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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. First accurately measured the speed of light in a vacuum
Metals
Zenith
Red Giant
Ole Roemer
2. Highlands: rocks are made of lighter anorthosite (similar to old earth rocks) Maria: rocks made of heavy mare basalt (volcanic rock) everywhere else is loose regolith created by meteoric impact.
anorthosite
radio galaxy
synchrotron radiation
difference between maria and highlands of the moon.
3. Massive compact halo objects (MACHO) - weakly interacting massive particles (WIMPY's)
plate tectonics
Dark matter candidates
Inverse Square Law
Superior planets
4. The larger bodies that formed early in teh solar nebula that were chemically differentiated
Resolving Power
Sa spiral galaxy
force
planetesimal
5. The ratio of the actual density of the universe to the critical density. (actual density divided by the critical density
Planck time
Occam's razor
Geocentric
density parameter
6. An element of a highly efficient - two-dimensional electronic light detector
Resolving Power
Pixel
superclusters
planetary nebula
7. Then the Sun moves from north to south across the celestial equator (about September 23)
Autumnal Equinox
Molecular Clouds
Extrasolar Planet
self-propagating star formation
8. When the Sun is farthest north of the celestial equator (about June 22)
Focal Length
great red spot
Summer Solstice
AGN
9. Sudden blasts of gamma radiation from a very distant galaxy caused possibly by a supernova explosion.
Gamma ray bursts
Thickest atmosphere
terrestrial planet
Electromagnetic Radiation: Ultraviolet Light
10. A measure of the seasonal shifting of a star's position against farther stars or galaxies. The closer the star - the greater is the angular distance it shifts. We use it to find distances to stars that are up to 1000 pc away.
Doppler Shift
Parallax
Planetary Nebula
plate tectonics
11. In a CLOSED UNIVERSE - the curvature of space-time is _________. Parallel beams will converge/diverge/remain parallel (circle one). The density parameter - Ω0 - is _____.
Corona
Electromagnetic Radiation: Gamma Ray
Dark Matter
Positive - Converge - Greater than 1
12. Medium bulge - moderately would arms - arms have H2 regions in them and look sort of lumpy
Red Giant Branch Star
Refractor
Photon
Sb spiral galaxy
13. 100 nm 10 nm
Precession
era of recombination
Dark Nebula
Electromagnetic Radiation: Ultraviolet Light
14. When massive objects bend space and time enough to create multiple images of an object located behind them
cosmology
Degeneracy
Gravitational Lens
aurora
15. 1μm 100 nm
Precession
Electromagnetic Radiation: Visible Light
Electromagnetic Radiation
evidence of water on mars
16. The science of measuring light energy by wavelength.
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
Photon
Spectroscopy
disk
17. When the Sun is farthest south of the celestial equator (About December 22)
Most dense
Globular Cluster
Winter Solstice
plate tectonics
18. An important quality of telescopes that increases as the square of the primary mirror or objective lens
Light Gathering Power
Total Eclipse
Black Hole
standard candle
19. The layer of the sun just above the photosphere
aphelion
synchrotron radiation
Filament
Chromosphere
20. A rock or iron specimen that has fallen from space
meteorite
Electromagnetic Radiation: Visible Light
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.
molecular clouds
21. A collection of comets in the plane of the solar system - located beyond the orbit of Pluto
dark matter
dark energy
Electromagnetic Radiation: Radio
Kuiper belt
22. 1 mm 1μm
Electromagnetic Radiation: Infrared
Apparent Magnitude
Eclipses of the Moons of Jupiter
Jupiters red spot
23. Venus
Rich vs poor clusters
standard candle
quarks
Roundest orbit
24. The nuclei of very distant galaxies. Likely a manifestation of supermassive black holes
Spectroscopy
Cosmic Microwave Background (CMB)
Quasar
thinnest atmosphere
25. The state of having a balance between inward and outard pressures in a gas--the inward force from gravity is balanced by the outward force from heat.
least dense
Gravitational Lens
critical density
Hydrostatic Equilibrium
26. 10 nm 10^2 nm
epicycle
smallest diameter
Electromagnetic Radiation: X-Ray
Self-Propogating Star Formation
27. The process similar to conduction by which energy moves from the solar core to the convective layer
Interstellar Extinction
Proton-proton chain
Olber's paradox
Radiative Diffusion
28. Cold aggregates of gas - large and contain a huge amount of matter - so cold that molecules stick together to form molecules.
