SlideShare a Scribd company logo
1 of 25
ASTRONOMY
         OUR UNIVERSE
   A PRESENTATION BY HASSAN
ABDULLAH AND MUJTABA YAR KHAN.
Main Contents
We hope to cover the following topics by the end of this
  class :
 Concept of Astronomy
 Celestial Bodies
 Stars
 Planets
 Rocks in Space
 Black Holes
 Quasars
What is Astronomy ?
Astronomy is the study of the
  sun, moon, stars, planets, comets, gas, galaxie
  s, gas, dust and other non-Earthly bodies and
  phenomena. NASA defines astronomy as “the
  study of stars, planets and space.”
We come to gather that Astronomy is nothing
  but the study of “celestial bodies”.
Celestial Bodies
What are Celestial Bodies ?
The term celestial body is as expansive as the entire
  universe, both known and unknown. By definition
  a celestial body is any natural body outside of the
  Earth’s atmosphere. Easy examples are the Moon,
  Sun, and the other planets of our solar system.
  But those are very limited examples.
  There are plenty of other bodies that still remain
  shrouded in mystery.
Stars – What are they ?
A star is a sphere of gas held together by its
  own gravity. The force of gravity is continually
  trying to cause the star to collapse, but this is
  counteracted by the pressure of hot gas
  and/or radiation in the star's interior. This is
  called hydrostatic support. During most of the
  lifetime of a star, the interior heat and
  radiation is provided by nuclear reactions near
  the center, and this phase of the star's life is
  called the main sequence.
What are Planets ?
 The definition states that a planet is a body that
  orbits the Sun or any other
  star, is massive enough for its own gravity to
  make it round or circle the star, and has
  smaller objects around its orbit.
In our solar system, planets vary a great deal in
  size – smallest starting with a diameter of
  4880 while the biggest with a staggering
  diameter of 142740 km
Planets from our Solar System
 Mercury
 Venus
 Earth
 Mars
 Jupiter
 Saturn
 Neptune
 Uranus
Mercury – the smallest of ‘em all
Mercury is the innermost planet in the Solar System. It is
 also the smallest, and its orbit is the most the least
 perfectly circular of the eight
 planets. It orbits the Sun once in about 88 Earth
 days, completing three rotations about its axis for
 every two orbits.
Mercury's surface is heavily cratered and similar in
 appearance to Earth's Moon, indicating that it has been
 geologically inactive for billions of years. Due to its
 near lack of an atmosphere to retain heat, Mercury's
 surface experiences the steepest temperature gradient
 of all the planets, ranging from a very cold 100 K at
 night to a very hot 700 K during the day.
Venus – the hottest of ‘em all
Venus is the second planet from the Sun, orbiting it every
  224.7 Earth days. After the Moon, it is the brightest
  natural object in the night sky, bright enough to cast
  shadows. Because Venus is an inferior planet from
  Earth, it never appears to venture far from the Sun:
  its elongation reaches a maximum of 47.8°. Venus
  reaches its maximum brightness shortly before sunrise
  or shortly after sunset, for which reason it has been
  referred to by ancient cultures as the Morning Star or
  Evening Star.
Venus is classified as a terrestrial planet and is sometimes
  called Earth's "sister planet" owing to their similar size,
  gravity, and bulk composition.
Earth – the place to live
Earth is the third planet from the Sun, and
  the densest and fifth-largest of the eight planets in
  the Solar System. It is also the largest of the Solar
  System's four terrestrial planets. It is sometimes
  referred to as the world, the Blue Planet, or by its Latin
  name, Terra.
Earth formed approximately 4.54 billion years ago by
  accretion from the solar nebula, and life appeared on
  its surface within one billion years. The planet is home
  to millions of species, including humans and has
  everything to support life on it.
Mars – the red planet
Mars is the fourth planet from the Sun and the second
 smallest planet in the Solar System. It is often described
 as the "Red Planet", as the iron oxide prevalent on its
 surface gives it a reddish appearance. Mars is
 a terrestrial planet with a thin atmosphere, having
 surface features reminiscent both of the impact craters of
 the Moon and the volcanoes, valleys, deserts, and polar
 ice caps of Earth. The rotational period and seasonal
 cycles of Mars are likewise similar to those of Earth, as is
 the tilt that produces the seasons. Mars is the site
 of Olympus Mons, the highest known mountain within
 the Solar System, and of Valles Marineris, one of the
 largest canyons.
Jupiter – biggest of ‘em all
Jupiter, the largest planet in the Solar System, has a
  volume equal to more than 1,000 Earths. The fifth
  planet from the Sun is called a gas giant because
  it has no solid surface, being mainly composed of
  hydrogen and helium. It is believed to have liquid
  metallic hydrogen in its interior that generates
  the planet's intense magnetic field.
Powerful storms such as the centuries-oldGreat Red
