Unit E: Science Exploration

Things in space

Nebula

  • Nebulae are accumulations of gas and dust in space

  • the attraction of particles causes the nebula to start collapsing into a small, rotating cloud

  • If the core gets hot enough, it will start to glow. This is called a protostar, the first stage in a star’s formation

  • soon it becomes hot enough to achieve fusion, creating a star

Star

  • A star is a hot, glowing ball of gas (mainly hydrogen) that gives off a ton of light energy

  • The colour of a star depends on its surface temperature. Very hot stars look blue. Cooler stars look red.

Constellation

  • Constellations are grouping of stars we see as patterns in the night sky There are 88 rexognized constellations

  • Ex. Big dipper, Orion, and Virgo

Planet

  • Ancient people knew about 5 planets: Mercury, Venus, Mars, Jupiter, and Saturn (that’s all they could see and Earth wasn’t included becasue they believed it was the centre of the universe)

  • Planet- means “wanderer” in Greek

  • Over time, each planet moves in a weird way. This is called retrograde (the path a planet takes), but it’s just an optical illusion.

  • In contrast, the stars move in a perfect circle

Moon

  • The moon is a natural satellite that obrits a planet

  • Our moon moves from east to wast across the skiy. This movement is called the ecliptic

  • The moon had phases. It takes 28 days ti complete a cycle

Black hole

Solar wind and the Sun

  • solar wind is charged particles released by the sun in every direction

  • Earth is protected by solar wind with its magnetic field

  • solar wind is known as the aurora borealis

  • sunspots are spots on the sun that are darker. This is a result of the sun’s magnetic field that prevents heat from flowing to the surface

The Planets

  1. Mercury- closest to the sun

  2. Venus- the hottest planet

  3. Earth -the only planet that can sustain life

  4. Mars- - the red planet( from rust- iron III oxide)

  5. Jupiter- the largest planet

  6. Saturn- rings

  7. Uranus- tilted axis

  8. Neptune'

  9. (not really) Pluto- classified as a planetoid

Inner planets

  • The first 4 planets

  • smaller, rockier in composition, and closer to the sun that the Jovian planets

Outer planets (Jovian-Jupiter)

  • large, gaseous, and located great distance from the sun

The Protoplanet Hypothesis

The “protoplanet hypothesis” is a model for explaining the birth of solar systems. The process can be described in three steps:

1. A cloud of gas and dust in space begins swirling.

2. Most of the material (more than 90%) accumulates in the center, forming the Sun.

3. The remaining material accumulates in smaller clumps circling the center. These form the planets

Eclipses

  • A solar eclipse is when the moon, passing between the sun and the earth, casts a shadow on earth

  • A lunar eclipse occurs when Earth passes between the Sun and the Moon, casting its shadow over the Moon

Asteroids, Comets, and Meteors

  • Asteroids are belts of small rocky or metallic bodies travelling in space

  • Majority of them are found between the orbits of Mars and Jupiter

  • Comets are objects made of dust and ice. They are pushed by solar wind and their tails glow when they get close to the sun

  • Meteoroids are small or big pieces of rocks flying through space with no paticular path

  • A meteriod becomes a meteor when its pulled into the Earths atmoshphere and the the ifrsction causes it to give off light

  • A meteor becomes a meteorite when it hits Earth’s surface

Solstices and Equinoxes

  • Winter solstice- December 21st (shortest day)

  • Vernal equinox- March 21st (halfway to summer)

  • SUmmer equinox- June 21st (longest day)

  • Autumnal equinox- September 21st (halfway to winter)

Early Views of Space

The geocentric model of the universe

  • The arth is at the center of the universe

  • Every orbit is a perfect circle

  • This was the model of Airistotle, ptolemy, and pythagoras

  • it was believed that there was a dome of stars enclosing our solar system

The heliocentric model of the universe

  • Sun at the center

  • every orbit is eliptical (oval)

