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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. Old - pock marked - icy surface - interior is not differentiated - geologically dead - NOT ACTIVE SURFACE
meteoriod
semimajor axis
Callisto (Jupiter)
Granules
2. Cold aggregates of gas - large and contain a huge amount of matter - so cold that molecules stick together to form molecules.
Corona
epicycle
molecular clouds
open star clusters
3. Rich= dense crowded cores of galaxies - poor= few members and a looser organization of galaxies
Rich vs poor clusters
tectonics of Venus
Electron
Total Eclipse
4. The wavelengths where a specific element can absorb or emit light.
Cassini division
Spectral Lines
Focal Plane
jovian
5. Either Io -Europa - Ganymede - or Callisto
Gamma-ray Burst
Galilean satellite
greatest elongation
Ground State
6. The distance a moon can be from a planet before shattering from tidal forces
general star population
roche limit
Granules
Self-Propogating Star Formation
7. A method of finding a star's distance from its absolute magnitude and spectral type or color.
Spectroscopic Parallax
Ammonia - methane - and water
Grand design spirals
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.
8. Small bulges - loosely wound - massive arms - arms have many H2 regions and look very lumpy
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.
Make up of the jovian planets
Sc spiral galaxy
Vernal Equinox
9. Clouds of low density gas often found glowing faintly on either side of an AGN.
terrestrial planet
radio lobe
Electromagnetic Radiation
Celestial Sphere
10. What are the three possible geometries of the universe?
Open - flat - and closed.
Rich vs poor clusters
Eclipses of the Moons of Jupiter
Kuiper belt
11. Small bulges - loosely wound - massive arms - arms have many H2 regions and look very lumpy
Light Pollution
MOONS: roundest shape
Sc spiral galaxy
CCD
12. An element of a highly efficient - two-dimensional electronic light detector
Kirchhoff's Law
Pixel
most eccentric orbit
gravity
13. Mercury
Resolving Power
most eccentric orbit
Annular Eclipse
Focal Length
14. The elementary building blocks from which protons and neutrons are formed.
quarks
Make up of the terrestrial planets
meteoriod
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.
15. All wavelengths of light emitted by a blackbody.
Earth resurfaces itself due to erosion and plate tectonics - while the moon has neither.
Active Optics
Cepheid variables
Blackbody Curve
16. 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.
chondrite
Black Hole
Flat - Flat
Particle Horizon
17. A streak of light in the atmosphere
Cepheid Variable
Spectral Lines
meteor
Self-Propogating Star Formation
18. The science of measuring the apparent magnitudes of stars by imaging them through different filters.
synchronous rotation
fastest rotation
general star population
Photometry
19. 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)
cosmology
Electromagnetic Radiation
Doppler Shift
Filament
20. The gap etween saturn's A and B rings
cosmic fireball
Cassini division
standard candle
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.
21. Electromagnetic Radiation
Sidereal Day
Kirchhoff's Law
A family of radiant energy- includes light
Yes - frozen at the poles- remains protected from the suns rays
22. What do we think the actual fate of the universe will be and why do we think this?
inferior planets
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.
Main Sequence Stars
Yes - frozen at the poles- remains protected from the suns rays
23. The trapping of heat by carbon dioxide or other gases in the Earth's atmosphere.
smallest diameter
Occam's razor
greehouse effects
Stephen-Boltzman Law
24. 100 nm 10 nm
Electromagnetic Radiation: Ultraviolet Light
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.
Flat - Flat
gravity
25. The lowest energy of an atom.
Black Hole
Ground State
density waves
highlands
26. The shadow behind the Earth or Moon where the Sun is partially obscured.
shape and color of ELLIPTICAL galaxies
Penumbra
retrograde motion
Colestial Pole
27. 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.
Particle Horizon
Gamma-ray Burst
Cassegrain Focus
Trojan asteroids
28. Norhern lowlands- darker in color and have far fewer craters as if an ancient sea or ice field covered them. southern highlands- much higher in density of craters.
Sc spiral galaxy
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
contrast northern lowlands and the southern highlands of mars...
Make up of the jovian planets
29. The most mass a white dwarf can have before collapsing to a neutron star
Winter Solstice
Chandrasekhar Limit
greehouse effects
Hubble constant
30. Mercury
Plank's Law
smallest diameter
Inverse Square Law
fastest rotation
31. Matter that reveals itself only through its gravitational attraction.
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.
dark matter
Molecular Clouds
fusion crust
32. Latin for 'cloud'. A word used to describe the collections of gas and dust in the Milky Way and other galaxies
cosmological red shift
Nebula
Olber's paradox
The Local Group
33. The light produced when particles from the sun collide with atmospheric molecules
terrestrial planet
aurora
most eccentric orbit
3 reasons we orbit satellites to observe universe
34. A collection of galaxies like the one the Milky Way belongs to
Celestial Equator
Electromagnetic Radiation
Autumnal Equinox
Poor Cluster
35. A measure of the force of gravity on an object
weight
Electromagnetic Radiation
Celestial Equator
Open Cluster
36. A repeated - periodic push or pull capable of summing into a larger push or pull
Maria
Eyepiece Lens
resonance
Continuous Spectrum
37. The trapping of heat by carbon dioxide or other gases in the Earth's atmosphere.
The Local Group
Parsec
greehouse effects
Density Wave
38. What is the universe expanding into?
Maria
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.
Convection
Synchrotron Rotation
39. What Ole Roemer used to measure the speed of light in a vacuum
radiation pressure
conjunction
Maria
Eclipses of the Moons of Jupiter
40. Material that shoots rapidly out into space. Flares cause Auroras
Flare
accretion
Geocentric
Flat - Remain Parallel - Exactly 1
41. An important quality of telescopes that increases as the square of the primary mirror or objective lens
CNO Cycle
Light Gathering Power
bulge
Spectroscopic Parallax
42. A continuous spectrum of light missing energy at a few wave lengths.
gravity
great dark spots
Absorption Spectrum
Eclipses of the Moons of Jupiter
43. In an OPEN UNIVERSE - the curvature of space-time is ____ - Parallel beams will converge/diverge/remain parallel (circle one). The density parameter - Ω0 - is____.
Steady State Theory (Leads to Olber's Paradox)
Kuiper belt
Negative - Diverge - Less than 1
great red spot
44. The point directly overhead.
Zenith
Electromagnetic Radiation: Ultraviolet Light
Quasar
radio galaxy
45. The process responsible for creating the arms of flocculent spiral galaxies
opposition
Self-Propogating Star Formation
Autumnal Equinox
Neutron Star
46. The philosophical stand that says a simpler explanation is more likely to be correct than a complicated one.
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47. A star fusing hydrogen to helium in it's core
Asymptotic giant Branch Star
Main Sequence Stars
Eyepiece Lens
acceleration
48. An important quality of telescopes that increases as the square of the primary mirror or objective lens
Light Gathering Power
Hubble law
regolith
Chandrasekhar Limit
49. Half of the longest diameter across an ellipse
weight
MOONS: largest size
Plague
semimajor axis
50. The layer of the sun just above the photosphere
accretion
MOONS: largest size
Chromosphere
Electromagnetic Radiation: Visible Light