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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 fusion process that turns three helium nuclei into a carbon nucleus
Triple Alpha rocess
Open - flat - and closed.
smallest diameter
Stephen-Boltzman Law
2. Heavier elements such as iron - silicon - magnesium - sulfer - nickel
Make up of the terrestrial planets
Drake equation
How is winding dilemma solved?
Flat - Remain Parallel - Exactly 1
3. Mercury
Seyfert galaxy
Ionization
most eccentric orbit
synchrotron radiation
4. A huge sphere of tenuous gas surrounding the nucleus of a comet
Population 1 vs Population 2 stars
Vernal Equinox
coma
300000 KM/sec
5. The rotation period of the Earth measured relative to the stars.
Meridian
Bulge
mapping the structure of Milky Way disk
Sidereal Day
6. Jupiter
tectonics of Mars
great red spot
mare basalt
most moons
7. A toroidal or donut-shaped collection of material attracted to a central body like a star or black hole. Dust around an object
Primary Mirror
Electromagnetic Radiation: X-Ray
2 Reasons Why there are Supermassive Black holes at the center of every Galaxy
accretion disk
8. When one side of a body always faces the planet it revolves around
OB Associations
Sidereal Day
synchronous rotation
Kirkwood gaps
9. The science of measuring the apparent magnitudes of stars by imaging them through different filters.
Meridian
supernova
Photometry
Red Giant Branch Star
10. A very dense - highly populated cluster of galaxies
MOONS: roundest shape
opposition
Rich Cluster
Earth resurfaces itself due to erosion and plate tectonics - while the moon has neither.
11. The family of radiant energy that includes light as a subset
Main Sequence Stars
E=mc2
Electromagnetic Radiation
dark energy
12. A two-filter measure of the color - and hence temperature - of a star.
Summer Solstice
Magnification
Color Index
SETI
13. Infinitely long -> 10 cm
Light Curve
Magnification
Asymptotic giant Branch Star
Electromagnetic Radiation: Radio
14. The shadow behind the Earth or Moon where the Sun is partially obscured.
tectonics of Venus
Sunspot cycle
belt
Penumbra
15. 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 _____.
Seyfert galaxy
great red spot
Flat - Remain Parallel - Exactly 1
Focal Length
16. A technique using computer-controlled mirrors to sharpen images distorted by the atmosphere
Blackbody Curve
Void
Active Optics
acceleration
17. A very low mass particle formed in solar fusion reactions that reacts only weakly with matter
neutrino
Spectroscopic Parallax
Grand design spirals
density waves
18. A spherical shell of comets that orbit the sun at a great distance (roughly two light years from the sun)
Planck time
Positive - Converge - Greater than 1
Pulsar
Oort cloud
19. A small spherical dark nebula
Perihelion
AGN
Bok Globule
Ionization
20. Atmosphere blocks high energy wavelengths - atmosphere blurs optical radiation - atmosphere absorbs some radiation at all wavelengths even when it gets through.
Coldest surface
3 reasons we orbit satellites to observe universe
rotation curve = dark matter?
MOONS: thickest atmosphere
21. Matter that reveals itself only through its gravitational attraction.
least dense
weight
evidence of water on mars
dark matter
22. Dark areas on the sun that are cooler than the surrounding photosphere
Sunspots
Apollo asteroids
Radio Galaxy
Hipparchus
23. The dimming of starlight by intervening dust
Interstellar Extinction
Blackbody
Rich Cluster
MOONS: largest size
24. Light-colored high-pressure bands in Jupiter's atmosphere
Sidereal Day
Maria
zone
radio galaxy
25. Sc galaxies
great red spot
Open - flat - and closed.
CNO Cycle
Flocculent spirals
26. In a CLOSED UNIVERSE - the curvature of space-time is _________. Parallel beams will converge/diverge/remain parallel (circle one). The density parameter - Ω0 - is _____.
direct motion
Neutron Star
Color Index
Positive - Converge - Greater than 1
27. Venus
Resolving Power
Filament
Callisto (Jupiter)
Thickest atmosphere
28. Then the Sun moves from north to south across the celestial equator (about September 23)
bulge
Autumnal Equinox
Blackbody
smallest diameter
29. The point directly overhead.
Parallax
Zenith
Focal Plane
Maria
30. The measure of a variable star's apparent magnitude as it brightens and dims with time
Light Curve
fastest rotation
open star clusters
Total Eclipse
31. A particle of light
Photon
meteor
Electromagnetic Radiation
Light Curve
32. VENUS
Open Cluster
fastest rotation
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
chondrite
33. 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.
Focal Plane
era of recombination
How is winding dilemma solved?
Stephen-Boltzman Law
34. Is space infinitely large?
35. A logarithmically scaled value for the measured brightness of a star.
shape and color of SPIRAL galaxies
shape and color of ELLIPTICAL galaxies
Apparent Magnitude
cosmic singularity
36. A small and dim but hot star.
Cepheid Variable
MOONS: largest size
partile horizon
White Dwarf
37. Any change in the speed or direction of an object's motion
Total Eclipse
Ecliptic
acceleration
rotation curve=winding dilemma?
38. If stars have diff orbital periods - than any arms formed by stars will wind into a tight spiral pattern (billion yrs or so)
hottest surface
Eclipses of the Moons of Jupiter
rotation curve=winding dilemma?
Geocentric
39. A younger cluster of stars - found in the galaxy disk
nova
Milky way Galaxy
Open Cluster
Spectroscopic Parallax
40. The organization of clusters of galaxies into sheets and strings
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.
Red Giant Branch Star
radiant
Supercluster
41. The science of measuring light energy by wavelength.
Colestial Pole
Blackbody Curve
Spectroscopy
Meridian
42. The elementary building blocks from which protons and neutrons are formed.
protostar
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.
quarks
matter dominated universe
43. A planet that is farther from the sun than the Earth is
Superior planets
Spectroscopy
Particle Horizon
Winter Solstice
44. Formed from slow rotating clouds - collapsed quicker - initial star formation rate is high but died out - older - little rotation - look redder
interstellar dust
shape and color of ELLIPTICAL galaxies
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
Neutron Star
45. A rock or iron specimen that has fallen from space
meteorite
Colestial Pole
Dark Matter
great red spot
46. Atmosphere blocks high energy wavelengths - atmosphere blurs optical radiation - atmosphere absorbs some radiation at all wavelengths even when it gets through.
Hubble constant
standard candle
3 reasons we orbit satellites to observe universe
Seeing
47. The displacement of spectral lines to redder colors caused by the expansion of the universe.
cosmological red shift
retrograde motion
H-are Diagram
Planetary Nebula
48. A fusion process in which a carbon atom transmutes to oxygen and back - creating a helium atom in the process
Rich vs poor clusters
greehouse effects
CNO Cycle
Convection
49. The fate of the universe if it is closed. The universe expanding as much as possible and then retracting
Gravity only pulls matter back together. Therefore - if gravity is the only force that operates on cosmic scales then the expansion of the universe should decrease with time. The critical density is the value of matter density sufficient to halt the
isotropic
Big Crunch
radiation dominated universe
50. A representation of the changes in color and brightness of an evolving protostar.
Hyashi track
density parameter
SETI
cosmic fireball