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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. A term referring to the orbital character of stars near the Sun
Earth resurfaces itself due to erosion and plate tectonics - while the moon has neither.
Differential Rotation
most moons
Jovian Planets
2. The cosmological principle is the assumption that the universe is isotropic and homogeneous.The Big Bang assumes it to be a correct principle so that what we observe is exactly like What is too far away to be observed.
Largest diameter
tectonics of Earth
Cosmological Principle
Radio Galaxy
3. The apparent backward motion of a planet against the background of stars.
Gamma-ray Burst
retrograde motion
tectonics of Mars
Milky way Galaxy
4. A small and dim but hot star.
Main Sequence
E=mc2
White Dwarf
Hydrostatic Equilibrium
5. When the Sun is farthest south of the celestial equator (About December 22)
Bok Globule
Chandrasekhar Limit
Winter Solstice
Eclipses of the Moons of Jupiter
6. A planet that is farther from the sun than the Earth is
CCD
MOONS: largest size
meteorite
Superior planets
7. The linear correlation between the rate of the expansion of the universe and distance. Says that as galaxies get farther away in space - the speed with which they recede from us increases. So we can measure the amount of recessional velocity and use
semimajor axis
force
chemical differentiation
Hubble law
8. The source of the force that is accelerating the expansion rate of the universe.
dark energy
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
Parallax
Synchrotron Rotation
9. Mercury
differential rotation
asteroid
opposition
thinnest atmosphere
10. The surface of the sun
synchronous rotation
Blackbody
cosmology
Photosphere
11. Poitns of gravitational stability in the orbit of a planet
condensation temperature
meteor
least dense
Lagrangian Razor
12. The oldest part of the Milky Way
Winter Solstice
Halo
We don't know. It might be but does not have to be.
Big Crunch
13. A star that erratically and explosively brightens and dims
Apparent Magnitude
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
Primary Mirror
Nova
14. Any class of objects with a uniform luminosity used to determine distance.
jovian
standard candle
accretion disk
roche limit
15. 1 mm 1μm
Electromagnetic Radiation: Infrared
Black Hole
Photon
Pixel
16. When the Moon entirely blocks the Sun.
Total Eclipse
meteor shower
era of recombination
Rich Cluster
17. The apparent path of the Sun through the stars on the celestial sphere.
Ecliptic
radio galaxy
Celestial Sphere
Nucleus
18. A huge sphere of tenuous gas surrounding the nucleus of a comet
Positive - Converge - Greater than 1
coma
Lagrangian Razor
Electromagnetic Radiation: X-Ray
19. Small compact stars called white dwarfs can have material deposited on their surfaces. In time material heats up and explodes in surface nuclear reaction- star brightens - settles - repeats.
nova
Objective Lens
AGN
Cepheid variables
20. A repeated - periodic push or pull capable of summing into a larger push or pull
Astronomical Unit
resonance
Secondary Mirror
Instability strip
21. The mirror that gathers the light in a reflector
Bulge
radio galaxy
Primary Mirror
Precession
22. A particle of light
Photon
Apparent Magnitude
condensation temperature
Pulsar
23. A rock or iron specimen that has fallen from space
meteorite
Neutron Star
Summer Solstice
Brown dwarf
24. A star that has become a red giant for the second and final time. It is burning helium to carbon in a shell surrounding the core
Asymptotic giant Branch Star
3 reasons we orbit satellites to observe universe
Primary Mirror
Objective Lens
25. Extremely round - lots of liquid water - ice rafts on surface ACTIVE SURFACE
Hubble law
Wein's Law
density parameter
Europa (Jupiters moon)
26. VENUS
nova
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
Perihelion
Hipparchus
27. The rock that makes up the lunar maria
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.
slowest rotation
Synodic Day
mare basalt
28. When massive objects bend space and time enough to create multiple images of an object located behind them
Chromosphere
Gravitational Lens
Gamma-ray Burst
general star population
29. Electromagnetic Radiation
Chandrasekhar Limit
Flat - Remain Parallel - Exactly 1
Cosmological Principle
A family of radiant energy- includes light
30. Plate tectonics due to thickness of crust and maintain their general form when they collide-where most volcanoes are.
Dark matter candidates
Magnification
tectonics of Earth
Pixel
31. Is space infinitely large?
32. Ganymede
Kirchhoff's Law
Supercluster
Density Wave
MOONS: largest size
33. 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.
conjunction
Blackbody Curve
Parallax
Electromagnetic Radiation
34. A very dense - highly populated cluster of galaxies
Open - flat - and closed.
Callisto (Jupiter)
least dense
Rich Cluster
35. 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.
Hubble constant
Population 1 vs Population 2 stars
semimajor axis
cosmology
36. Radiation (possibly left over from the big bang) that fills the universe. Perfect black body spectrum and tells us a bit aout how galaxies are formed.
Blackbody Curve
rotation curve=winding dilemma?
Cosmic Microwave Background (CMB)
Proton-proton chain
37. A spherical shell of comets that orbit the sun at a great distance (roughly two light years from the sun)
meteor
Spectroscopy
Supernova (You can be my supernova girl)
Oort cloud
38. Wave- only waves cause an interference pattern when passing through a double slit - particle- only particles deposit energy at specific locations (the way an image builds up on digital camera)
Dark Matter
cosmic fireball
rotation curve=winding dilemma?
Light: travels like a wave - detected like a particle
39. A particle of light.
Doppler Shift
Penumbra
Photon
greatest elongation
40. The oldest grouping of stars - found in the galaxy halo
Doppler Shift
Globular Cluster
evidence of water on mars
aphelion
41. Flattened spherical distribution of old stars with some young stars too. 'hub' of Milky way - stars orbit with solid body speeds. Elongated into bar shape
Spectral Lines
standard candle
Eclipses of the Moons of Jupiter
bulge
42. Large bulge - tightly wound spiral arms - relatively few h2 regions and are smooth
Plague
Sa spiral galaxy
Enke gap
A family of radiant energy- includes light
43. Radiation emitted when charged particles spiral rapidly in a magnetic field. come off of jets from black holes.
Astronomical Unit
great dark spots
synchrotron radiation
nucleus
44. The 'edge' of the universe. Light beyond this has not reached us yet.
E=mc2
partile horizon
Nova
Parallax
45. The mix of pure photon energy that emerged at the start of the universe.
cosmological red shift
Halo
fewest moons
cosmic fireball
46. Centered on the sun.
Heliocentric
general star population
Parallax
Jovian Planets
47. The mirror that determines the focus configuration of a reflector
Secondary Mirror
Rich Cluster
Electromagnetic Radiation: Infrared
The Local Group
48. The imaginary sphere centered on the Earth that hols the stars.
Proton-proton chain
mapping the structure of Milky Way disk
Celestial Sphere
weight
49. Stars orvits do not define the spiral patterns - instead they are density waves that move at slower speeds (arms are defined by young O and B stars and gas clouds)
MOONS: thickest atmosphere
evidence of water on mars
How is winding dilemma solved?
Radiative Diffusion
50. When the Sun moves from south to north across the celestial equator (about March 21)
Reflector
Inverse Square Law
Vernal Equinox
era of recombination