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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. When the Sun is farthest north of the celestial equator (about June 22)
Summer Solstice
Light: travels like a wave - detected like a particle
condensation temperature
Sa spiral galaxy
2. The law stating that hotter blackbodies look bluer than cooler blackbodies.
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3. Poitns of gravitational stability in the orbit of a planet
Dark matter candidates
Thermal Equilibrium
CMB
Lagrangian Razor
4. A rock or iron specimen that has fallen from space
Open Cluster
meteorite
Spectroscopy
CMB
5. The universe is isotropic - homogeneous - and without beginning or end in time and space. If the universe is truly homogeneous then every line of sight will eventually end on a galaxy. If it has existed forever then there has been enough time for lig
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6. Mercury
Earth resurfaces itself due to erosion and plate tectonics - while the moon has neither.
most eccentric orbit
greatest elongation
Metals
7. The distance a moon can be from a planet before shattering from tidal forces
Light Gathering Power
Perihelion
Objective Lens
roche limit
8. Venus (retrograde)
slowest rotation
Electromagnetic Radiation: Ultraviolet Light
Radio Galaxy
HII Region
9. A streak of light in the atmosphere
meteor
Density Wave
Photosphere
Corona
10. A word meaning 'the same in all directions.'
mass
epicycle
isotropic
Roundest orbit
11. The dimming of starlight by intervening dust
Interstellar Extinction
meteor shower
direct motion
Stephen-Boltzman Law
12. Then the Sun moves from north to south across the celestial equator (about September 23)
Largest diameter
Instability strip
Neutron Star
Autumnal Equinox
13. Any class of objects with a uniform luminosity used to determine distance.
Interstellar Extinction
SETI
standard candle
Jovian Planets
14. Radiation given off by electrons accelerating in a magnetic field
fusion crust
Synchrotron Rotation
evidence of water on mars
H-are Diagram
15. The average distance between the Earth and the Sun (=1.5 x10^8km)
rotation curve = dark matter?
blazar
Bok Globule
Astronomical Unit
16. The lens that gathers the light in a refractor
Objective Lens
Limb darkening
Sc spiral galaxy
Spectroscopic parallax
17. A star that is in the process of forming. It glows from gravitational contraction
Big Crunch
homogeneous
Electromagnetic Radiation
protostar
18. Formed from slow rotating clouds - collapsed quicker - initial star formation rate is high but died out - older - little rotation - look redder
Supercluster
aphelion
Callisto (Jupiter)
shape and color of ELLIPTICAL galaxies
19. Infinitely long -> 10 cm
Spectroscopy
Electromagnetic Radiation: Radio
quasar
The Big Bang Theory resolves Olber's Paradox
20. The amount of density needed to stop the universe from expanding and to begin the big crunch represented by Pc
smallest diameter
Photosphere
critical density
Cassini division
21. The lowest energy of an atom.
acceleration
Eclipses of the Moons of Jupiter
Ground State
era of recombination
22. A measure of the ability of a telescope to see fine detail
Spectroscopic Parallax
Steady State Theory (Leads to Olber's Paradox)
self-propagating star formation
Resolving Power
23. Sc galaxies where star formation and destruction is so rapid that supernova explosions are mainly responsible for compressing gas to create new stars.
Stephen-Boltzman Law
self-propagating star formation
Penumbra
Triple Alpha rocess
24. Small bulges - loosely wound - massive arms - arms have many H2 regions and look very lumpy
Maria
Sc spiral galaxy
supernova
synchronous rotation
25. A high-pressure bulge in Neptune's southern hemisphere
Dwarf planets
great dark spots
Trojan asteroids
era of recombination
26. Where is the center of the expansion
Total Eclipse
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.
Absorption Spectrum
Convection
27. A star that is burning hydrogen to helium in a shell surrounding it's core
resonance
Sidereal Day
Cosmic Microwave Background (CMB)
Red Giant Branch Star
28. A word meaning 'the same in all directions.'
Superior planets
isotropic
Thermal Equilibrium
MOONS: roundest shape
29. The oldest terrain on the moon
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.
highlands
Supernova (You can be my supernova girl)
Ecliptic
30. Formed from slow rotating clouds - collapsed quicker - initial star formation rate is high but died out - older - little rotation - look redder
If it is in a denser medium - such as glass - it will move slower
most eccentric orbit
contrast northern lowlands and the southern highlands of mars...
shape and color of ELLIPTICAL galaxies
31. The entity from which the whole universe is postulated to have come from.
isotropic
SETI
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
cosmic singularity
32. An empirical scheme for predictin ghe orbital distances of planets
self-propagating star formation
Oort cloud
Titus-Bode Law
Active Optics
33. 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)
High Velocity Stars
Largest diameter
Doppler Shift
Total Eclipse
34. Formed rapidly - collapsed slower into disk shape - star birth rate is low but lasts longer and ongoing - contain higher mass blue stars.
shape and color of SPIRAL galaxies
difference between maria and highlands of the moon.
inferior planets
fastest rotation
35. Titan
retrograde motion
molecular clouds
MOONS: thickest atmosphere
Molecular Clouds
36. Medium bulge - moderately would arms - arms have H2 regions in them and look sort of lumpy
Sb spiral galaxy
Summer Solstice
Void
Doppler Shift
37. A highly variable galaxy nucleus of which BL Lac is one. Their light is highly energetic and their spectra are featureless. (face on)
meteor
blazar
Rich vs poor clusters
self-propagating star formation
38. Mercury and venus
AGN
thinnest atmosphere
fewest moons
Winter Solstice
39. The powdered stone fragments that make up the lunar 'soil'
interstellar dust
regolith
Black Hole
Maria
40. A cool collection of gas and dust silhouetted against a brighter background of stars and/or gas
Dark Nebula
retrograde motion
great red spot
Light Pollution
41. The organized effort to find life elsewhere in the universe. (Search for Extra-Terrestrial Intelligence)
fewest moons
Liquid metallic hydrogen
Brown dwarf
SETI
42. 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
Maria
High Velocity Stars
Plank's Law
Black Hole
43. In a FLAT UNIVERSE(our universe) - the curvature of space-time is ________. Parallel beams will converge/diverge/remain parallel (circle one). The density parameter - Ω0 - is _____.
Flat - Remain Parallel - Exactly 1
zone
Open Cluster
shape and color of SPIRAL galaxies
44. The point where an inferior planet is as far away from the sun as it can be (as seen from the Earth)
Kuiper belt
greatest elongation
Electromagnetic Radiation: Radio
most moons
45. Ganymede and Titan
superclusters
homogeneous
greatest elongation
MOONS: larger than mercury
46. A location on an H-are Diagram where evolving stars pulsate
blazar
Cosmic Microwave Background (CMB)
Ecliptic
Instability strip
47. In an OPEN UNIVERSE - the curvature of space-time is ____ - Parallel beams will converge/diverge/remain parallel (circle one). The density parameter - Ω0 - is____.
open star clusters
chondrite
greatest elongation
Negative - Diverge - Less than 1
48. The final end state of an intermediate to high mass star. An entity in which all the electrons have been pushed into the protons.
homogeneous
dark energy
Dark matter candidates
Neutron Star
49. Light-colored high-pressure bands in Jupiter's atmosphere
zone
Wein's Law
mapping the structure of Milky Way disk
HII Region
50. Mercury and venus
Umbra
Blackbody
fewest moons
bulge