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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. An object that may remain after a star explodes
Neutron Star
Granules
Dark matter candidates
cosmological principle
2. 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:
isotropic
Resolving Power
Drake equation
epicycle
3. The mass of an object divided by its volume
Gravitational Lens
The Local Group
Apollo asteroids
density
4. Large nebula consisting of very cold gas and dust
Molecular Clouds
highlands
Pixel
Triple Alpha rocess
5. Jupiter
Light Pollution
Io (jupiters moon)
Most dense
Largest diameter
6. The apparent path of the Sun through the stars on the celestial sphere.
Hubble constant
Big Crunch
Electron
Ecliptic
7. In Ptolemy's geocentric solar system - the large circle on which a planet's epicycle moved around the Earth.
interstellar dust
Thermonuclear Fusion
Electromagnetic Radiation
deferent
8. A bright area of higher temperature that often proceeds the formation of sunspots.
Color Index
conjunction
Plague
Parsec
9. Massive compact halo objects (MACHO) - weakly interacting massive particles (WIMPY's)
Interstellar Extinction
Disk
Dark matter candidates
Black Hole
10. 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.
mapping the structure of Milky Way disk
Positive - Converge - Greater than 1
Vernal Equinox
Pulsar
11. The trapping of heat by carbon dioxide or other gases in the Earth's atmosphere.
greehouse effects
zone
dark matter
meteoriod
12. A very dense - highly populated cluster of galaxies
supernova
supermassive black hole
most eccentric orbit
Rich Cluster
13. Venus (retrograde)
Photometry
Photosphere
slowest rotation
The Big Bang Theory resolves Olber's Paradox
14. A collection of comets in the plane of the solar system - located beyond the orbit of Pluto
Kuiper belt
MOONS: thickest atmosphere
SETI
coma
15. A fusion process in which a carbon atom transmutes to oxygen and back - creating a helium atom in the process
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.
CNO Cycle
Chromosphere
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.
16. 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.
Photon
Hydrostatic Equilibrium
scarp
blazar
17. Formed rapidly - collapsed slower into disk shape - star birth rate is low but lasts longer and ongoing - contain higher mass blue stars.
meteoriod
shape and color of SPIRAL galaxies
quarks
Geocentric
18. A term referring to Jupiter-like planets
Halo
dark matter
jovian
supernova
19. The Big Bang was not an explosion of matter into empty space - like the explosion of a bomb. Instead - it was an emergence of space and time filled with pure energy where before none of this was present. The point from which is emerged is called the
Grand design spirals
Kirkwood gaps
Sidereal Day
The Big Bang Theory
20. The entity responsible for spiral arms in grand-design spiral galaxies
Density Wave
gravity
deferent
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.
21. In a CLOSED UNIVERSE - the curvature of space-time is _________. Parallel beams will converge/diverge/remain parallel (circle one). The density parameter - Ω0 - is _____.
Blackbody
Cassini division
Positive - Converge - Greater than 1
Open Cluster
22. The process that powers the sun and hydrogen bombs
Oort Cloud
Thermonuclear Fusion
Globular Cluster
tectonics of Mars
23. Jupiter
fusion crust
most moons
chondrite
resonance
24. VENUS
Primary Mirror
Asymptotic giant Branch Star
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
Horizontal Branch Star
25. Long - meandering cliff formed when a planet surface cools and shrinks
Electromagnetic Radiation: Ultraviolet Light
scarp
Sc spiral galaxy
Proton-proton chain
26. The average distance between the Earth and the Sun (=1.5 x10^8km)
2 Reasons Why there are Supermassive Black holes at the center of every Galaxy
Astronomical Unit
Vernal Equinox
synchrotron radiation
27. All wavelengths of light emitted by a blackbody.
Blackbody Curve
Primary Mirror
aphelion
Granules
28. Elliptical orbits that come inside orbit of the Earth.
Apollo asteroids
Ecliptic
The Big Bang Theory
Pulsar
29. VENUS
bulge
Rich Cluster
Kirkwood gaps
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
30. 1μm 100 nm
CMB
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.
Parsec
Electromagnetic Radiation: Visible Light
31. 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)
rotation curve = dark matter?
epicycle
Sc spiral galaxy
Electromagnetic Radiation: Infrared
32. Finding a star's absolute magnitude from it's placement on an HR diagram. After finding the absolute magnitude - we measure the apparent magnitude - for a distance modulus and use this to find the distance. This method is good for finding distances t
Spectroscopic parallax
Sb spiral galaxy
interstellar dust
Pulsar
33. The law that describes the blackbody curve - and let to quantum mechanics.
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34. Formed from slow rotating clouds - collapsed quicker - initial star formation rate is high but died out - older - little rotation - look redder
Cosmic Microwave Background (CMB)
shape and color of ELLIPTICAL galaxies
Sc spiral galaxy
direct motion
35. Plate tectonics due to thickness of crust and maintain their general form when they collide-where most volcanoes are.
quasar
Blackbody Curve
tectonics of Earth
superclusters
36. What Ole Roemer used to measure the speed of light in a vacuum
Resolving Power
Summer Solstice
Turn off Point
Eclipses of the Moons of Jupiter
37. The elementary building blocks from which protons and neutrons are formed.
Drake equation
quarks
radio galaxy
Cassegrain Focus
38. A term referring to the orbital character of stars near the Sun
Differential Rotation
Rich vs poor clusters
Focal Plane
tectonics of Earth
39. Infinitely long -> 10 cm
superclusters
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.
Electromagnetic Radiation: Radio
least dense
40. Light scattered through the atmosphere that degrades astronomical images
radiation dominated universe
shape and color of SPIRAL galaxies
fusion crust
Light Pollution
41. Milky way galaxy is a member - a small poor cluster-about 30 galaxies
The Local Group
Cassegrain Focus
Hydrostatic Equilibrium
homogeneous
42. Heavier elements such as iron - silicon - magnesium - sulfer - nickel
Black Hole
Titus-Bode Law
Celestial Equator
Make up of the terrestrial planets
43. The rock that makes up the lunar maria
tectonics of Earth
mare basalt
H-are Diagram
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.
44. The law that predicts the possible types of spectra.
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45. A measure of how an object resists accelerating when acted upon by a force. It is proportional the amount of matter in an object
tectonics of Earth
rotation curve = dark matter?
mass
Cosmic Microwave Background
46. Extremely round - lots of liquid water - ice rafts on surface ACTIVE SURFACE
jovian
Europa (Jupiters moon)
Electromagnetic Radiation: Gamma Ray
Plank's Law
47. Cold aggregates of gas - large and contain a huge amount of matter - so cold that molecules stick together to form molecules.
critical density
Flat - Flat
White Dwarf
molecular clouds
48. A push or a pull
The Big Bang Theory resolves Olber's Paradox
Apollo asteroids
evidence of water on mars
force
49. Neptune or uranus
molecular clouds
Electron
roche limit
Coldest surface
50. In an OPEN UNIVERSE - the curvature of space-time is ____ - Parallel beams will converge/diverge/remain parallel (circle one). The density parameter - Ω0 - is____.
Negative - Diverge - Less than 1
asteroid
interstellar dust
least dense