introducing: the solar system!
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Introducing: The solar system!. Our Home. Our home. The solar system is where we reside. Our only home – earth, is but a small speck among the myriad objects that make up the solar system Our curiosity has taken us far into the reaches of the solar system, but only remotely. - PowerPoint PPT PresentationTRANSCRIPT
Our Home.
• The solar system is where we reside. Our only home – earth, is but a small speck among the myriad objects that make up the solar system
• Our curiosity has taken us far into the reaches of the solar system, but only remotely.
• Though it is infinitely tiny compared to our galaxy, and especially the universe, we continue to explore and discover new things about our solar system every day.
• The Solar System consists of the Sun and the astronomical objects gravitationally bound in orbit around it.
• Formed from the collapse of a giant molecular cloud approximately 4.6 billion years ago. (protostar formation)
• Edge of the solar system sometimes defined as where the solar wind stops. (Heliopause) This is about 100 A.U. from the sun
• Furthest known objects may extend to 50,000 A.U. (1 light-year) from the sun.
• Estimated boundary of the suns gravitational dominance is about 2 light-years.
• Remember, the closest star, Alpha Centauri, is 4.3 light years away.
• Inner solar system
• From the sun to the Asteroid Belt
• 0 – 5 A.U.
• Asteroid Belt
• ~5 A.U. Contains 25,000,000+ asteroids
• Outer solar system
• From Jupiter to Neptune
• 5 – 30 A.U.
• Kuiper Belt
• Beyond Neptune, includes Pluto
• 30 – 50 A.U. from the sun
• Oort cloud
• Beyond the Kuiper Belt
• 2000 – 50,000 A.U. ( 1 light-year)
• (Greek "wandering star") A celestial body orbiting a star or stellar remnant
• Massive enough to be rounded by its own gravity,
• Not massive enough to cause thermonuclear fusion.
• Has cleared its neighboring region of planetesimals.
• A celestial body that orbits a planet or smaller body, which is called its primary.
• A moon can orbit a Planet, minor planet, or dwarf planet.
Between the meteorites and the moons.
• A celestial body orbiting the Sun
• Massive enough to be spherical as a result of its own gravity
• Has not cleared its neighboring region of planetesimals
• Is not a satellite (does not orbit another planet).
• 5 currently recognized by the IAU: Ceres, Pluto, Haumea, Makemake, and Eris.
• 50 – 200 other current candidates.
• No true formal definition
• Tends to refer to minor planets within the inner solar system, larger than 10 km diameter.
• Can also be referred to as Planetoid or “Small Solar System Object”
• ANY object that is part of the solar system and beyond the orbit of Neptune.
• Kuiper Belt:
• Objects from 30 – 50 A.U. (KBO = Kuiper Belt Object)
• Primarily Icy, with frozen volatiles (methane, ammonia, etc.)
• Scattered Disc:
• Sparse collection of larger TNOs, beyond the Kuiper Belt
• Similar in composition to Kuiper Belt Objects
• It is now believed that most comets originated from this region.
• Oort Cloud:
• Farthest reaches of the solar system
• Spherical in structure, instead of flat, disc shaped regions
Boulders to Dust
• Highly eccentric orbits
• Believed to originate from the scattered disc
• Many come from the Kuiper Belt or Oort Cloud as well.
• Can range from “Icy mudball” to “dirty snowball” in composition.
• sand to boulder-sized particle of debris in the solar system
• Ranges from icy to rocky to metallic
• When it enters the earth’s atmosphere it becomes a METEOR
• Once it lands on the surface of the earth, it becomes a METEORITE