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    Space Science and Environment

    Dr. Ugur GUVEN

    Aerospace Engineer (PhD)Nuclear Engineer (MSc)

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    Definition of Space

    Legal definition ofspace starts around100 miles (160 km)

    Up to 1000 Km ofaltitude, the effectsof molecular flowand drag can be felton spacecraft.

    Above 1000 km,microgravity

    conditions exist.

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    Space Science Distance Definitions

    One Astronomical Unit (AU),

    is the distance from the Sunto the Earth. It is149,597,870.7 kilometers(92,955,807.3 mi).

    One Light Year (ly) is thedistance that light travels invacuum in one year. Equal to

    101015

    meters=63.24103 AU

    Parsec (pc) is equal to 3.26light years (3.11013) km. It is

    206,265 AU

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    Brightness Measurement Units

    The apparent magnitude (m) of a celestial body is a

    measure of its brightness as seen by an observer on

    Earth, adjusted to the value it would have in the

    absence of the atmosphere. The brighter the object

    appears, the lower the value of its magnitude.

    Absolute Magnitude (M) is the apparent

    magnitude a star would have if it were 32.6 light

    years (10 parsecs) away from Earth

    Luminosity is the amount of electromagnetic

    energy a body radiates per unit of time

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    Brightness Distance Equations

    is the Stefan-Boltzmann constant 5.67108Wm-2K-4

    temperature Tand radius R of the star

    d in parsecs

    http://en.wikipedia.org/wiki/Stefan-Boltzmann_constanthttp://en.wikipedia.org/wiki/Watthttp://en.wikipedia.org/wiki/Watthttp://en.wikipedia.org/wiki/Stefan-Boltzmann_constanthttp://en.wikipedia.org/wiki/Stefan-Boltzmann_constanthttp://en.wikipedia.org/wiki/Stefan-Boltzmann_constant
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    Planet Earth Planet Earth is our first stop in space.

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    Moon Moon is our planets natural

    satellite. It is also the fifthlargest satellite in the SolarSystem. Its properties are:

    - Quarter diameter of the Earth

    1/6 of the gravitational pull

    Its rotation is synchronous(same face toward Earth)

    Perigee :362,570 km Apogee: 405,410 km

    It has no atmosphere or

    magnetic field.

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    Solar System

    Our solar system is a very unique structure with its

    9 planets, inner & outer belts as well as its

    originality in the nearby star systems

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    Solar System The overall structure of the charted regions of the

    Solar System consists of the Sun, four relativelysmall inner planets surrounded by a belt of rocky

    asteroids, and four gas giants surrounded by the

    outer Kuiper belt of icy objects.

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    Sun Sun is the main component of

    our solar system, as all planets,

    plenetoids, comets, meteors,asteroids, moons and otherbodies orbit around it.

    Its 109 times the size of Earth

    75% is Hydrogen, 23.31 % is

    Helium and 1.69% is made upof oxygen, carbon, iron andother elements.

    It works by fusion (convertingHydrogen to Helium) with 620million metric tons of Hydrogenfusing into Helium releasinglight, energy and heat of thesun.

    Sun rotates around the galacticcenter with a period of 225

    million years

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    Mercury Mercury is a planet that is closest to the sun and it is slightly larger than our moon.

    Mercury has a very little atmosphere of escaped atoms due to suns rays.

    It orbits the sun in 88 days and it is scorching hot on the day side and it is freezing

    on the night side.

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    Venus

    Venus is a dim world of intenseheat and volcanic activity

    Similar in structure and size toEarth, Venus' thick, toxicatmosphere traps heat in arunaway "greenhouse effect. As

    a result, The scorched world hastemperatures hot enough tomelt lead.

    Venus orbits the sun in 225 days.

    Venus' atmosphere consistsmainly of carbon dioxide, withclouds of sulfuric acid droplets

    Surface temperature is around

    470 Celsius

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    Mars Mars is a rocky planet with half

    the size of Earth

    Red appearance of Mars iscaused by abundance of ironoxide.

    Martian atmosphere is about 95

    % of CO2 and 3 % of Nitrogenalong with trace gases.

    The mean pressure is 0.6 kPawhich is less then 1 % of Earthatmospheric pressure (101.3

    kPa) It rotates around the sun in 687

    days.

    Its two moons are Phobos and

    Deimos

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    Jupiter Jupiter is the biggest planet in our

    solar system and it is a gas giant(composed of dense gases)

    It is made up of mostly hydrogenand helium as well as ammonia

    Jupiter has a total of 50 moons withIo, Europa, Ganymede and Callisto asthe larger ones.