  Spot travel in bands across Jupiter. Its many
  satellites include the moons Io,
  Europa, Ganymede and Callisto.
Saturn – the ring planet
Saturn is the sixth planet from the Sun and the second largest planet in
   the Solar System, after Jupiter. Saturn is a gas giant with an average
   radius about nine times that of Earth. While only one-eighth the
   average density of Earth, with its larger volume Saturn is just over
   95 times as massive as Earth.
Saturn's interior is probably composed of a core of iron, nickel and rock
   (silicon and oxygen compounds), surrounded by a deep layer of
   metallic hydrogen, an intermediate layer of liquid
   hydrogen and liquid helium and an outer gaseous layer. The planet
   exhibits a pale yellow hue due to ammonia crystals in its upper
   atmosphere. Electrical current within the metallic hydrogen layer is
   thought to give rise to Saturn's planetary magnetic field, which is
   slightly weaker than Earth's and around one-twentieth the strength
   of Jupiter's. Wind speeds on Saturn can reach 1,800 km/h
   (1,100 mph), faster than on Jupiter, but not as fast as those
   on Neptune.
Uranus – the ice giant
Uranus is the seventh planet from the Sun. It has the
  third-largest planetary radius and fourth-largest
  planetary mass in the Solar System. Though it is visible
  to the naked eye like the five classical planets, it was
  never recognized as a planet by ancient observers
  because of its dimness and slow orbit. Sir William
  Herschel announced its discovery on March
  13, 1781, expanding the known boundaries of the Solar
  System for the first time in modern history. Uranus was
  also the first planet discovered with a telescope.
Uranus is similar in composition to Neptune, and both are
  of different chemical composition than the larger gas
  giants, Jupiter and Saturn. Astronomers sometimes
  place them in a separate category called "ice giants".
Neptune – the windy planet
Neptune is the eighth and farthest planet from the Sun in
  the Solar System. It is the fourth-largest planet by diameter
  and the third-largest by mass. Neptune is 17 times the mass
  of Earth and is somewhat more massive than its near-
  twin Uranus, which is 15 times the mass of Earth but not as
  dense. On average, Neptune orbits the Sun at a distance of
  30.1 AU, approximately 30 times the Earth–Sun distance.
Neptune is similar in composition to Uranus, and both have
  compositions which differ from those of the larger gas
  giants, Jupiter and Saturn. Neptune's atmosphere, while
  similar to Jupiter's and Saturn's in that it is composed
  primarily of hydrogen and helium, along with traces of
  hydrocarbons and possibly nitrogen, contains a higher
  proportion of "ices" such as water, ammonia and methane.
Rocks in Space
Asteroids
Shooting Stars
Meteorite
Comets
Shooting Stars
Shooting star is a common name for
 the visible path of a meteoroid as it
 enters the atmosphere to become a
 meteor.
Also, shooting stars are the glowing
 tails of meteors, which heat up as
 they enter the Earth’s Atmosphere.
Asteroids
Asteroids are a class of small Solar
 System bodies in orbit around
 the Sun. They have also been
 called planetoids, especially the
 larger ones.
Also, asteroids are mini – planets that
 orbit the Sun in a ‘belt’ between
 Mars and Jupiter.
Meteorites
A meteorite is a natural object originating
  in outer space that survives impact with
  the Earth's surface. A meteorite's size can
  range from small to extremely large.
  Most meteorites derive from
  small astronomical
  objects called meteoroids, but they are
  also sometimes produced by impacts of
  asteroids.
Comets
Comets are chunks of ice filled with
 dust and rock that orbit the sun, just
 like planets.
However, comets travel much farther
 out into distant space, often to the
 outer reaches of the Solar System, so
 comets can take up to thousands of
 years to make on orbit of the sun.
Black Holes
A black hole is a region of space time where gravity prevents
   anything, including light, from escaping. The theory
   of general relativity predicts that a sufficiently
   compact mass will deform space time to form a black hole.
   Around a black hole there is a mathematically defined
   surface called an event horizon that marks the point of no
   return. It is called "black" because it absorbs all the light
   that hits the horizon, reflecting nothing, just like a
   perfect black body in thermodynamics. Quantum
   mechanics predicts that black holes emit radiation like a
   black body with a finite temperature. This temperature is
   inversely proportional to the mass of the black hole, making
   it difficult to observe this radiation for black holes of stellar
   mass or greater.
Quasars
The word quasar stands for quasi-stellar
  radio source. They are the brightest and
  most distant objects in the universe as we
  know it. The term quasar has fallen out
  of common use by astronomers and they
  are now known as quasi-stellar
  objects(QSOs) because we now know
  that they are not true stars.
Life of a star




