0% found this document useful (0 votes)
4 views9 pages

Science 12.1

The document provides an overview of the solar system, detailing its components including the sun, planets, moons, asteroids, meteoroids, and comets. It describes the structure of the sun, the characteristics of each planet, and the formation of the solar system from nebulas to planetesimals. Additionally, it highlights the various small solar system objects and their classifications.
Copyright
© © All Rights Reserved
We take content rights seriously. If you suspect this is your content, claim it here.
Available Formats
Download as DOCX, PDF, TXT or read online on Scribd
0% found this document useful (0 votes)
4 views9 pages

Science 12.1

The document provides an overview of the solar system, detailing its components including the sun, planets, moons, asteroids, meteoroids, and comets. It describes the structure of the sun, the characteristics of each planet, and the formation of the solar system from nebulas to planetesimals. Additionally, it highlights the various small solar system objects and their classifications.
Copyright
© © All Rights Reserved
We take content rights seriously. If you suspect this is your content, claim it here.
Available Formats
Download as DOCX, PDF, TXT or read online on Scribd
You are on page 1/ 9

12.

1 Solar System objects


UNDERSTANDING THE SOLAR SYSTEM
Vocabs

Solar system: consists of the sun, the planets, their moons, and a variety of smaller objects

Astronomical unit: distances between objects in the solar system.

1 AU = 150,000,000 km, from the center of the sun to the center of the Earth

Sun:

 is a star with gaseous body


 contains no solid surface
 about ¾ of the sun’s mass is hydrogen
 about ¼ is helium

Planet: is round, orbits around the sun, has cleared out the region of the solar system along its orbit

Moon:

 Earth’s natural satellite


 A celestial body in orbit

Asteroids: small, rocky bodies

Meteoroids: chunks of rock or dust, smaller than asteroids

Comets:

 loose balls of ice and rock


 have very long and narrow orbits
 develop tails as they orbit the sun
STRUCTURE OF THE SUN
Vocabs

Plasma: a very hot fluid-like gas consisting of electrically charged particles

Convection zone:

 the outermost layer of the sun’s interior


 Plasma heated by the radiative zone rises up to the surface
 Cooling plasma at the surface -> plasma contracts and sinks -> convection loops

Radiative zone: Most heat flows through as forms of electromagnetic radiation

Core: The sun produces an enormous amount of energy here

Nuclear fusion:

 The sun’s energy is produced through nuclear fusion


 Hydrogen atoms are forced together in the core
 Extreme temperature and pressure -> create helium atoms

Photosphere:

 the sun’s inner atmosphere


 Plasma in this layer is dense enough to be visible and directly observed

Chromosphere:

 Middle layer of the sun’s atmosphere


 Reddish glow -> “color sphere”

Corona:

 The outer layer of the sun’s atmosphere


 White halo around the sun
 Extend into space for millions of kilometers
 Gradually thins into streams of electrically charged particles (solar wind)

Sunspot:

 areas of plasma on the sun that are cooler than the plasma around them
 Cooler plasma gives of less light -> dark spots

Prominence:

 huge loops of plasma that are polarized


 Particles following these magnetic forces flow out and back on the sun’s surface

Solar Flare:

 The eruptions of prominence (plasma loops)


 Loops in the sunspot regions connects, release large amounts of magnetic energy -> heat plasma
up to millions of degrees Celsius -> the eruption
PLANETS AND MOONS
Mercury:

 Closest planet to sun (.39 AU)


 Smallest planet (4,879 km diameter)
 Has no moons
 If you weighed 100kg on earth, you would weight 38kg on mercury
 1 day on mercury = 59 earth days
 1 year mercury = 88 days
 At night: -170°C
 During the day: 430°C
 Has no atmosphere

Venus:

 Almost same size as Earth (12,103 km diameter)


 90% Earth’s gravity
 1 venus day = 243 Earth days
 1 year = 225 days
 Has no moons
 2nd closest planet to sun (.72 AU)
 Had oceans billions of years ago
 Today, venus has an atmosphere that is 96.5% carbon dioxide (CO2)
 Thick atmosphere -> the air pressure at its surface is 92 times of Earth
 High CO2 levels make a very strong greenhouse effect -> venus is very hot
 Average temperature is 462°C
 Its surface is mostly flat lava plains and volcanoes
 Has a crust, mantle, and core
 The brightest object in the night sky after the moon

Mars:

 4th planet from the sun (1.52 AU)


 About half the size of Earth (6,792 km diameter)
 Gravity is about 38% as strong as Earth’s gravity
 1 day on Mars = 24.6 hours
 1 year = 687 days
 Has 2 small moons
 Atmosphere is 95% CO2, 100 times thinner than Earth’s atmosphere
 Has weather like dust storms
 Average temperature = -60°C in winter
 Near the poles, temperature = - 125°C
 Has seasons due to its tilted axis
 Some of mar’s surface features were formed by water
 Used to have oceans and still have sub surface water and ice
 Sedimentary rocks only form in the presence of water.
 Some of Mars’ surface features were formed by volcanism (and may still be)
 Mars has the solar system’s largest volcano. Olympus mons is 22 km tall
 Mars has one of the solar system’s largest valleys. Valles Marineris is 4000 km.Long, 200
km.wide and 7 km.deep
 Some of Mars’ surface features by impacts from space.
 We know a lot about mars because we have sent many probes and landers there.

