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. When particles are compressed to an unnatural state where their pressure is not related to their temperature
Degeneracy
Earth resurfaces itself due to erosion and plate tectonics - while the moon has neither.
Radio Galaxy
Bok Globule
2. Originially thought to be stars emitting radio radiation but are now concluded to be nuclei of distant galaxies (same as radio galaxies aka emit streams of material)
quasar
Globular Cluster
Hipparchus
Flare
3. Form honeycomb like patterns surrounding empty or nearly empty voids.
MOONS: larger than mercury
superclusters
density
most eccentric orbit
4. A bright area of higher temperature that often proceeds the formation of sunspots.
roche limit
Nebula
Plague
chondrite
5. Venus
direct motion
acceleration
Ground State
Roundest orbit
6. A faint - remarkably uniform distribution of radiation in space
molecular clouds
Flat - Flat
Cosmic Microwave Background
Rich Cluster
7. The ratio of the actual density of the universe to the critical density. (actual density divided by the critical density
Coronal Loop
density parameter
Extrasolar Planet
Extrasolar Planet
8. Mercury and venus
Parsec
Cosmic Microwave Background
fewest moons
Dark Matter
9. What is the universe expanding into?
E=mc2
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.
asteroid
homogeneous
10. Earth
Focal Plane
highlands
Most dense
A family of radiant energy- includes light
11. A volume of space where few - if any - galaxies are located
supernova
Void
planetary nebula
Zenith
12. The location in an H-are diagram of a star cluster - where stars have just left the main sequence. Used to estimate the cluster age.
Turn off Point
Summer Solstice
Hydrostatic Equilibrium
Geocentric
13. The layer of the sun just above the photosphere
Cosmic Microwave Background (CMB)
Earth resurfaces itself due to erosion and plate tectonics - while the moon has neither.
Chromosphere
Sunspots
14. A rock or iron specimen that has fallen from space
Plague
meteorite
If it is in a denser medium - such as glass - it will move slower
HII Region
15. Small bulges - loosely wound - massive arms - arms have many H2 regions and look very lumpy
Degeneracy
Europa (Jupiters moon)
Resolving Power
Sc spiral galaxy
16. We can infer the absolute magnitude of pulsating variable stars by measuring their pulsation periods. The longer the pulsations - the greater their luminosities. We then again measure their apparent magnitudes - compare it with their absolute magnitu
Cepheid variables
plate tectonics
Hipparchus
Prominence
17. The linear correlation between the rate of the expansion of the universe and distance. Says that as galaxies get farther away in space - the speed with which they recede from us increases. So we can measure the amount of recessional velocity and use
accretion
tectonics of Mars
Asymptotic giant Branch Star
Hubble law
18. The imaginary sphere centered on the Earth that hols the stars.
H2 Regions
Dark Nebula
Celestial Sphere
Positive - Converge - Greater than 1
19. In what chemical form are jupiters nitrogen - carbon and oxygen?
HII Region
Ammonia - methane - and water
Perihelion
mapping the structure of Milky Way disk
20. 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
21. A galaxy sending out a stream of material from its nucleus
Plank's Law
fastest rotation
Radio Galaxy
Void
22. The instant of time after the Big Bang when space and time obtained their characteristics. (t=10^-43 sec when gravity freezes out-instant when gravity started existing as a separate force)
Electromagnetic Radiation: Infrared
opposition
mass
Planck time
23. The distance light travels in one year (=9.46x10^12km).
Light-Year
dark energy
Roundest orbit
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
24. Jupiter
coma
Penumbra
Largest diameter
solar nebula
25. A particle of light
Interstellar Extinction
Photon
Thermonuclear Fusion
Open Cluster
26. Jupiter
inferior planets
A family of radiant energy- includes light
Quasar
fastest rotation
27. The fusion process that turns three helium nuclei into a carbon nucleus
widmanstatten pattern
Triple Alpha rocess
Synodic Day
Milky way Galaxy
28. 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)
Parallax
H2 Regions
accretion
Grand design spirals
29. Extends to a distance of 50000AU. Same objects as in the Kuiper belt-when they fall in toward the sun they become comets. Debris from comets hitting the Earths atmosphere cause meteor showers.
nova
Oort Cloud
Population 1 vs Population 2 stars
Most dense
30. The faint glow of light left over from the Big Bang. cosmic microwave background are the photons that remain after the big bang that have not turned into matter.
Instability strip
CMB
mapping the structure of Milky Way disk
Energy Level
31. Jupiter
most moons
tectonics of Mars
Spectroscopy
Nucleus
32. The oldest grouping of stars - found in the galaxy halo
The Big Bang Theory resolves Olber's Paradox
density
Kirchhoff's Law
Globular Cluster
33. Old - pock marked - icy surface - interior is not differentiated - geologically dead - NOT ACTIVE SURFACE
Callisto (Jupiter)
The Big Bang Theory resolves Olber's Paradox
density waves
Metals
34. A measure of the ability of a telescope to see fine detail
Resolving Power
Prominence
gravity
Planetary Nebula
35. Matter so dense that even light cannot escape its gravity
MOONS: larger than mercury
Black Hole
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
gravity
36. Jupiter - Saturn - Uranus - Neptune
supermassive black hole
Flat - Remain Parallel - Exactly 1
Degeneracy
Jovian Planets
37. The entity responsible for spiral arms in grand-design spiral galaxies
Total Eclipse
Seyfert galaxy
Sb spiral galaxy
Density Wave
38. The final end state of an intermediate to high mass star. An entity in which all the electrons have been pushed into the protons.
aphelion
Neutron Star
radiation pressure
Electron
39. Mercury
Emission Spectrum
Cepheid variables
smallest diameter
Granules
40. As open clusters age - they push gas away but dust remains this can reflect light giving the cluster a blue-ish color. also called reflection nebula
Precession
Meridian
reflection star clusters
Most dense
41. Cold aggregates of gas - large and contain a huge amount of matter - so cold that molecules stick together to form molecules.
Ground State
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.
Cosmic Microwave Background
molecular clouds
42. When one side of a body always faces the planet it revolves around
synchronous rotation
Roundest orbit
Photon
Drake equation
43. The seasonal shifting of a nearby star's position relative to more distant objects.
Continuous Spectrum
Absolute Magnitude
Parallax
Celestial Equator
44. The apparent path of the Sun through the stars on the celestial sphere.
Ecliptic
Sidereal Day
density
Planetary Nebula
45. A collection of galaxies like the one the Milky Way belongs to
Liquid metallic hydrogen
Dark Matter
Poor Cluster
shape and color of ELLIPTICAL galaxies
46. 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 ________.
Thermonuclear Fusion
Flat - Flat
Stephen-Boltzman Law
Bok Globule
47. Heavier elements such as iron - silicon - magnesium - sulfer - nickel
Thermal Equilibrium
Liquid metallic hydrogen
Make up of the terrestrial planets
The Big Bang Theory resolves Olber's Paradox
48. VENUS
300000 KM/sec
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
interstellar dust
Ground State
49. The point where an inferior planet is as far away from the sun as it can be (as seen from the Earth)
greatest elongation
Spectral Lines
Plague
Bok Globule
50. The telescope configuration that has the focus placed at the back of the primary mirror
Shepherd satellite
Secondary Mirror
Cassini division
Cassegrain Focus