  • This was the model of Coppernicus, Galileo. Kepler, and Newton

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  • Gailieos observations (and the conclusions he made)

  1. Craters on the moon- celestial bodies are not perfect

  2. Sunspots- the sun turns of its axis so maybe the earth does too.

  3. Moon orbiting jupiter- not everything revolves around the earth

  4. Phases of venus- venus orbits the sun so maybe the earth does too

Defending heliocentricity

  • Galieo used his observations to defend copernicus’ theory

  • The main point- celestial bodies (like earth) can orbit other celestial bdies

  • followed by two astronomers Tycho Brahe and Johannes Kepler

Kepler’s Laws (techically Brahe’s, his teacher)

  1. Planets move in elliptical orbits

  2. The closer to the sun a planet is, the faster it will move

Discoveries

The Atronomical Unit

  • 1 A.U = the distance between teh Earth and the Sun = 150,000,000 km

The Light Year

  • 1 light year = the distance that light travels in a year = 9,460,728,000km= 63,240 A.U

  • Speed of Light = 299,792 km/sec

  • It takes 8 minutes fro light to travel from the Sun to the Earth

Astronomer tools

  • Astrolabe- measured altitude

  • cross-staff- measure the angle bewtween the moon nand any given star

Positions of Objects in Space

Azimuth

  • Azimuth is direction(degrees)

  • North = 0 degrees

  • East = 90 degrees

  • South = 180 degrees

  • West = 270 degrees

  • measured with a compass

Finding a celestial body in the sky

  • Altitude is height- horizon = 0 degrees.

  • Zenith (directly overhead) = 90 degrees

Rockets

Compiled of three components

  1. structural components- the rockets itself, engines storage tanks, fins

  2. fuel- liquid oxygen, liquid hydrogen, gasoline

  3. payload- what its carrying- people water, air, food

Soviet Satellites

  • October 4th 1957- first launched satellite, the Sputnik

  • A month later a second space capsule was launched , carrying a small dog named Laika

IMPORTANT DATES TO REMEMBER

  • First satellite- 1957

  • Went to the moon and back-1969

Cool stuff

Microgravity- the condition which the gravitational forces are greatly reduced

Space shuttles- rockets used by space until 2011. They were re-usable

Ion drives- engines that use xenon fas instead of chemical fuel, The gas is electrically charged. Pros: lasts a long time and only rewuires a small amount of xenon gas. Cons: weak as hell

Solar sails- used to power spacecrafts. Pros- fast and saves on fuel. Cons- no power outside the solar system

Producing Water and Oxygen

Water- waste water is distlled and the steam is condensed into potable water

Oxygen- electrically electrocute water to seperate the elements. Hyfrogen is thrown overboard and oxygen is kept.

Dangers of Space

Environmental

  • cosmic and solar radiation

  • Extreme hot and cold

  • meteors

Body changes

  • Bones expand

  • visual depth is affected

SATELLITES

Observation

  • What satellites were mostly used for

  • geosynchronous orbit (high orbit)

Remote sensing

  • Low orbit

  • take high resoloution of the earths surface

Communication

  • low to medium orbit

  • Ex. Satellite radio

GPS

  • Global postitioning system

  • geosynchronous (high) orbit

  • requirea t least 4 satellietes to recieve an accurate calculation

Technology made for space used on earth

  • Space food- baby and freeze-dried foods

  • computer robotics- emergency response robots for use in dangerous situations (bombs)

  • Simulation of space environment for space training- VR

    Refracting optical telescopes

  • Optical telescopes uses visible light

  • a refracting telescope had a objective lens that refracts light from the outside

  • as well as an ocular lens that refracts light to the eye

  • When multiple telescopes are used to view n object, it is called inferometry (we do this with our eyes)

    Reflecting telescope

  • Has a primary and secondary mirror that capture light from outside

  • and an eye eyes that refracts light to the eye

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