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. A crystalline patter found in iron meteorites
Thermal Equilibrium
Milky way Galaxy
zone
widmanstatten pattern
2. A planet orbiting about a distant star
Dark Matter
Extrasolar Planet
Parsec
most moons
3. Poitns of gravitational stability in the orbit of a planet
Largest diameter
Lagrangian Razor
Trojan asteroids
radiant
4. The material from which the solar system formed
Electromagnetic Radiation: Infrared
Absorption Spectrum
H-are Diagram
solar nebula
5. The number of protons in an atom.
Atomic Number
Limb darkening
Celestial Sphere
3 reasons we orbit satellites to observe universe
6. Places in the asteroid belt - caused by resonance with Jupiter - where there are no asteroids
Most dense
evidence of water on mars
Kirkwood gaps
meteorite
7. Hot cells of gas that rise and fall in the hotosphere
Cosmic Microwave Background (CMB)
cosmology
Granules
Nucleus
8. A highly variable galaxy nucleus of which BL Lac is one. Their light is highly energetic and their spectra are featureless. (face on)
Earth resurfaces itself due to erosion and plate tectonics - while the moon has neither.
Astronomical Unit
blazar
Milky way Galaxy
9. Rich= dense crowded cores of galaxies - poor= few members and a looser organization of galaxies
Chandrasekhar Limit
Rich vs poor clusters
Corona
superclusters
10. Jupiter
fastest rotation
Prominence
Rich Cluster
Gamma-ray Burst
11. Disk dust grains are made of all the elements that are not in gaseous form in space which blocks starlight and causes interstellar extinction
Ganymede (Jupiter)
Blackbody
Electromagnetic Radiation: Gamma Ray
interstellar dust
12. 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 ________.
Earth resurfaces itself due to erosion and plate tectonics - while the moon has neither.
Flat - Flat
Plank's Law
cosmic fireball
13. Venus (retrograde)
Oort Cloud
Nucleus
slowest rotation
Electromagnetic Radiation: Infrared
14. Sc galaxies
Nova
accretion
Flocculent spirals
Sunspot cycle
15. What are the three possible geometries of the universe?
300000 KM/sec
acceleration
Open - flat - and closed.
Neutron Star
16. How did Earth come to have an oxygen rich atmosphere?
Electromagnetic Radiation: X-Ray
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.
quasar
H2 Regions
17. The particle horizon is the farthest we can see. It exists because the universe had a beginning and thus a definite age. Light from distances farther away from the particle horizon have not had time to reach us yet.
tectonics of Venus
Particle Horizon
Jupiters red spot
Steady State Theory (Leads to Olber's Paradox)
18. Earth
Wein's Law
Most dense
High Velocity Stars
Ground State
19. A phenomenon seen when the Earth passes through the orbit of a burned out comet
Sidereal Day
smallest diameter
Objective Lens
meteor shower
20. After stars form they pump light energy into surrounding gas causing it to heat up and glow (H2=ionized hydrogen - H1= neutral hydrogen in molcular couds)
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.
H2 Regions
slowest rotation
CCD
21. The rotation of a star or planet at different speeds at its equator and poles
dark energy
standard candle
differential rotation
planetary nebula
22. An efficient - two-dimensional electronic light detector. Common in digital cameras - they revolutionized astronomical imaging
quarks
Interstellar Extinction
Population 1 vs Population 2 stars
CCD
23. When the Moon entirely blocks the Sun.
Thermal Equilibrium
Total Eclipse
Vernal Equinox
Oort cloud
24. A term referring to Earth-like planets
Hubble constant
roche limit
Sidereal Day
terrestrial planet
25. Relativity predicts that nothing can travel faster than the speed of light in a vacuum - How can it move slower?
Earth resurfaces itself due to erosion and plate tectonics - while the moon has neither.
If it is in a denser medium - such as glass - it will move slower
Earth resurfaces itself due to erosion and plate tectonics - while the moon has neither.
Hydrostatic Equilibrium
26. Mercury
synchronous rotation
thinnest atmosphere
Yes - frozen at the poles- remains protected from the suns rays
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.
27. Dark areas on the sun that are cooler than the surrounding photosphere
molecular clouds
Sunspots
Inverse Square Law
Limb darkening
28. The shadow behind the Earth or Moon where the Sun is partially obscured.
Colestial Pole
density
Parsec
Penumbra
29. Formed from slow rotating clouds - collapsed quicker - initial star formation rate is high but died out - older - little rotation - look redder
Photon
Hydrostatic Equilibrium
shape and color of ELLIPTICAL galaxies
weight
30. A long-lived high-pressure bulge in Jupiter's southern hemisphere
great red spot
E=mc2
Cepheid variables
retrograde motion
31. The gap inthe outer portion of Saturn's A ring
general star population
Horizontal Branch Star
Enke gap
Parsec
32. The force of attraction between any two objects having mass
gravity
coma
difference between maria and highlands of the moon.
