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SSA Review # 1 - Astronomy

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Presentation on theme: "SSA Review # 1 - Astronomy"— Presentation transcript:

1 SSA Review # 1 - Astronomy

2 Universe - Space and all of the matter and energy that is in it.

3 UNIVERSE GALAXY STARS SOLAR SYSTEMS PLANETS

4 *Galaxy – a massive system of stars (billions), gases, dust, and other matter held together by a central gravitational force

5 Spiral Elliptical Irregular

6 *Stars – large spherical(round) bodies composed of gas (H, He) and gives off light
The Sun Sirius Betelgeuse Aldebaran Regulus

7 *Solar System – a central star with planets and other small objects orbiting it

8 *Planet – a spherical body that orbits a star

9 Measuring Distances in the Universe

10 *Astronomical Unit (AU’s) – the distance from Earth to the Sun
--used to measure distances in the Solar System

11 *Light year – the distance light travels through space in 1 year of time (measures distances in the rest of the Universe) From Earth to stars The size of galaxies From galaxy to galaxy

12 Size of Stars

13 *The color of a star indicates its temperature
Blue (Hottest) Red (Coolest)

14 *Apparent Magnitude - How bright a star appears to be from Earth
The Sun 26.8 Sirius -1.46 Vega +0.03 Betelgeuse +0.5 *The smaller the number (value), the brighter the star appears

15 *Absolute Magnitude (Luminosity) – How bright a star actually is
Apparent Magnitude Absolute Magnitude The Sun 26.8 +4.8 Sirius -1.46 +1.2 Vega +0.03 +0.6 Rigel +0.12 -8.1 Betelgeuse +0.5 -7.2 *The smaller the number (value), the brighter the star actually is

16 Models of the Solar System

17 *Geocentric Model – Earth in the center

18 *Heliocentric Model – Sun in the center

19 Structure of the Sun Core where energy is produced through the process of fusion

20 Structure of the Sun Convective Zone – Energy moves to the surface by convection currents

21 Structure of the Sun the visible surface of the sun
Photosphere the visible surface of the sun Structure of the Sun *approx 300 miles thick *takes 8 minutes for light to reach the Earth

22 The Sun’s Rotation – Differential Rotation
*Different parts of the sun rotate at different rates of speed (the sun is a ball of gases , not solid like the Earth

23 SOLAR ACTIVITY Solar Flare an explosive burst of energy extending out from the sun *appears as very bright spots on the photosphere *Similar to a volcanic eruption on Earth

24 SOLAR ACTIVITY Prominence huge loops of gases extending out from the sun *many Earths could fit inside one

25 SOLAR ACTIVITY Sunspots dark areas that form on the sun’s surface
*cooler regions of the photosphere caused by a change in the sun’s magnetic field

26 *How does solar activity affect conditions on Earth?
*Solar flares can affect satellites, astronauts, GPS systems, jet airplanes, and electrical systems and devices on Earth.

27 1 - Inner Planets (Terrestrial) *Small *Rocky *Thin atmospheres *Closer to the Sun

28 *Fast rotational period
2 - Outer Planets (Gas Giants) *Large *Thick, gaseous atmospheres (hydrogen & helium) with a solid core *Fast rotational period *Many moons and rings *Farther away from the Sun (colder)

29 1. Dwarf Planet *A round object that orbits the Sun, but has other objects that cross its orbit PLUTO

30 2. Natural Satellites (Moons)
*A round object that orbits a planet *Why does Jupiter and Saturn have so many satellites? *They have a stronger gravitational pull on objects

31 3. Asteroids *Chunks of rocks & metal orbiting the Sun

32 5. Comets *An icy body that releases glowing gases as it orbits close to the Sun Coma Tail

33 What is the universal force that hold galaxies together, caused a nebula to collapse inward and flatten into a disk that eventually formed our solar system, and keeps objects in orbit around other objects? Gravity


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