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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. The wavelengths where a specific element can absorb or emit light.
Io (jupiters moon)
Celestial Sphere
Spectral Lines
conjunction
2. The dark - relativley smooth areas on the moon; Latin for sea
Maria
Doppler Shift
Synchrotron Rotation
Electromagnetic Radiation
3. Mercury
Callisto (Jupiter)
Gravitational Lens
Gravitational Lens
smallest diameter
4. A high-pressure bulge in Neptune's southern hemisphere
retrograde motion
great dark spots
Parallax
Open Cluster
5. The area behind a lens where images are resolved
Active Optics
Focal Plane
Spectroscopic Parallax
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
6. The assumption that the universe is isotropic (same in all directions) and homogeneous (Same everywhere throughout)
Disk
cosmological principle
synchronous rotation
Cassegrain Focus
7. The location in the Milky Way where stars orbit like a solid wheel
Hyashi track
contrast northern lowlands and the southern highlands of mars...
Bulge
Maria
8. The law that describes the blackbody curve - and let to quantum mechanics.
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9. The nuclei of very distant galaxies. Likely a manifestation of supermassive black holes
Cassegrain Focus
Quasar
widmanstatten pattern
Convection
10. The trapping of heat by carbon dioxide or other gases in the Earth's atmosphere.
greehouse effects
Void
zone
cosmological principle
11. When the Moon entirely blocks the Sun.
Total Eclipse
Annular Eclipse
Open - flat - and closed.
Sunspot cycle
12. A method of finding a star's distance from its absolute magnitude and spectral type or color.
Hyashi track
Parallax
Spectroscopic Parallax
resonance
13. The number of protons in an atom.
disk
Quasar
Atomic Number
Dark Matter
14. Milky way galaxy is a member - a small poor cluster-about 30 galaxies
coma
Sa spiral galaxy
The Local Group
comet
15. 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)
Lagrangian Razor
Doppler Shift
retrograde motion
White Dwarf
16. A small spherical dark nebula
Bok Globule
Light-Year
Degeneracy
Big Crunch
17. Dying large-mass stars lose their outer layers in a violent explosion creating large - chaotic remnants. these brighten like nova but are so much brighter and only occur ONCE PER STAR
supernova
tectonics of Venus
Light: travels like a wave - detected like a particle
planetary nebula
18. A planet that is farther from the sun than the Earth is
Sc spiral galaxy
Superior planets
cosmological principle
High Velocity Stars
19. The gap inthe outer portion of Saturn's A ring
Open - flat - and closed.
Enke gap
Thickest atmosphere
Extrasolar Planet
20. Arcs of increased mass concentration that slow stars and gas down as they orbit through which cause the formation of stars.
Extrasolar Planet
CCD
density waves
rotation curve=winding dilemma?
21. The Greek philosopher responsible for making the stellar magnitude scale.
Continuous Spectrum
Light Gathering Power
Hipparchus
Astronomical Unit
22. In what chemical form are jupiters nitrogen - carbon and oxygen?
Ammonia - methane - and water
Penumbra
Thermal Equilibrium
Limb darkening
23. If stars have diff orbital periods - than any arms formed by stars will wind into a tight spiral pattern (billion yrs or so)
Photometry
Dark matter candidates
Triple Alpha rocess
rotation curve=winding dilemma?
24. A measure of the force of gravity on an object
Most dense
Meridian
Particle Horizon
weight
25. Cold aggregates of gas - large and contain a huge amount of matter - so cold that molecules stick together to form molecules.
molecular clouds
Ecliptic
gravity
Hubble constant
26. The philosophical stand that says a simpler explanation is more likely to be correct than a complicated one.
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27. The north-south line passing directly overhead through the zenith.
Meridian
Celestial Equator
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.
Nebula
28. How did Earth come to have an oxygen rich atmosphere?
Kuiper belt
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.
Rich vs poor clusters
tectonics of Venus
29. Where is the center of the expansion
radio lobe
Seeing
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.
chondrite
30. Matter that reveals itself only through its gravitational attraction
Black Hole
Dark matter is located at center of clusters - pulling the cluster members into faster orbits--dark matter gravity keeps objects in galxies bound.
Dark Matter
Shepherd satellite
31. Largest moon in solar system - two differenet types of terrain - darker terrain is older - NOT ACTIVE SURFACE
Ganymede (Jupiter)
SETI
Light Curve
Black Hole
32. 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.
zone
cosmic singularity
Horizontal Branch Star
Parallax
33. Centered on the Earth
Geocentric
Callisto (Jupiter)
partile horizon
Seeing
34. The opaque universe that existed for 300000 years after the Big Bang. (photons outnumbered nuclei by 1 billion to one - so less light)
radiation dominated universe
radio galaxy
Chandrasekhar Limit
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 large and bright but cool star.
Zenith
radiation dominated universe
Yes - frozen at the poles- remains protected from the suns rays
Red Giant
36. The location around an atom where an electron resides.
highlands
Spectral Lines
Focal Length
Energy Level
37. The mirror that determines the focus configuration of a reflector
great dark spots
Coldest surface
Secondary Mirror
Shepherd satellite
38. If stars have diff orbital periods - than any arms formed by stars will wind into a tight spiral pattern (billion yrs or so)
Geocentric
Triple Alpha rocess
Dark Matter
rotation curve=winding dilemma?
39. Atmosphere blocks high energy wavelengths - atmosphere blurs optical radiation - atmosphere absorbs some radiation at all wavelengths even when it gets through.
Nova
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.
CCD
3 reasons we orbit satellites to observe universe
40. Then the Sun moves from north to south across the celestial equator (about September 23)
Autumnal Equinox
disk
self-propagating star formation
Plank's Law
41. IO
greatest elongation
Parsec
Geocentric
MOONS: most geologically active
42. The displacement of spectral lines to redder colors caused by the expansion of the universe.
cosmological red shift
widmanstatten pattern
Electromagnetic Radiation
terrestrial planet
43. A crystalline patter found in iron meteorites
nova
Dark matter candidates
widmanstatten pattern
Dark Matter
44. The dimming of starlight by intervening dust
Bok Globule
Summer Solstice
Reflector
Interstellar Extinction
45. The dimming of starlight by intervening dust
Kirchhoff's Law
Jovian Planets
Interstellar Extinction
nova
46. Sudden blasts of gamma radiation from a very distant galaxy caused possibly by a supernova explosion.
Self-Propogating Star Formation
Neutron Star
Gamma ray bursts
Perihelion
47. A plot of star absolute magnitude verses spectral type.
H-are Diagram
Atomic Number
MOONS: roundest shape
nucleus
48. The organized effort to find life elsewhere in the universe. (Search for Extra-Terrestrial Intelligence)
Earth resurfaces itself due to erosion and plate tectonics - while the moon has neither.
SETI
Umbra
opposition
49. How is the Hubble Law consistent with an expanding universe?
Thermonuclear Fusion
planetary nebula
Main Sequence
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.
50. Thick rigid crust - no longer has plate tectonics but still has convective hot spots that create earth-like volcanoes except that last for billions of years because of lack of tectonics.
Cosmological Principle
Eclipses of the Moons of Jupiter
tectonics of Mars
Most dense
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