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. Small bulges - loosely wound - massive arms - arms have many H2 regions and look very lumpy
Sc spiral galaxy
fewest moons
radio galaxy
opposition
2. The universe is isotropic - homogeneous - and without beginning or end in time and space. If the universe is truly homogeneous then every line of sight will eventually end on a galaxy. If it has existed forever then there has been enough time for lig
Warning
: Invalid argument supplied for foreach() in
/var/www/html/basicversity.com/show_quiz.php
on line
183
3. 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.
Black Hole
Gamma-ray Burst
Cosmological Principle
Europa (Jupiters moon)
4. The source of the force that is accelerating the expansion rate of the universe.
Prominence
3 reasons we orbit satellites to observe universe
dark energy
Kirchhoff's Law
5. The opaque universe that existed for 300000 years after the Big Bang. (photons outnumbered nuclei by 1 billion to one - so less light)
Cosmic Microwave Background
Self-Propogating Star Formation
partile horizon
radiation dominated universe
6. A word meaning 'the same in all directions.'
Extrasolar Planet
bulge
isotropic
chemical differentiation
7. When the Moon entirely blocks the Sun.
Negative - Diverge - Less than 1
Apollo asteroids
Eyepiece Lens
Total Eclipse
8. A measure of how an object resists accelerating when acted upon by a force. It is proportional the amount of matter in an object
mass
bulge
Energy Level
Electromagnetic Radiation: Microwave
9. The rotation period of the Earth measured relative to the Sun.
Asymptotic giant Branch Star
greehouse effects
Synodic Day
Nebula
10. Flat disk with gas - dust - H2 regions - molecular clouds - dust young stars and remnants of old planetary nebula and supernova remnants. stars spin together with similar velocities called differential rotation
epicycle
Eclipses of the Moons of Jupiter
disk
Light Gathering Power
11. IO
Cosmic Microwave Background
MOONS: most geologically active
Cepheid Variable
Enke gap
12. Venus
rotation curve = dark matter?
Thickest atmosphere
Negative - Diverge - Less than 1
Disk
13. When the Sun is farthest south of the celestial equator (About December 22)
Apparent Magnitude
Differential Rotation
Winter Solstice
meteoriod
14. Elliptical orbits that come inside orbit of the Earth.
Kirkwood gaps
Flat - Remain Parallel - Exactly 1
Rich Cluster
Apollo asteroids
15. The area behind a lens where images are resolved
condensation temperature
Focal Plane
Convection
Celestial Sphere
16. A bridge of material held in position above the solar surface. They can remain for hours even days
Black Hole
Prominence
Absolute Magnitude
synchronous rotation
17. Milky way galaxy is a member - a small poor cluster-about 30 galaxies
The Local Group
Void
Poor Cluster
Gravitational Lens
18. A spherical shell of comets that orbit the sun at a great distance (roughly two light years from the sun)
Oort cloud
self-propagating star formation
Most dense
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.
19. The distance between a lens and its focal plane
SETI
Focal Length
Open Cluster
Cepheid Variable
20. The rotation of a star or planet at different speeds at its equator and poles
differential rotation
open star clusters
dark matter
Reflector
21. A star that blows itself apart
Resolving Power
Supernova (You can be my supernova girl)
Focal Length
Cosmological Principle
22. The surface of the sun
Photometry
condensation temperature
neutrino
Photosphere
23. 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.
Seeing
CMB
synchrotron radiation
Nebula
24. The final end state of an intermediate to high mass star. An entity in which all the electrons have been pushed into the protons.
Pulsar
Neutron Star
Light Gathering Power
Winter Solstice
25. In Ptolemy's geocentric solar system - the large circle on which a planet's epicycle moved around the Earth.
radiation pressure
deferent
Olber's paradox
HII Region
26. The point directly overhead.
Jupiters red spot
Zenith
protostar
dark matter
27. A large - irregularly shaped rocky object orbiting the sun mostly between mars and jupiter. Left-over planetesimals
asteroid
Dark Nebula
Kirchhoff's Law
Cosmological Principle
28. Is space infinitely large?
Warning
: Invalid argument supplied for foreach() in
/var/www/html/basicversity.com/show_quiz.php
on line
183
29. Infinitely long -> 10 cm
jovian
Electromagnetic Radiation: Radio
Perihelion
Dark matter is located at center of clusters - pulling the cluster members into faster orbits--dark matter gravity keeps objects in galxies bound.
30. Hurricane-like vortex in southern-hemisphere winds to north and south blow in opposite directions which keep it spinning and with no subsurface features like mountians it persists.
dark energy
Objective Lens
mass
Jupiters red spot
31. A two-filter measure of the color - and hence temperature - of a star.
Color Index
Absolute Magnitude
Radio Galaxy
How is winding dilemma solved?
32. Matter that reveals itself only through its gravitational attraction.
aurora
Inverse Square Law
3 reasons we orbit satellites to observe universe
dark matter
33. 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.
Oort Cloud
Hubble constant
radio galaxy
Milky way Galaxy
34. The elementary building blocks from which protons and neutrons are formed.
Steady State Theory (Leads to Olber's Paradox)
Black Hole
quarks
Photon
35. The light produced when particles from the sun collide with atmospheric molecules
aurora
Ionization
density
H-are Diagram
36. The number of protons in an atom.
Rich Cluster
Total Eclipse
Nova
Atomic Number
37. What is the universe expanding into?
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.
synchrotron radiation
Winter Solstice
Parallax
38. The mix of pure photon energy that emerged at the start of the universe.
Lagrangian Razor
cosmic fireball
Europa (Jupiters moon)
3 reasons we orbit satellites to observe universe
39. A planet orbiting about a distant star
Nucleus
Photometry
Light-Year
Extrasolar Planet
40. Light-flaky crust - convective currents cause it to wrinkle and bunch (1/5 of surface). uniform cratering suggests lack of weathering and tectonics. volcanoes are flat due to atmospheric pressure.
tectonics of Venus
Occam's razor
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.
Quasar
41. A nearby galaxy with a quasar-like nucleus. closer but less bright than quasars-weaker
Red Giant
Horizontal Branch Star
Seyfert galaxy
Limb darkening
42. A subatomic particle with a negative charge. It creates light.
Electron
Terrestrial Planets
Globular Cluster
High Velocity Stars
43. How is the Hubble Law consistent with an expanding universe?
Apollo asteroids
The Big Bang Theory
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.
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
44. The family of radiant energy that includes light as a subset
Electromagnetic Radiation
great red spot
Earth resurfaces itself due to erosion and plate tectonics - while the moon has neither.
greehouse effects
45. If stars have diff orbital periods - than any arms formed by stars will wind into a tight spiral pattern (billion yrs or so)
rotation curve=winding dilemma?
least dense
Big Crunch
Planetary Nebula
46. A star that erratically and explosively brightens and dims
terrestrial planet
aphelion
Gamma ray bursts
Nova
47. Mercury and venus
Hubble constant
fewest moons
meteoriod
Kuiper belt
48. The science of measuring light energy by wavelength.
Red Giant Branch Star
Spectroscopy
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
partile horizon
49. 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.
accretion
chemical differentiation
open star clusters
Chromosphere
50. 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
Black Hole
Spectral Lines
H-are Diagram