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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. We can infer the absolute magnitude of pulsating variable stars by measuring their pulsation periods. The longer the pulsations - the greater their luminosities. We then again measure their apparent magnitudes - compare it with their absolute magnitu
H-are Diagram
Astronomical Unit
Photon
Cepheid variables
2. Places in the asteroid belt - caused by resonance with Jupiter - where there are no asteroids
Absolute Magnitude
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.
great red spot
Kirkwood gaps
3. As open clusters age - they push gas away but dust remains this can reflect light giving the cluster a blue-ish color. also called reflection nebula
Kuiper belt
reflection star clusters
Kuiper belt
tectonics of Mars
4. The rock that makes up the lunar highlands
Precession
anorthosite
HII Region
Radiative Diffusion
5. Hurricane-like vortex in southern-hemisphere winds to north and south blow in opposite directions which keep it spinning and with no subsurface features like mountians it persists.
partile horizon
matter dominated universe
Jupiters red spot
Negative - Diverge - Less than 1
6. Mercury
Molecular Clouds
smallest diameter
mare basalt
CMB
7. A distance measure determined by the shifting of a star against the background sky every 6 months.
Energy Level
Parsec
scarp
tectonics of Venus
8. Relativity predicts that nothing can travel faster than the speed of light in a vacuum - How can it move slower?
Differential Rotation
If it is in a denser medium - such as glass - it will move slower
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
rotation curve = dark matter?
9. The philosophical stand that says a simpler explanation is more likely to be correct than a complicated one.
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10. The point directly overhead.
Electromagnetic Radiation: Microwave
Galilean satellite
Zenith
evidence of water on mars
11. The source of the force that is accelerating the expansion rate of the universe.
dark energy
Energy Level
Plague
radio galaxy
12. A two-filter measure of the color - and hence temperature - of a star.
Apollo asteroids
Color Index
Bok Globule
Plague
13. The 'edge' of the universe. Light beyond this has not reached us yet.
radiant
Spectroscopy
partile horizon
Molecular Clouds
14. The dark - relativley smooth areas on the moon; Latin for sea
fusion crust
Maria
belt
radiant
15. Small moons that maintain the shape of rings around Saturn and Uranus
Shepherd satellite
weight
Spectroscopy
acceleration
16. The number of protons in an atom.
MOONS: larger than mercury
accretion
Atomic Number
Flare
17. The point where a superior planet is as far away from the sun as it can be (as seen from the Earth)
Photometry
Sa spiral galaxy
Wein's Law
opposition
18. A small round distribution of gas surrounding a dying star
Quasar
Electromagnetic Radiation: Visible Light
Apollo asteroids
Planetary Nebula
19. A galaxy emitting large amounts of energy at long wavelengths.
Titus-Bode Law
Rich Cluster
radio galaxy
Heliocentric
20. A toroidal or donut-shaped collection of material attracted to a central body like a star or black hole. Dust around an object
Halo
Focal Length
accretion disk
Planetary Nebula
21. Centered on the sun.
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.
cosmological red shift
Heliocentric
Vernal Equinox
22. A rock or iron specimen that has fallen from space
meteorite
Chromosphere
Rich Cluster
greatest elongation
23. The area behind a lens where images are resolved
Wein's Law
Focal Plane
homogeneous
Electromagnetic Radiation: Radio
24. The light produced when particles from the sun collide with atmospheric molecules
Absorption Spectrum
aurora
AGN
hottest surface
25. What do we think the actual fate of the universe will be and why do we think this?
planetary nebula
Europa (Jupiters moon)
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.
interstellar dust
26. Large nebula consisting of very cold gas and dust
How is winding dilemma solved?
Eyepiece Lens
Blackbody Curve
Molecular Clouds
27. Venus
Roundest orbit
Energy Level
Metals
Europa (Jupiters moon)
28. Either Io -Europa - Ganymede - or Callisto
Galilean satellite
epicycle
Cassegrain Focus
Hubble constant
29. A term referring to Jupiter-like planets
jovian
Photosphere
thinnest atmosphere
Sb spiral galaxy
30. A term referring to the orbital character of stars near the Sun
radio lobe
Differential Rotation
Dwarf planets
Population 1 vs Population 2 stars
31. Titan
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
Cosmic Microwave Background
MOONS: thickest atmosphere
Superior planets
32. The apparent backward motion of a planet against the background of stars.
Total Eclipse
Halo
Asymptotic giant Branch Star
retrograde motion
33. Largest moon in solar system - two differenet types of terrain - darker terrain is older - NOT ACTIVE SURFACE
Make up of the terrestrial planets
Ganymede (Jupiter)
conjunction
Plank's Law
34. The first rock-sized bodies that formed in the solar nebula from dust grains
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.
fewest moons
chondrite
Instability strip
35. Massive compact halo objects (MACHO) - weakly interacting massive particles (WIMPY's)
Sc spiral galaxy
Electromagnetic Radiation
Dark matter candidates
meteoriod
36. The surface of the sun
Pulsar
Photosphere
Synodic Day
Electromagnetic Radiation
37. The era when the ratio of matter to energy greatly favored matter. (verses radiation dominated universe where it was opaque. Matter is now dominated by gravity not photons)
Oort Cloud
Main Sequence
matter dominated universe
Secondary Mirror
38. The north-south line passing directly overhead through the zenith.
Meridian
Sidereal Day
Titus-Bode Law
Yes - frozen at the poles- remains protected from the suns rays
39. When a planet lines up with the sun inthe sky
gravity
nucleus
conjunction
Thermal Equilibrium
40. The amount of density needed to stop the universe from expanding and to begin the big crunch represented by Pc
critical density
tectonics of Earth
Main Sequence Stars
Photon
41. The rotation period of the Earth measured relative to the Sun.
Sunspots
Synodic Day
evidence of water on mars
quasar
42. What is the universe expanding into?
mapping the structure of Milky Way disk
Drake equation
Negative - Diverge - Less than 1
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.
43. An entity that is likely in the nucleus of most - if not all - galaxies.
Prominence
conjunction
supermassive black hole
Coronal Loop
44. The powdered stone fragments that make up the lunar 'soil'
density waves
deferent
Total Eclipse
regolith
45. The opaque universe that existed for 300000 years after the Big Bang. (photons outnumbered nuclei by 1 billion to one - so less light)
Black Hole
radio galaxy
radiation dominated universe
contrast northern lowlands and the southern highlands of mars...
46. Stars fromt he Halo that have drifted into the disk. as earth zooms past them in a faster orbit they appear to be going backward very fast
High Velocity Stars
Eyepiece Lens
Absorption Spectrum
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.
47. The shadow behind the Earth or Moon where the Sun is partially obscured.
conjunction
Cosmic Microwave Background (CMB)
Penumbra
greehouse effects
48. The mirror that gathers the light in a reflector
Spectral Lines
tectonics of Venus
Oort cloud
Primary Mirror
49. A high-pressure bulge in Neptune's southern hemisphere
Light Pollution
great dark spots
gravity
We don't know. It might be but does not have to be.
50. 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)
tectonics of Earth
Vernal Equinox
Spectral Lines
planetary nebula