SUBJECTS
|
BROWSE
|
CAREER CENTER
|
POPULAR
|
JOIN
|
LOGIN
Business Skills
|
Soft Skills
|
Basic Literacy
|
Certifications
About
|
Help
|
Privacy
|
Terms
|
Email
Search
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. What do we think the actual fate of the universe will be and why do we think this?
Cepheid Variable
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.
Blackbody Curve
Seyfert galaxy
2. Plate tectonics due to thickness of crust and maintain their general form when they collide-where most volcanoes are.
tectonics of Earth
rotation curve = dark matter?
planetesimal
era of recombination
3. A spinning neutron star
CMB
Pulsar
epicycle
superclusters
4. A term referring to Jupiter-like planets
jovian
open star clusters
Objective Lens
Cepheid Variable
5. A large and bright but cool star.
zone
smallest diameter
Red Giant
Sidereal Day
6. The mirror that gathers the light in a reflector
SETI
Eyepiece Lens
Drake equation
Primary Mirror
7. The line on an H-are diagram going from upper left to lower right where normal stars of different masses reside.
Light Gathering Power
Main Sequence
anorthosite
evidence of water on mars
8. The average distance between the Earth and the Sun (=1.5 x10^8km)
fewest moons
Metals
Cepheid Variable
Astronomical Unit
9. The larger bodies that formed early in teh solar nebula that were chemically differentiated
planetesimal
Kuiper belt
Electromagnetic Radiation: Radio
quarks
10. A star that is in the process of forming. It glows from gravitational contraction
acceleration
protostar
Sidereal Day
Dark Nebula
11. A perfect absorber and radiator of electromagnetic radiation.
CMB
Blackbody
zone
Photosphere
12. The family of radiant energy that includes light as a subset
Bulge
Electromagnetic Radiation
Synchrotron Rotation
Secondary Mirror
13. The point in its orbit where a planet is nearest the sun
High Velocity Stars
Perihelion
critical density
Quasar
14. 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
Open Cluster
Red Giant
Milky way Galaxy
open star clusters
15. The apparent backward motion of a planet against the background of stars.
greatest elongation
Hubble law
retrograde motion
It does not have to expand into anything. It might just be that the 3 dimensions of space are getting bigger. It may also be that our 3 spatial dimensions are expanding into higher dimensions if such things exist.
16. The location of a supermassive black hole
Nucleus
Pixel
aphelion
superclusters
17. A spherical shell of comets that orbit the sun at a great distance (roughly two light years from the sun)
Oort cloud
Cosmic Microwave Background
Light Curve
gravity
18. The rate of expansion of the universe.
Coronal Loop
Vernal Equinox
Photosphere
Hubble constant
19. How is the Hubble Law consistent with an expanding universe?
Largest diameter
Pulsar
Electromagnetic Radiation: Visible Light
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.
20. The location in the Milky Way where stars orbit like a solid wheel
Globular Cluster
Photon
open star clusters
Bulge
21. 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.
fusion crust
Cosmological Principle
dark energy
Enke gap
22. The mix of pure photon energy that emerged at the start of the universe.
mare basalt
Heliocentric
blazar
cosmic fireball
23. In Ptolemy's geocentric solar system - the large circle on which a planet's epicycle moved around the Earth.
deferent
radio lobe
Yes - frozen at the poles- remains protected from the suns rays
Turn off Point
24. Stars fromt he Halo that have drifted into the disk. as earth zooms past them in a faster orbit they appear to be going backward very fast
High Velocity Stars
Neutron Star
widmanstatten pattern
The Big Bang Theory resolves Olber's Paradox
25. Sa - Sb galaxies where two magnificent arms wind their way from nucleus out in a symmetrical manner.
Grand design spirals
widmanstatten pattern
Roundest orbit
Hubble law
26. The organization of clusters of galaxies into sheets and strings
Supercluster
Synodic Day
Globular Cluster
Main Sequence Stars
27. The law that describes the blackbody curve - and let to quantum mechanics.
Warning
: Invalid argument supplied for foreach() in
/var/www/html/basicversity.com/show_quiz.php
on line
183
28. Long - meandering cliff formed when a planet surface cools and shrinks
direct motion
contrast northern lowlands and the southern highlands of mars...
