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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 rock or iron specimen that has fallen from space
Perihelion
Galilean satellite
meteorite
planetary nebula
2. Form honeycomb like patterns surrounding empty or nearly empty voids.
superclusters
High Velocity Stars
AGN
meteorite
3. A star that erratically and explosively brightens and dims
cosmology
Ammonia - methane - and water
inferior planets
Nova
4. The mirror that gathers the light in a reflector
Red Giant
scarp
Primary Mirror
Corona
5. 10^2 nm 10^7 nm
Meridian
Electromagnetic Radiation: Gamma Ray
plate tectonics
meteor shower
6. A spherical shell of comets that orbit the sun at a great distance (roughly two light years from the sun)
Precession
Energy Level
Cosmic Microwave Background (CMB)
Oort cloud
7. The number of protons in an atom.
fastest rotation
Atomic Number
Cosmological Principle
semimajor axis
8. A star fusing hydrogen to helium in it's core
meteor shower
Largest diameter
Steady State Theory (Leads to Olber's Paradox)
Main Sequence Stars
9. Thick rigid crust - no longer has plate tectonics but still has convective hot spots that create earth-like volcanoes except that last for billions of years because of lack of tectonics.
Triple Alpha rocess
Dark matter candidates
tectonics of Mars
Liquid metallic hydrogen
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.
Earth resurfaces itself due to erosion and plate tectonics - while the moon has neither.
opposition
Annular Eclipse
Parallax
11. Norhern lowlands- darker in color and have far fewer craters as if an ancient sea or ice field covered them. southern highlands- much higher in density of craters.
Spectroscopy
contrast northern lowlands and the southern highlands of mars...
Dwarf planets
The Big Bang Theory resolves Olber's Paradox
12. 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 _____.
Nova
MOONS: thickest atmosphere
Flat - Remain Parallel - Exactly 1
semimajor axis
13. Distribution of dust (tells us disk is thin) - find distances to O&B stars and H2 regions (arms are sights of star formation and OB stars live and die at location of birth) -Milky way has four arms. Sun is in spur apart from arms.
smallest diameter
accretion disk
E=mc2
mapping the structure of Milky Way disk
14. Electromagnetic Radiation
Cosmic Microwave Background (CMB)
A family of radiant energy- includes light
SETI
Spectroscopic Parallax
15. Material that shoots rapidly out into space. Flares cause Auroras
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.
Jupiters red spot
Flare
cosmic singularity
16. Hydrogen and helium (mainly)
Annular Eclipse
Make up of the jovian planets
radio galaxy
Kuiper belt
17. A particle of light
terrestrial planet
Photon
OB Associations
Sunspot cycle
18. A volume of space where few - if any - galaxies are located
Jovian Planets
most eccentric orbit
Focal Plane
Void
19. A small spherical dark nebula
Photon
Bok Globule
Seeing
retrograde motion
20. Elliptical orbits that come inside orbit of the Earth.
Apollo asteroids
Active Optics
greatest elongation
supermassive black hole
21. A long-lived high-pressure bulge in Jupiter's southern hemisphere
MOONS: roundest shape
Primary Mirror
Coronal Loop
great red spot
22. What do we think the actual fate of the universe will be and why do we think this?
open star clusters
contrast northern lowlands and the southern highlands of mars...
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.
MOONS: thickest atmosphere
23. When massive objects bend space and time enough to create multiple images of an object located behind them
Gravitational Lens
Eclipses of the Moons of Jupiter
In an expanding universe all galaxies see all other galaxies that are not gravitationally bound to them receding away. This is what we see in the Hubble Law. We infer that the Hubble law also holds true for all other galaxies.
radiation dominated universe
24. Very center of galaxy. suggestion of a black hole
Proton-proton chain
Electromagnetic Radiation: Gamma Ray
Ecliptic
nucleus
25. The point in its orbit where a planet is nearest the sun
Ecliptic
jovian
Perihelion
anorthosite
26. 100 nm 10 nm
Differential Rotation
Superior planets
Electromagnetic Radiation: Ultraviolet Light
Energy Level
27. In Ptolemy's geocentric solar system - the small circle on which a planet moved.
epicycle
Chandrasekhar Limit
Kirchhoff's Law
Galilean satellite
28. Elliptical orbits that come inside orbit of the Earth.
Density Wave
Spectroscopic parallax
Eyepiece Lens
Apollo asteroids
29. The shadow area behind the Earth or Moon where the Sun is completely obscured.
Main Sequence Stars
Sunspots
Umbra
Focal Length
30. Half of the longest diameter across an ellipse
Nova
Photometry
semimajor axis
plate tectonics
31. The point where an inferior planet is as far away from the sun as it can be (as seen from the Earth)
greatest elongation
fastest rotation
Make up of the terrestrial planets
Sb spiral galaxy
32. A perfect absorber and radiator of electromagnetic radiation.
Filament
Blackbody
Largest diameter
Coronal Loop
33. 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.
Ole Roemer
Radio Galaxy
Population 1 vs Population 2 stars
Cosmological Principle
34. Where is the center of the expansion
Kuiper belt
Synchrotron Rotation
dark matter
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.
35. Arcs of increased mass concentration that slow stars and gas down as they orbit through which cause the formation of stars.
density waves
Astronomical Unit
Spectral Lines
Coronal Loop
36. A high-pressure bulge in Neptune's southern hemisphere
Disk
great dark spots
Thermal Equilibrium
Doppler Shift
37. The rotation period of the Earth measured relative to the Sun.
Spectral Lines
weight
Metals
Synodic Day
38. A spinning neutron star
direct motion
Pulsar
Neutron Star
Open Cluster
39. 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.
most eccentric orbit
anorthosite
Coronal Loop
molecular clouds
40. The crust of a meteorite caused by its entry into Earth's atmosphere
Perihelion
Winter Solstice
Supernova (You can be my supernova girl)
fusion crust
41. The north-south line passing directly overhead through the zenith.
Meridian
Photometry
Supercluster
Maria
42. 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.
Light Curve
Primary Mirror
Cosmic Microwave Background (CMB)
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.
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:
Electromagnetic Radiation: Infrared
CMB
Drake equation
Olber's paradox
44. A star that is burning hydrogen to helium in a shell surrounding it's core
Electromagnetic Radiation: Gamma Ray
slowest rotation
Continuous Spectrum
Red Giant Branch Star
45. The shadow behind the Earth or Moon where the Sun is partially obscured.
Cosmological Principle
Thickest atmosphere
Penumbra
Black Hole
46. A subatomic particle with a negative charge. It creates light.
Ganymede (Jupiter)
Grand design spirals
radio lobe
Electron
47. Theory virtually demands that the geometry of the universe be ______. Results of measuring lumps in the cosmic background radiation indicate that the universe geometry is ________.
Flat - Flat
Nebula
Light-Year
Electromagnetic Radiation: Radio
48. Distance from sun to nucleus- 8 kiloparsecs (26000 LY) - diameter of Milky way- 150000 LY - length for sun to orbit once around milky way- 250 million years
radio galaxy
Milky way Galaxy
cosmic fireball
inferior planets
49. Formed rapidly - collapsed slower into disk shape - star birth rate is low but lasts longer and ongoing - contain higher mass blue stars.
solar nebula
Dwarf planets
shape and color of SPIRAL galaxies
Hyashi track
50. A phenomenon seen when the Earth passes through the orbit of a burned out comet
meteor shower
Seeing
neutrino
Differential Rotation