Guiding Question: In what ways can the solar system be explored?
A medium-sized star; provides light and heat
Inner Planets (rocky): Mercury, Venus, Earth, Mars
Outer Planets (gas/ice giants): Jupiter, Saturn, Uranus, Neptune
Pluto, Eris, Ceres
Rock fragments (mostly in the asteroid belt between Mars & Jupiter).
Ice & dust; tails form when near Sun.
Smaller rocks in space → become meteors when entering Earth’s atmosphere.
Celestial bodies differ in size, shape, composition, atmosphere, and temperature.
Some emit light (Sun), others reflect (planets, moons).
Scientists often use models to understand or visualize things that are too large, small, or distant to study directly.
For the solar system, models help us picture:
the Sun and the planets,
their relative sizes,
their order and orbits around the Sun.
We can’t show both size and distance perfectly in one convenient model—if planet sizes look right, distances are too short, and vice versa.
Orbits shown in neat circles are really slightly elliptical.
Planets don’t line up; they constantly move.
Models can’t easily display the tilt of rotation axes, moons, or atmospheric features to true scale.
Despite these limits, good models help us see patterns—like the order of planets, asteroid belt position, and the difference between inner rocky and outer gas planets.
Telescopes: gather light to view distant objects.
Satellites: objects orbiting Earth or other planets (can be natural or artificial).
Probes: unmanned spacecraft (Voyager, New Horizons).
Rovers: move on planets’ surfaces (e.g., Curiosity on Mars).
Manned spacecraft: astronauts explore, e.g., Artemis 2!
ISS: orbiting research station.
Ex‑Alta 1: Alberta’s first satellite, launched 2017.