Summer Solstice
scarp
29. A continuous spectrum of light missing energy at a few wave lengths.
most moons
Summer Solstice
Electromagnetic Radiation: Radio
Absorption Spectrum
30. Form honeycomb like patterns surrounding empty or nearly empty voids.
Yes - frozen at the poles- remains protected from the suns rays
superclusters
inferior planets
Kuiper belt
31. Young clusters in disk are irregularly shaped since they have no time to relax into the rounder relaxed shape of globular clusters-will constantly be torn apart and assimilated.
Ionization
Make up of the terrestrial planets
Positive - Converge - Greater than 1
open star clusters
32. An entity that is likely in the nucleus of most - if not all - galaxies.
supermassive black hole
Spectral Lines
Neutron Star
Convection
33. A technique using computer-controlled mirrors to sharpen images distorted by the atmosphere
Spectroscopic parallax
Milky way Galaxy
Active Optics
Instability strip
34. The line on an H-are diagram going from upper left to lower right where normal stars of different masses reside.
Absorption Spectrum
rotation curve = dark matter?
Oort cloud
Main Sequence
35. Heavier elements such as iron - silicon - magnesium - sulfer - nickel
radiation pressure
blazar
Make up of the terrestrial planets
Void
36. The point where a superior planet is as far away from the sun as it can be (as seen from the Earth)
great red spot
opposition
Yes - frozen at the poles- remains protected from the suns rays
Parallax
37. The point where an inferior planet is as far away from the sun as it can be (as seen from the Earth)
greatest elongation
great dark spots
retrograde motion
2 Reasons Why there are Supermassive Black holes at the center of every Galaxy
38. Largest moon in solar system - two differenet types of terrain - darker terrain is older - NOT ACTIVE SURFACE
Ganymede (Jupiter)
Ecliptic
Astronomical Unit
synchrotron radiation
39. Matter that reveals itself only through its gravitational attraction
Stephen-Boltzman Law
H2 Regions
Earth resurfaces itself due to erosion and plate tectonics - while the moon has neither.
Dark Matter
40. A repeated - periodic push or pull capable of summing into a larger push or pull
resonance
Ole Roemer
The Big Bang Theory resolves Olber's Paradox
Flat - Flat
41. The oldest terrain on the moon
Radiative Diffusion
shape and color of ELLIPTICAL galaxies
Thickest atmosphere
highlands
42. The dimming of starlight by intervening dust
Interstellar Extinction
High Velocity Stars
Main Sequence
Kirchhoff's Law
43. Venus
terrestrial planet
Open - flat - and closed.
Thickest atmosphere
Apollo asteroids
44. 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
Light Gathering Power
The Big Bang Theory
Horizontal Branch Star
Plank's Law
45. The entity responsible for spiral arms in grand-design spiral galaxies
Density Wave
Population 1 vs Population 2 stars
Cepheid Variable
difference between maria and highlands of the moon.
46. The apparent path of the Sun through the stars on the celestial sphere.
Disk
Flat - Flat
Ecliptic
partile horizon
47. A star without enough mass to begin hydrogen fusion
Brown dwarf
era of recombination
radiation dominated universe
Corona
48. The location in the Milky Way where stars orbit like a solid wheel
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
Bulge
Big Bang
Hydrostatic Equilibrium
49. What are the three possible geometries of the universe?
Open - flat - and closed.
Kirchhoff's Law
planetesimal
supermassive black hole
50. 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 _____.
Radio Galaxy
Neutron Star
White Dwarf
Flat - Remain Parallel - Exactly 1