent Magnitude
50. VENUS
SETI
Extrasolar Planet
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
planetary nebula
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