Space Flashcards
(109 cards)
What is the frame of reference?
Anything that explains and gives you a relative sense of position/motion (e.g. relative to the Earth, the bus is moving, but to people on the bus, no) (参照物)
What are some examples of frames of reference that people use to examine the skies and what did they use them for?
Equator and Prime Meridian axes (latitude and longitude) celestial poles, etc.; to identify individual coordinates for celestial bodies
What did ancient people conclude about the skies (non-mythical)?
- Stars make unchanging patterns (untrue, but only very little changes), these patterns look like objects (constellations)
- Geocentric (False, but they used it)
- On each successive day, each star rises 4 minutes earlier than before, so they change and people used this to create calendars (stars seen on different nights)
- The sun and moon rise and set at a different rate than all the other stars, and the moon has phases
- 5 other planets also rise and set differently (ancient people thought of them as special stars)
What are some legends/myths that ancient people made from the stars?
- Egypt: 1. Pyramids built to align with stars so that pharaoh could go to heavens 2. Sun god Ra was carried by a boat in skies
- Romans: 1. Jupiter = king of the gods and god of the skies
- First Nations: 1. Bighorn Medicine Wheel (?) may have been observation 2. Big Dipper is bear running away from hunters 3. 3 hunters, 4 elk (Snohomish)
- Maya: 1. Stars = gods 2. Events believed to coincide with celestial movement 3. Temples/pyramids designed to see certain stars through a window at certain important times 4. Accurate calendar by 800 AD
- Ancient Celts: Stonehenge = summer+winter solstice
- Polynesians: Sailors used stars to sail
- Chinese: 1. First star catalogue by 甘德 400 BC 2. Detailed records/observations stored from 600 BC 3. Precisely predict eclipses
- Ursa Major most well-known
- Constellations change position but change shape rarely (Appear to rotate around North Star Polaris (but changes due to seasons (Earth revolution), and Earth’s axis tilt, Earth self rotation)
How do you measure celestial coordinates?
Altitude + Azimuth = Coordinates
- Altitude measured by an astrolabe and is degree from horizon
- Azimuth measured by a compass and is clockwise degree from direct north
- POLARIS ON HANDLE OF URSA MINOR
How do you observe the movement of celestial bodies?
You use other stars as a frame of reference (since their relative movement is less observable in calculations due to being so far) rather than Earth perspective since the Earth has self rotation
What are the 4 solstices and equinoxes and what are their dates?
Winter solstice (December 21, least daylight, Summer solstice (June 21, most daylight), Vernal equinox (March 20, equal day and night), Autumnal equinox (September 22, equal day and night)
What is the zenith?
The point directly above the observer (90 degree altitude)
History of the Geocentric Model
- First proposed: Aristotle (Greek): Earth = centre of universe, everything revolves around it in circular orbits
- Failed to explain planets’ reversed motions (retrograde motion)
- Universe had Earth and orbiting planets + outer spherical shell containing fixed stars (false) - Improved: Ptolemy (Greek): Epicycles to explain retrograde motion, made more sense (Still complicated)
History of the Heliocentric Model
Proposed: Nicholas Copernicus (Polish): Sun = centre of universe, planets orbit in circular motion (Still contained epicycles)
- 1608: HANS LIPPERSHEY (Dutch) INVENTED TELESCOPE TO MAGNIFY
Improved (1): Galileo Galilei (Italian): Improved the telescope, used it on the skies
1. Found craters and mountains on Moon
2. Found Jupiter’s moons
3. Sun spots (cold areas on sun surface)
4. Could not see details of stars = Planets are much closer than stars
Improved (2): Johannes Kepler (German): Planetary orbits = elliptical (ellipses) not circular (Matches Tycho Brahe’s star chart numbers), finally removed epicycles
What is Isaac Newton’s Law of Universal Gravitation?
A law that states that any two things in the universe has an attraction force that acts on each other depending on mass and mutual distance
Ellipses
- Two focal points F1(-c,0) and F2(c,0)
- Point M
- MF1+MF2 =2a = 2*length of long axis
- Formula: x2/a2 + y2/b2 = 1
- Area = πab
- Perimeter = 2π√((a2+b2)/2)
What is a telescope and what are its main components?
A tool used to observe objects that are very far away by magnifying them. It has ocular (eyepiece) and objective lens/mirrors. The objective is usually much larger than the ocular to gather more light and produce the magnifying effect.
What is resolving power and how can we increase it?
The clarity of the image a telescope can make; Make the objective lens larger
What is a refracting telescope, and its pros/cons?
A telescope that uses 2 lens (convex) (Objective to ocular).
Pros: Simple, good for planetary range, no maintenance required
Cons: Not good for deep sky, easy to sag, lens expensive
What is a reflecting telescope and its pros/cons?
A telescope that uses 1 lens and 2 mirrors (1 plane, 1 concave) (Concave to plane to eyepiece lens)
Pros: Good for deep sky, easy, low cost
Cons: Prone to optic damage, constant alignment
What is a combination telescope?
A telescope that uses both lens and mirrors (Order: Correcting lens to objective mirror to secondary mirror to eyepiece)
Refractors vs Reflectors
Refractors can give better images when having the same diameter as a reflector, but a reflector can be made much bigger
What are radio telescopes, who invented them, and what do they do?
- Radio telescopes use radio waves to see through dust clouds optical telescopes cannot (Computers colour the data to produce images)
- Invented by Karl Jansky+Grote Reber in 1930s
- Images have less quality than opticals but can be used any time
What are arcseconds and arcminutes?
(NOT ACTUAL TIME) 1/3600th of 1 degree = 1 arcsecond, 1/60th of 1 degree = 1 arcminute
How to calculate magnification for a refracting telescope?
Magnification = objective focal length / eyepiece focal length
What is interferometry?
The technology of connecting two or more telescopes to unite into producing 1 whole image that is AS GOOD AS IF THE TELESCOPE HAD THE DIAMETER OF THE DISTANCE BETWEEN THE TWO
e.g. Mauna Kea Twin Keck Optical Telescopes (reflective) and Karl G. Jansky VLA (25 radio telescopes in Y formation)
What is very long baseline interferometry (VLBI)?
Using non-wired radio telescopes + space telescopes (far away) to mimic the function of a massive telescope larger than Earth
(Much better than optical)
What are ground based telescopes and their pros/cons?
Telescopes built on the ground. They are usually in highly elevated areas.
- Can be connected together
- Cheaper
- Easier to maintain/upgrade
- Not as clear as space based
E.g. Gran Telescopio Canary Islands (10.4m reflective), Mauna Kea, Karl G. Jansky, etc.