    Jupiter has a very powerful magneticfield at least 20,000 times more thenEarth

    It completes an orbit around the sun

    in 11.86 years.

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    Saturn

    It is the second largest planet in the solar

    system. Saturn's interior is probably composed of

    a core of iron, nickel and rock and theouter layer is hydrogen and helium.

    Saturn has a ring system that consists of

    nine continuous main rings and threediscontinuous arcs, composed mostly ofice particles with a smaller amount ofrocky debris

    Saturn has 63 moons with Titan the

    largest. (Titan is the second largest moonand it is the only moon in the SolarSystem with an atmosphere)

    It takes a 29.5 years for Saturn tocomplete one orbit around the sun.

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    Uranus

    Uranus has an atmosphere ofmethane, hydrogen andhelium. It is the methane whichgives it the blue color.

    Like Venus, Uranus rotates eastto west.

    It is an ice giant with two sets

    of rings It has 27 moons with Miranda

    being the famous one.

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    Neptune

    Neptune is an ice giant

    planet. It is 4.5 billion km away

    from the sun and itrotates around the sun in165 years.

    Neptune also has largeamounts of hydrogen,helium and methane infrozen form

    Neptune has a surfacetemperature of -235 Cand it has 13 moons.

    The blue color comesfrom Methane

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    Pluto

    Pluto is a dwarf planet.

    It is fifth of the mass ofEarths moon

    Until 2006 it was a full planet It rotates around the sun in

    248 years

    It consists of rock and ice Temperature is around -230 C

    and its atmosphere consistsof nitrogen, methane and

    carbon dioxide

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    Kuiper Belt Kuiper Belt is the

    outer region ofour solar systemwhich consists ofthousands ofrocks andasteroids

    It consists ofrock, ice andmetal

    Starts at 30 AUand continuesuntil 50 AU

    It contains theremnants of presolar systemformation

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    Oort Cloud

    It is the spherical region around

    the Sun whose radius is about50,000 AU

    Oort Cloud consists of blocks of

    ice of varying shape and sizes.

    Some of these ice blocks move

    toward the inner solar system

    and they will have elongatedorbits to become comets

    The outer layer of Kuiper Belt

    coincides with the Oort Cloud

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    Heliopause

    The heliopause is the

    theoretical boundary wherethe Sun's solar wind isstopped by the interstellarmedium; where the solarwind's strength is no longer

    great enough to push backthe stellar winds of thesurrounding stars

    It is hypothesized that the

    Sun also has a bow shockproduced in its travelswithin the interstellarmedium

    It is about 230 AU away

    from the sun

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    Solar System and Interstellar Space

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    Interstellar Space Interstellar space is the physical

    space within a galaxy notoccupied by stars or theirplanetary systems

    The average density of matter inthis region is about 106 particlesper m3

    Nearly 70% of this mass consists

    of lone hydrogen atoms. This isenriched with helium atoms aswell as trace amounts ofheavier atoms

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    Nearby Star Systems

    The nearest star to our

    solar system is theAlpha Centauri systemwhich is a star systemwith Proxima Centaurias the closest star with

    4.3 light years ofdistance. It would take40,000 years with ourpropulsion technologyto travel there.

    Barnards star is thesecond closest star toour solar system with6 light years of

    distance

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    Milky Way Galaxy

    The Milky Way is a spiral galaxy

    100,000-120,000 light-years indiameter containing 200400billion stars.

    Earth is located within the galacticplane of this disk, around twothirds of the way out from thecenter, on the inner edge of aspiral-shaped concentration of gasand dust called the OrionCygnus

    Arm The galaxy is also moving at a

    velocity of 552 to 630 km persecond

    It is estimated to be about 13.2

    billion years old

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    Other Galaxies

    There are probably more than

    170 billion (1.7 1011) galaxies inthe observable universe

    Elliptical galaxy has an ellipse-shaped light profile. Spiral galaxiesare disk-shaped with dusty, curvingarms. Those with irregular orunusual shapes are known asirregular galaxies and typicallyoriginate from disruption by the

    gravitational pull of neighboringgalaxies.

    Closest galaxy to our galaxy is theAndromeda Galaxy. (2.6 millionlight years)

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    THANK YOU

    [email protected]

    www.aerospacelectures.co.cc

    mailto:[email protected]://www.aerospacelectures.co.cc/http://www.aerospacelectures.co.cc/mailto:[email protected]:[email protected]:[email protected]:[email protected]