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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 movement of the Earth's crustal plates riding on top of the mantle.
Kuiper belt
Open - flat - and closed.
plate tectonics
zone
2. The nuclei of very distant galaxies. Likely a manifestation of supermassive black holes
Io (jupiters moon)
Quasar
Color Index
Globular Cluster
3. The line on an H-are diagram going from upper left to lower right where normal stars of different masses reside.
Main Sequence
highlands
Color Index
rotation curve=winding dilemma?
4. Jupiter
Largest diameter
MOONS: thickest atmosphere
belt
fusion crust
5. A measure of how an object resists accelerating when acted upon by a force. It is proportional the amount of matter in an object
Maria
mass
great dark spots
Differential Rotation
6. A point in the sky where meteors appear to come from during a shower
Jupiters red spot
radiant
Ganymede (Jupiter)
widmanstatten pattern
7. The law that predicts the possible types of spectra.
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8. Latin for 'cloud'. A word used to describe the collections of gas and dust in the Milky Way and other galaxies
Degeneracy
Cassegrain Focus
Neutron Star
Nebula
9. The dimming of starlight by intervening dust
Granules
inferior planets
Interstellar Extinction
Objective Lens
10. The projection of the Earth's equator onto the celestial sphere.
Celestial Equator
greatest elongation
critical density
radiant
11. When the Moon entirely blocks the Sun.
Total Eclipse
Synodic Day
great red spot
Hubble constant
12. A method of finding a star's distance from its absolute magnitude and spectral type or color.
Photon
Spectroscopic Parallax
Ionization
plate tectonics
13. Population 1 with higher metals and contain many young stars in star clusters. Distribution of stars is everywhere in disk (arms only have 5% more stars)
Poor Cluster
general star population
Photosphere
Granules
14. When the Sun is farthest south of the celestial equator (About December 22)
3 reasons we orbit satellites to observe universe
Wein's Law
Winter Solstice
Parallax
15. Half of the longest diameter across an ellipse
semimajor axis
Cosmic Microwave Background
Io (jupiters moon)
Magnification
16. The line on an H-are diagram going from upper left to lower right where normal stars of different masses reside.
Main Sequence
Photometry
Vernal Equinox
Light Pollution
17. In what chemical form are jupiters nitrogen - carbon and oxygen?
Ammonia - methane - and water
Wein's Law
meteoriod
difference between maria and highlands of the moon.
18. A volume of space where few - if any - galaxies are located
MOONS: thickest atmosphere
greatest elongation
radio lobe
Void
19. Largest moon in solar system - two differenet types of terrain - darker terrain is older - NOT ACTIVE SURFACE
OB Associations
Absorption Spectrum
Molecular Clouds
Ganymede (Jupiter)
20. Large bulge - tightly wound spiral arms - relatively few h2 regions and are smooth
Sa spiral galaxy
Cosmic Microwave Background (CMB)
Neutron Star
bulge
21. A perfect absorber and radiator of electromagnetic radiation.
self-propagating star formation
Trojan asteroids
We don't know. It might be but does not have to be.
Blackbody
22. 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
Ammonia - methane - and water
radio galaxy
Positive - Converge - Greater than 1
23. 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)
MOONS: most geologically active
Asymptotic giant Branch Star
Planck time
Limb darkening
24. A star that blows itself apart
Stephen-Boltzman Law
Supernova (You can be my supernova girl)
Precession
epicycle
25. The distance between a lens and its focal plane
Focal Length
Cosmological Principle
Supernova (You can be my supernova girl)
accretion
26. 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)
Chromosphere
H2 Regions
meteorite
contrast northern lowlands and the southern highlands of mars...
27. The mix of pure photon energy that emerged at the start of the universe.
cosmic fireball
comet
plate tectonics
Cosmic Microwave Background
28. Places in the asteroid belt - caused by resonance with Jupiter - where there are no asteroids
Superior planets
inferior planets
quarks
Kirkwood gaps
29. The amount of density needed to stop the universe from expanding and to begin the big crunch represented by Pc
mare basalt
Kirkwood gaps
E=mc2
critical density
30. 10^2 nm 10^7 nm
Electromagnetic Radiation: Gamma Ray
Lagrangian Razor
Apparent Magnitude
Neutron Star
31. A telescope that uses mirrors to focus light
meteor shower
CMB
Reflector
Red Giant
32. Why do Galaxies move very rapidly in the interiors of the dense clusters?
Hubble law
Electromagnetic Radiation: Ultraviolet Light
Hubble law
Dark matter is located at center of clusters - pulling the cluster members into faster orbits--dark matter gravity keeps objects in galxies bound.
33. The process of acquiring material
semimajor axis
Dwarf planets
accretion
Callisto (Jupiter)
34. The temp at which a substance in the vacuum of space solidifies
Rich Cluster
epicycle
scarp
condensation temperature
35. A word used in astronomy to describe all elements besides hydrogen and helium
Metals
Roundest orbit
Primary Mirror
Callisto (Jupiter)
36. An empirical scheme for predictin ghe orbital distances of planets
asteroid
Density Wave
Meridian
Titus-Bode Law
37. An important quality of telescopes that increases as the square of the primary mirror or objective lens
Kuiper belt
Light Gathering Power
meteoriod
Turn off Point
38. The number of protons in an atom.
Hubble constant
radiation dominated universe
Atomic Number
Spectral Lines
39. 1μm 100 nm
terrestrial planet
Apparent Magnitude
Terrestrial Planets
Electromagnetic Radiation: Visible Light
40. Hot cells of gas that rise and fall in the hotosphere
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.
Granules
Hubble constant
If it is in a denser medium - such as glass - it will move slower
41. Mercury
Synodic Day
smallest diameter
dark energy
Bulge
42. The gap etween saturn's A and B rings
Focal Plane
Cassini division
Hydrostatic Equilibrium
Most dense
43. Earth
Photon
Most dense
general star population
Plank's Law
44. A planet orbiting about a distant star
Spectral Lines
Make up of the terrestrial planets
Sb spiral galaxy
Extrasolar Planet
45. When massive objects bend space and time enough to create multiple images of an object located behind them
Gravitational Lens
The Big Bang Theory resolves Olber's Paradox
mare basalt
Void
46. A particle of light
Summer Solstice
Photon
Light Pollution
resonance
47. Light scattered through the atmosphere that degrades astronomical images
quasar
Wein's Law
planetesimal
Light Pollution
48. When material is heated and moves taking the heat energy with it
greatest elongation
Liquid metallic hydrogen
Convection
Oort cloud
49. A measure of the force of gravity on an object
weight
Bok Globule
Refractor
Umbra
50. Matter that reveals itself only through its gravitational attraction
fewest moons
molecular clouds
Secondary Mirror
Dark Matter
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