š 1. Geocentric vs. Heliocentric Models
⢠Geocentric: Earth at the center (supported by Aristotle).
⢠Heliocentric: Sun at the center (proposed by Copernicus, supported by Galileo and Kepler).
šØāš¬ 2. Key Scientists
⢠Aristotle: Believed in geocentric universe.
⢠Copernicus: Proposed heliocentric model.
⢠Galileo: Used telescope, observed moons of Jupiter ā proved heliocentric model.
⢠Kepler: Discovered orbits are elliptical, not circular.
š 3. Ellipse & Ecliptic
⢠Ellipse: Oval shape of planetary orbits.
⢠Ecliptic: The Sunās apparent path through the sky over the year.
šš 4. Equinox vs. Solstice
⢠Equinox: Equal day and night (spring & fall).
⢠Solstice: Longest and shortest days (summer = longest, winter = shortest).
ā 5. Solar Winds
⢠Stream of charged particles from the Sun.
⢠Protected by: Earthās magnetic field and atmosphere.
š§® 6. Astronomical Unit (AU)
⢠1 AU = 149,599,000 km ā Distance from Earth to Sun.
š 7. Celestial Objects
⢠Stars: Glowing spheres of gas.
⢠Constellations: Patterns of stars.
⢠Galaxy: Group of stars, gas, dust held by gravity (e.g., Milky Way).
⢠Solar System: Sun + planets + moons + other objects orbiting it.
ā 8. Life Cycle of a Star
⢠Nebula ā Protostar ā Main Sequence ā Red Giant ā Supernova ā Neutron Star / Black Hole.
š 9. Hertzsprung-Russell Diagram
⢠Graphs stars by brightness (luminosity) vs. temperature (color).
šŖ 10. Inner vs Outer Planets
⢠Inner (Terrestrial): Mercury, Venus, Earth, Mars ā small, rocky.
⢠Outer (Jovian): Jupiter, Saturn, Uranus, Neptune ā large, gaseous.
š 11. Light-Year
⢠Distance light travels in a year = 9.5 trillion km.
š§ 12. Azimuth & Altitude
⢠Azimuth: Compass direction (N = 0°, E = 90°, S = 180°, W = 270°).
⢠Altitude: Angle above the horizon (0° = horizon, 90° = overhead).
ā 13. Space Rocks
⢠Asteroid: Rock in space (main belt between Mars & Jupiter).
⢠Comet: āDirty snowball,ā ice and dust, has a tail.
⢠Meteoroid: Small rock in space.
⢠Meteor: Meteoroid burns in Earthās atmosphere.
⢠Meteorite: Lands on Earth.
š 14. Space Technology
⢠Space shuttle: Reusable spacecraft.
⢠Space probe: Unmanned; collects data (e.g., planet atmospheres).
⢠Space station: Human habitat for long missions (e.g., ISS).
šØ 15. Rocket Propulsion
⢠Rockets use Newtonās 3rd Law: For every action, thereās an equal and opposite reaction.
⢠Burn fuel ā gas pushed out ā rocket moves up.
š° 16. Launch Milestones
⢠Sputnik (1957): First artificial satellite (USSR).
⢠Anik 1 (1972): Canadian communications satellite.
⢠ISS (1998+): International Space Station launched and assembled in stages.
šŖ 17. Gravity & Microgravity
⢠Gravity: Force pulling objects toward each other.
⢠Microgravity: Very weak gravity in orbit ā bones weaken, muscles shrink, fluids shift.
š 18. Satellites & Remote Sensing
⢠Satellites: Orbit Earth; used for weather, communication, GPS.
⢠Remote sensing: Observing Earth without direct contact (e.g., weather, land use).
š 19. GPS
⢠Uses satellites to pinpoint location on Earth using triangulation.
š 20. Telescopes
⢠Optical:
⢠Refracting: Uses lenses.
⢠Reflecting: Uses mirrors ā clearer images.
⢠Radio:
⢠Uses radio waves.
⢠Works in any weather/day or night.
š 21. Hubble Space Telescope
⢠Launched in 1990.
⢠Orbits Earth, takes clear images (above the atmosphere).
š 22. Spectroscope
⢠Analyzes light spectrum from stars ā determines elements in stars.
š 23. Triangulation
⢠Measure angles from 2 points to find distance.
⢠Wider baseline = more accuracy.
šØāš 24. Space Suits
⢠Provide:
⢠Oxygen
⢠Pressure
⢠Temperature control
⢠Protection from radiation
ā» 25. Space Junk
⢠Debris from satellites, rockets.
⢠Risks: Damage to spacecraft and satellites.
š 26. Parallax
⢠Object appears to shift position when viewed from different places.
⢠Used to measure distances to nearby stars.
š° 27. Pros and Cons of Space Exploration
Pros:
⢠New tech (GPS, materials)
⢠Scientific knowledge
⢠Global cooperation
Cons:
⢠High cost
⢠Space junk
⢠Risks to astronauts