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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 science of measuring the apparent magnitudes of stars by imaging them through different filters.
Celestial Equator
Milky way Galaxy
Void
Photometry
2. The process of acquiring material
matter dominated universe
Light Gathering Power
shape and color of ELLIPTICAL galaxies
accretion
3. The lens that gathers the light in a refractor
synchrotron radiation
MOONS: thickest atmosphere
Objective Lens
Colestial Pole
4. The most mass a white dwarf can have before collapsing to a neutron star
Halo
Disk
Chandrasekhar Limit
Plank's Law
5. Ancient stream channels - flood planes - and sedimentary-type rock. Frozen water is found in the polar ice caps and in the soil.
Electromagnetic Radiation: Gamma Ray
evidence of water on mars
Refractor
Thermonuclear Fusion
6. Mercury
Flat - Remain Parallel - Exactly 1
smallest diameter
coma
supermassive black hole
7. The source of the force that is accelerating the expansion rate of the universe.
Plague
Electromagnetic Radiation: Infrared
dark energy
Sb spiral galaxy
8. A very dense - highly populated cluster of galaxies
Resolving Power
Spectroscopic Parallax
Rich Cluster
Focal Length
9. A word meaning 'the same in all directions.'
isotropic
Most dense
White Dwarf
Maria
10. Atmosphere blocks high energy wavelengths - atmosphere blurs optical radiation - atmosphere absorbs some radiation at all wavelengths even when it gets through.
Corona
Flare
3 reasons we orbit satellites to observe universe
Jovian Planets
11. The layer of the sun just above the photosphere
Light-Year
Coronal Loop
Chromosphere
Shepherd satellite
12. The wavelengths where a specific element can absorb or emit light.
condensation temperature
Resolving Power
Color Index
Spectral Lines
13. Moon in less than the angular diameter of the Sun.
Heliocentric
Annular Eclipse
Occam's razor
quasar
14. The science of measuring light energy by wavelength.
Earth resurfaces itself due to erosion and plate tectonics - while the moon has neither.
Spectroscopy
cosmology
Black Hole
15. The elementary building blocks from which protons and neutrons are formed.
Stephen-Boltzman Law
Neutron Star
quarks
Granules
16. Extremely round - lots of liquid water - ice rafts on surface ACTIVE SURFACE
Nova
Flat - Flat
Annular Eclipse
Europa (Jupiters moon)
17. A small spherical dark nebula
Bok Globule
Refractor
Nova
Neutron Star
18. How did Earth come to have an oxygen rich atmosphere?
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.
Hydrostatic Equilibrium
Magnification
Atomic Number
19. 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.
Oort Cloud
Cosmological Principle
Bulge
Void
20. In what chemical form are jupiters nitrogen - carbon and oxygen?
Flocculent spirals
Apollo asteroids
Ammonia - methane - and water
Astronomical Unit
21. Possible Fates of the Universe
Cepheid Variable
Vernal Equinox
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
Flocculent spirals
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)
Umbra
rotation curve = dark matter?
Ground State
Differential Rotation
23. 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.
Parallax
cosmic singularity
Nebula
Cassegrain Focus
24. The point in its orbit where a planet is farthest from the sun
aphelion
Red Giant
Grand design spirals
rotation curve=winding dilemma?
25. An object that may remain after a star explodes
Heliocentric
Neutron Star
reflection star clusters
Coldest surface
26. Flat disk with gas - dust - H2 regions - molecular clouds - dust young stars and remnants of old planetary nebula and supernova remnants. stars spin together with similar velocities called differential rotation
MOONS: most geologically active
disk
smallest diameter
CMB
27. A two-filter measure of the color - and hence temperature - of a star.
Color Index
Galilean satellite
Cosmic Microwave Background
Cassini division
28. 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.
Flocculent spirals
cosmic fireball
direct motion
29. Loops that trace the magnetic field as it erupts from a sunspot area and arches over to an adjacent area. They glow in the light of gas pouring out of corona and falling into photosphere.
Resolving Power
planetary nebula
Coronal Loop
Big Bang
30. Plate tectonics due to thickness of crust and maintain their general form when they collide-where most volcanoes are.
Sb spiral galaxy
Hubble law
tectonics of Earth
Light-Year
31. The oldest grouping of stars - found in the galaxy halo
Plank's Law
matter dominated universe
radio galaxy
Globular Cluster
32. The distance a moon can be from a planet before shattering from tidal forces
Extrasolar Planet
roche limit
Flat - Remain Parallel - Exactly 1
least dense
33. A very distant - star-like object with huge - broad emission lines. Probably the nucleus of a distant active galaxy.
quasar
terrestrial planet
Apparent Magnitude
superclusters
34. A high-pressure bulge in Neptune's southern hemisphere
smallest diameter
Plague
great dark spots
The Big Bang Theory
35. 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)
Dark Matter
greehouse effects
Doppler Shift
rotation curve=winding dilemma?
36. Dark areas on the sun that are cooler than the surrounding photosphere
Jovian Planets
Sunspots
matter dominated universe
density parameter
37. Electromagnetic Radiation
SETI
A family of radiant energy- includes light
evidence of water on mars
Shepherd satellite
38. Hurricane-like vortex in southern-hemisphere winds to north and south blow in opposite directions which keep it spinning and with no subsurface features like mountians it persists.
Extrasolar Planet
Jupiters red spot
3 reasons we orbit satellites to observe universe
Neutron Star
39. A measure of the ability of a telescope to see fine detail
meteoriod
most eccentric orbit
2 Reasons Why there are Supermassive Black holes at the center of every Galaxy
Resolving Power
40. The displacement of spectral lines to redder colors caused by the expansion of the universe.
cosmological red shift
Eyepiece Lens
Spectroscopic Parallax
Apparent Magnitude
41. Heavier elements such as iron - silicon - magnesium - sulfer - nickel
Coldest surface
Pulsar
Make up of the terrestrial planets
Light-Year
42. The movement of the Earth's crustal plates riding on top of the mantle.
plate tectonics
scarp
We don't know. It might be but does not have to be.
Photon
43. Any change in the speed or direction of an object's motion
Spectroscopic parallax
nova
asteroid
acceleration
44. A collection of comets in the plane of the solar system - located beyond the orbit of Pluto
Horizontal Branch Star
Kuiper belt
most moons
Seeing
45. Electromagnetic Radiation
mare basalt
Neutron Star
A family of radiant energy- includes light
Energy Level
46. A highly variable galaxy nucleus of which BL Lac is one. Their light is highly energetic and their spectra are featureless. (face on)
Jovian Planets
blazar
Largest diameter
Celestial Sphere
47. Population 1 with higher metals and contain many young stars in star clusters. Distribution of stars is everywhere in disk (arms only have 5% more stars)
Kuiper belt
Cosmological Principle
Olber's paradox
general star population
48. A toroidal or donut-shaped collection of material attracted to a central body like a star or black hole. Dust around an object
CCD
Light Pollution
Planetary Nebula
accretion disk
49. A fusion process in which a carbon atom transmutes to oxygen and back - creating a helium atom in the process
Oort Cloud
critical density
CNO Cycle
meteor
50. When the Sun is farthest north of the celestial equator (about June 22)
Summer Solstice
Seeing
general star population
How is winding dilemma solved?