Dark matter is located at center of clusters - pulling the cluster members into faster orbits--dark matter gravity keeps objects in galxies bound.
cosmological principle
molecular clouds
Electromagnetic Radiation: Gamma Ray
29. A cool collection of gas and dust silhouetted against a brighter background of stars and/or gas
Sc spiral galaxy
Dark Nebula
Cosmic Microwave Background (CMB)
Trojan asteroids
30. A word meaning 'the same everywhere throughout.'
quasar
homogeneous
Most dense
Bok Globule
31. Ganymede
MOONS: largest size
cosmology
Oort Cloud
Apollo asteroids
32. An empirical scheme for predictin ghe orbital distances of planets
Turn off Point
nova
Titus-Bode Law
Shepherd satellite
33. A continuous spectrum of light missing energy at a few wave lengths.
Light Curve
Absorption Spectrum
Halo
partile horizon
34. The place in the sky that the Earth's axis points toward (can be either north or south)
Colestial Pole
Perihelion
Pulsar
highlands
35. Mercury - Venus - Earth - Mars
Terrestrial Planets
shape and color of ELLIPTICAL galaxies
Wein's Law
Perihelion
36. Sc galaxies
Milky way Galaxy
Reflector
Flocculent spirals
Positive - Converge - Greater than 1
37. Highlands: rocks are made of lighter anorthosite (similar to old earth rocks) Maria: rocks made of heavy mare basalt (volcanic rock) everywhere else is loose regolith created by meteoric impact.
gravity
difference between maria and highlands of the moon.
Autumnal Equinox
The Local Group
38. What do we think the actual fate of the universe will be and why do we think this?
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.
Asymptotic giant Branch Star
Objective Lens
meteorite
39. Clouds of low density gas often found glowing faintly on either side of an AGN.
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
regolith
comet
radio lobe
40. The 11 or 22 period on the sun durin which sunspots increase - decrease - change polarity - increase and decrease again.
cosmic singularity
Summer Solstice
Sunspot cycle
Inverse Square Law
41. Formed rapidly - collapsed slower into disk shape - star birth rate is low but lasts longer and ongoing - contain higher mass blue stars.
isotropic
shape and color of SPIRAL galaxies
Corona
great dark spots
42. The organized effort to find life elsewhere in the universe. (Search for Extra-Terrestrial Intelligence)
neutrino
Convection
SETI
Cepheid variables
43. Massive compact halo objects (MACHO) - weakly interacting massive particles (WIMPY's)
era of recombination
Granules
Dark matter candidates
Nebula
44. A push or a pull
If it is in a denser medium - such as glass - it will move slower
The Local Group
Annular Eclipse
force
45. A term referring to Jupiter-like planets
tectonics of Earth
weight
molecular clouds
jovian
46. Heavier elements such as iron - silicon - magnesium - sulfer - nickel
slowest rotation
Parallax
Turn off Point
Make up of the terrestrial planets
47. When the Sun moves from south to north across the celestial equator (about March 21)
radio galaxy
Flocculent spirals
Oort cloud
Vernal Equinox
48. The line on an H-are diagram going from upper left to lower right where normal stars of different masses reside.
CCD
Main Sequence
Seeing
Autumnal Equinox
49. A very distant - star-like object with huge - broad emission lines. Probably the nucleus of a distant active galaxy.
Callisto (Jupiter)
Eclipses of the Moons of Jupiter
quasar
quarks
50. The time when the universe cooled sufficiently for atoms to exist. radiation dominated= first 300000 years - THEN era of recombination turns into matter dominated for next.
opposition
era of recombination
Seeing
fastest rotation