Jupiter

 Jupiter is the 5th planet from the sun (5.2 AU)


 Jupiter’s diameter is 11 times wider than Earth (142,800 km diameter)
 Jupiter has no surface to stand on, but if you could stand on the surface Jupiter’s gravity would
be 2.4 times stronger than earth’s
 Jupiter’s day is 9.9 hours long. it spins at 43,000 km/h
 1 year on Jupiter is 12 Earth years.
 Jupiter has 95 moons.
 The 4 largest moons are known as the Galilean moons (discovered by Galileo and his telescope).
 Scientists believe Ganymede, Callisto and Europa all have oceans under the ice and could have
their own forms of life.

 Io Has active volcanoes. Its yellow color comes from sulfur.


 Callisto is covered in ice and most likely has a liquid salt water ocean.
 Ganymede is covered in ice and most likely has a liquid salt water ocean.
 Europa is covered in ice and most likely has a liquid salt water ocean.
 Jupiter’s outer layers are hydrogen (90%) and helium (10%) gas
 Jupiter’s inner layers are metallic hydrogen
 The temperature in the clouds of Jupiter is about minus 145 degrees Celsius.
 The temperature near the core may be about 50,000 degrees Celsius.

Saturn

 Saturn is a gas giant. A planet made mostly of gas, Unlike the inner planets which are rocky.
 All the outer planets have rings, including Saturn.
 Saturn is the 6th planet from the sun (9.6 AU)
 Saturn’s diameter is about 120,000 km.
 Saturn has no surface to stand on, but if you could stand on Saturn, it’s gravity would be 7%
stronger than earth’s. Saturn is big but not very dense.
 Saturn’s density is actually less than water, which means it would float.
 Saturn’s atmosphere is made of mostly hydrogen gas with a smaller amount of helium gas.
 Saturn's average temperature varies from about - 185°C to -122°C
 The core could be as hot as 11,700 c.
 Saturn’s day is 10 hours 39 minutes long. it spins at 35,500 km/h
 1 year on Saturn is 29 Earth years.
 Saturn has 62 moons.
 Titan has a thick atmosphere that makes it hard to see the surface.
 Titan has methane rain, rivers, lakes and oceans.
 These rocks on titan’s surface are made of water ice.
 Enceladus Is covered in ice and we see very few craters which means the surface of the moon is
young.
 The plumes were water vapor coming from Enceladus’s liquid ocean.
 minerals and chemicals that come from hydrothermal vents on the bottom of the ocean.
 Saturn’s rings are one of the most distinct features in the solar system.
 Saturn’s rings are made of many small particles, ranging in size from micrometers to meters.
 The ring particles are made almost entirely of water ice, with a small amount of rocky material.
 Earth has hydrothermal vents on its ocean floor also.
 On earth the vents provide chemical and heat energy for bacteria, shrimp, crabs and worms.

Uranus and Neptune

 Are ice giants. They have atmospheres similar to Jupiter and Saturn but have more ices (water,
ammonia and methane).
 All the outer planets have rings, including Uranus and Neptune.
 Uranus is the 7th planet from the sun (19.2 AU)
 Uranus’s diameter is about 50,724 km.
 Neptune's diameter is about 49,244 km.
 If you weigh 100 kg. on earth, you would weigh 86 kg. on Uranus and 110 kg. on Neptune.
 Uranus and Neptune both have atmospheres made mostly of hydrogen gas with a smaller
amount of helium gas. They both have layers of ices and rocky cores.
 Uranus's average temperature is -224°C. Uranus’s core is about 5,000°C.
 Neptune is warmer, with an average temperature is -214°C. Neptune’s core is about 7,000°C.
 Uranus’s day is 17 hours 14 minutes long. it spins at 9,320 km/h
 Neptune’s day is 16 hours 6 minutes long. it spins at 9,650 km/h
 1 year on Uranus is 84 Earth years.
 Uranus is tilted 98 degrees off axis and basically rolls around the sun.
 1 year on Neptune is 165 Earth years.
 Uranus has 27 moons
 Neptune has 14 moons
 Neptune’s moon triton is geologically active. ITS SURFACE is young with very few craters.

SMALL SOLAR SYSTEM OBJECTS

• Dwarf planet

• Trans Neptunian object (Kuiper belt objects)


• Asteroid

• Asteroid belt

• Meteoroid

• Meteor

• meteorite

• Comet

• Oort cloud

• Kuiper belt

• There are many (many) objects in the solar system that are smaller than planets.

• Asteroids are rocky or metallic objects often found in the asteroid belt, between the orbit of
mars and Jupiter.

• Smaller pieces of rock in space are called meteoroids.

• Sometimes meteoroids enter earth’s atmosphere and burn up making a streak of light. These
are called meteors.

• If a meteoroid reaches earth’s surface it’s called a meteorite.

• Comets are loose collections of frozen gases and dust.

• Comets usually come from the Kuiper belt or the oort cloud.

• the oort cloud Is a giant spherical shell of icy objects that surrounds our solar system.

• The oort cloud may contain billions or trillions of comets. It is 50,000 to 100,000 AU from the
sun.

• Dwarf planets are rounded by gravity but don’t have their own orbits.

• Dwarf planets are also known as trans Neptunian objects or Kuiper belt objects.
SOLAR SYSTEM FORMATION

• Nebula

• Protoplanetary disk

• Protostar

• Nuclear Fusion

• planetesimals

 Clouds of gas and dust in space are called nebulas.


 Nebulas can form when stars explode
 Some nebulas are leftovers from the early universe.
 Stars are formed in nebulas.
 This flat rotating disk of materials is known as a protoplanetary disk.
 A Protostar is a young star that has not started nuclear fusion yet.
 Nuclear fusion is how the sun produces energy.
 Planetesimals are 0bjects formed from dust, rock, and other materials. They can be as small as
a couple of meters or as large as hundreds of kilometers.

You might also like