Ecliptic
33. The part of the Milky way that has on-going star formation
Sunspots
slowest rotation
Disk
weight
34. The amount of density needed to stop the universe from expanding and to begin the big crunch represented by Pc
Neutron Star
cosmological principle
critical density
Spectroscopic Parallax
35. Where is the center of the expansion
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.
The Big Bang Theory resolves Olber's Paradox
Electromagnetic Radiation: Gamma Ray
Globular Cluster
36. A spherical shell of comets that orbit the sun at a great distance (roughly two light years from the sun)
Oort cloud
Heliocentric
great red spot
Molecular Clouds
37. Form honeycomb like patterns surrounding empty or nearly empty voids.
radiation dominated universe
3 reasons we orbit satellites to observe universe
Ionization
superclusters
38. The light produced when particles from the sun collide with atmospheric molecules
Dark Nebula
plate tectonics
aurora
reflection star clusters
39. 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.
Perihelion
supernova
Cosmic Microwave Background (CMB)
Poor Cluster
40. A particle of light.
neutrino
CMB
Photon
Light Gathering Power
41. Half of the longest diameter across an ellipse
The Local Group
semimajor axis
aurora
meteoriod
42. The 'edge' of the universe. Light beyond this has not reached us yet.
Grand design spirals
Kuiper belt
partile horizon
Milky way Galaxy
43. 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
Radiative Diffusion
Spectroscopic parallax
meteoriod
greatest elongation
44. The final end state of a high mass star. .An entity for which gravity has completely overwhelmed all other forces of nature.
molecular clouds
Black Hole
self-propagating star formation
Sc spiral galaxy
45. When a planet lines up with the sun inthe sky
conjunction
Spectral Lines
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.
Earth resurfaces itself due to erosion and plate tectonics - while the moon has neither.
46. 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.
Celestial Equator
Parallax
Chandrasekhar Limit
Red Giant Branch Star
47. The source of the force that is accelerating the expansion rate of the universe.
Light Gathering Power
Stephen-Boltzman Law
Nova
dark energy
48. Cold aggregates of gas - large and contain a huge amount of matter - so cold that molecules stick together to form molecules.
Negative - Diverge - Less than 1
Continuous Spectrum
molecular clouds
highlands
49. What is the universe expanding into?
H2 Regions
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.
aurora
Gravitational Lens
50. Matter that reveals itself only through its gravitational attraction
Coronal Loop
Dark Matter
Parallax
Io (jupiters moon)
Sorry!:) No result found.
Can you answer 50 questions in 15 minutes?
Let me suggest you:
Browse all subjects
Browse all tests
Most popular tests
Major Subjects
Tests & Exams
AP
CLEP
DSST
GRE
SAT
GMAT
Certifications
CISSP go to https://www.isc2.org/
PMP
ITIL
RHCE
MCTS
More...
IT Skills
Android Programming
Data Modeling
Objective C Programming
Basic Python Programming
Adobe Illustrator
More...
Business Skills
Advertising Techniques
Business Accounting Basics
Business Strategy
Human Resource Management
Marketing Basics
More...
Soft Skills
Body Language
People Skills
Public Speaking
Persuasion
Job Hunting And Resumes
More...
Vocabulary
GRE Vocab
SAT Vocab
TOEFL Essential Vocab
Basic English Words For All
Global Words You Should Know
Business English
More...
Languages
AP German Vocab
AP Latin Vocab
SAT Subject Test: French
Italian Survival
Norwegian Survival
More...
Engineering
Audio Engineering
Computer Science Engineering
Aerospace Engineering
Chemical Engineering
Structural Engineering
More...
Health Sciences
Basic Nursing Skills
Health Science Language Fundamentals
Veterinary Technology Medical Language
Cardiology
Clinical Surgery
More...
English
Grammar Fundamentals
Literary And Rhetorical Vocab
Elements Of Style Vocab
Introduction To English Major
Complete Advanced Sentences
Literature
Homonyms
More...
Math
Algebra Formulas
Basic Arithmetic: Measurements
Metric Conversions
Geometric Properties
Important Math Facts
Number Sense Vocab
Business Math
More...
Other Major Subjects
Science
Economics
History
Law
Performing-arts
Cooking
Logic & Reasoning
Trivia
Browse all subjects
Browse all tests
Most popular tests