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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 sinking of denser elements to the center of a young molten planet
Electromagnetic Radiation
inferior planets
Refractor
chemical differentiation
2. When the Sun moves from south to north across the celestial equator (about March 21)
Most dense
Apollo asteroids
regolith
Vernal Equinox
3. The Greek philosopher responsible for making the stellar magnitude scale.
Quasar
era of recombination
Ecliptic
Hipparchus
4. The location in an H-are diagram of a star cluster - where stars have just left the main sequence. Used to estimate the cluster age.
solar nebula
Synodic Day
Doppler Shift
Turn off Point
5. The science of measuring light energy by wavelength.
Thermal Equilibrium
Spectroscopy
Electron
Limb darkening
6. 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)
Spectroscopic Parallax
planetary nebula
Differential Rotation
homogeneous
7. An element of a highly efficient - two-dimensional electronic light detector
Pixel
zone
Refractor
Nucleus
8. The amount of density needed to stop the universe from expanding and to begin the big crunch represented by Pc
density parameter
Cepheid variables
Chandrasekhar Limit
critical density
9. A plot of star absolute magnitude verses spectral type.
Color Index
H-are Diagram
fewest moons
accretion disk
10. The apparent backward motion of a planet against the background of stars.
Electromagnetic Radiation: Radio
retrograde motion
OB Associations
epicycle
11. The point directly overhead.
Parsec
Zenith
accretion
Doppler Shift
12. The assumption that the universe is isotropic (same in all directions) and homogeneous (Same everywhere throughout)
nucleus
Limb darkening
Main Sequence
cosmological principle
13. The north-south line passing directly overhead through the zenith.
Instability strip
great dark spots
Meridian
quasar
14. The place in the sky that the Earth's axis points toward (can be either north or south)
fusion crust
Ammonia - methane - and water
White Dwarf
Colestial Pole
15. Large nebula consisting of very cold gas and dust
Molecular Clouds
Enke gap
homogeneous
Shepherd satellite
16. A bright area of higher temperature that often proceeds the formation of sunspots.
tectonics of Mars
tectonics of Earth
Plague
Planck time
17. Why does the earth have few craters while the moon has many?
Density Wave
Earth resurfaces itself due to erosion and plate tectonics - while the moon has neither.
Bok Globule
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.
18. The nuclei of very distant galaxies. Likely a manifestation of supermassive black holes
rotation curve = dark matter?
Quasar
Electromagnetic Radiation: X-Ray
CNO Cycle
19. The gap etween saturn's A and B rings
Cassini division
rotation curve=winding dilemma?
SETI
most eccentric orbit
20. 100 nm 10 nm
Synodic Day
Maria
Electromagnetic Radiation: Ultraviolet Light
standard candle
21. Largest moon in solar system - two differenet types of terrain - darker terrain is older - NOT ACTIVE SURFACE
H-are Diagram
Grand design spirals
Ganymede (Jupiter)
radiant
22. Star speed at outer edge of galaxy should begin to diminish - but they dont so we guess that this means there is increasing force (aka dark matter)
Liquid metallic hydrogen
supernova
Corona
rotation curve = dark matter?
23. Formed from slow rotating clouds - collapsed quicker - initial star formation rate is high but died out - older - little rotation - look redder
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.
Color Index
superclusters
shape and color of ELLIPTICAL galaxies
24. A star that is burning hydrogen to helium in a shell surrounding it's core
Big Crunch
neutrino
Red Giant Branch Star
cosmological red shift
25. The mirror that gathers the light in a reflector
CNO Cycle
Electromagnetic Radiation
Primary Mirror
Steady State Theory (Leads to Olber's Paradox)
26. The rotation period of the Earth measured relative to the stars.
Ground State
Coronal Loop
A family of radiant energy- includes light
Sidereal Day
27. A streak of light in the atmosphere
Cepheid Variable
meteor
Convection
Big Bang
28. Venus
Thickest atmosphere
Neutron Star
Coronal Loop
isotropic
29. A planet that is farther from the sun than the Earth is
Particle Horizon
Superior planets
Stephen-Boltzman Law
Nova
30. Light scattered through the atmosphere that degrades astronomical images
mapping the structure of Milky Way disk
isotropic
The Big Bang Theory resolves Olber's Paradox
Light Pollution
31. A particle of light
Photon
meteorite
Flat - Remain Parallel - Exactly 1
Nucleus
32. The imaginary sphere centered on the Earth that hols the stars.
radio lobe
semimajor axis
AGN
Celestial Sphere
33. The imaginary sphere centered on the Earth that hols the stars.
How is winding dilemma solved?
force
Degeneracy
Celestial Sphere
34. Population 1- similar to the sun and 2% of elements are metal - Population 2- formed before gas was metal- only a fraction of mass is metal.
Population 1 vs Population 2 stars
gravity
aurora
force
35. Relativity predicts that nothing can travel faster than the speed of light in a vacuum - How can it move slower?
If it is in a denser medium - such as glass - it will move slower
Chromosphere
Spectral Lines
Cosmic Microwave Background
36. The rotation period of the Earth measured relative to the stars.
Summer Solstice
Sidereal Day
Cosmological Principle
Nucleus
37. 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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38. The first rock-sized bodies that formed in the solar nebula from dust grains
chondrite
most moons
radiation pressure
Wein's Law
39. The final end state of a high mass star. .An entity for which gravity has completely overwhelmed all other forces of nature.
Electromagnetic Radiation: Ultraviolet Light
Black Hole
Vernal Equinox
Planetary Nebula
40. First accurately measured the speed of light in a vacuum
condensation temperature
Dark matter candidates
Ole Roemer
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.
41. An empirical scheme for predictin ghe orbital distances of planets
Dark matter candidates
Ole Roemer
Titus-Bode Law
CMB
42. Why do Galaxies move very rapidly in the interiors of the dense clusters?
Dark Matter
Dark matter is located at center of clusters - pulling the cluster members into faster orbits--dark matter gravity keeps objects in galxies bound.
Cosmic Microwave Background
Annular Eclipse
43. N=are*Fp(Ne)(Fl)(Fi)(Fc)(L) N: number of civilizations possible to communicate with are*: rate solar-like stars are created Fp: fraction of stars with planets Ne: number of planets like ours Fl: fraction of planets with life Fi: intelligent life Fc:
CMB
Focal Plane
Planck time
Drake equation
44. The act of removing an electron from an atom.
Maria
belt
H-are Diagram
Ionization
45. The high- temperatature outer layer of the sun
open star clusters
Colestial Pole
tectonics of Venus
Corona
46. The average distance between the Earth and the Sun (=1.5 x10^8km)
planetary nebula
Astronomical Unit
Gamma ray bursts
Cosmological Principle
47. The state of having a balance between inflowing and outflowing heat-- the temp at every radial point is different but constant
Dwarf planets
Thermal Equilibrium
Spectroscopic parallax
Rich Cluster
48. 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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49. The material from which the solar system formed
smallest diameter
Vernal Equinox
Plague
solar nebula
50. Matter so dense that even light cannot escape its gravity
Black Hole
blazar
Gravitational Lens
belt