Stars begin life when Nebulae are pulled together by their own gravity.. They get squeezed and begin to get hot. Nuclear fusion begin as Hydrogen
atoms fused together to make Helium. The heat from the fusion makes the Star shine. The heat generated in the core pushes gas out as hard as
gravity pulls in it. After 10 Billion years all the Hydrogen in the Stars core is burned up and it begins to burn Helium.
Then the Star goes on swri;ing into super giants, once Iron forms in the center the Star fails to give energy and collapses that triggers an explosion
like the nuclear bomb which is called super nova.
.Then the Star either turns into a Black hole or a Neutron Star.
Astronomy

More Related Content

What's hot (20)

The Universe
The UniverseThe Universe
The Universe
 
Milky way galaxy
Milky way galaxyMilky way galaxy
Milky way galaxy
 
Solar System
Solar SystemSolar System
Solar System
 
Our milky way
Our milky wayOur milky way
Our milky way
 
Galaxies
GalaxiesGalaxies
Galaxies
 
Astronomy presentation
Astronomy presentation Astronomy presentation
Astronomy presentation
 
Galaxies and stars
Galaxies and starsGalaxies and stars
Galaxies and stars
 
Jupiter
JupiterJupiter
Jupiter
 
Universe ppt 6 B
Universe ppt 6 BUniverse ppt 6 B
Universe ppt 6 B
 
What is Solar system? FORMATION OF SOLAR SYSTEM. SOLAR SYSTEM: Structure
What is Solar system? FORMATION OF SOLAR SYSTEM. SOLAR SYSTEM: StructureWhat is Solar system? FORMATION OF SOLAR SYSTEM. SOLAR SYSTEM: Structure
What is Solar system? FORMATION OF SOLAR SYSTEM. SOLAR SYSTEM: Structure
 
Space Facts for Kids Infographic
Space Facts for Kids InfographicSpace Facts for Kids Infographic
Space Facts for Kids Infographic
 
BASIC SOLAR SYSTEM PRESENTATION
BASIC SOLAR SYSTEM PRESENTATIONBASIC SOLAR SYSTEM PRESENTATION
BASIC SOLAR SYSTEM PRESENTATION
 
Galaxies
GalaxiesGalaxies
Galaxies
 
Galaxies
GalaxiesGalaxies
Galaxies
 
Space
SpaceSpace
Space
 
Stars and Galaxies
Stars and GalaxiesStars and Galaxies
Stars and Galaxies
 
E1 - Introduction to the Universe
E1 - Introduction to the UniverseE1 - Introduction to the Universe
E1 - Introduction to the Universe
 
The universe
The universeThe universe
The universe
 
Our Moon
Our MoonOur Moon
Our Moon
 
The milky way galaxy
The milky way galaxyThe milky way galaxy
The milky way galaxy
 

Similar to Astronomy

The Solar System by VI - Edison (PASAY CITY WEST HIGH SCHOOL, 2012)
The Solar System by VI - Edison  (PASAY CITY WEST HIGH SCHOOL, 2012)The Solar System by VI - Edison  (PASAY CITY WEST HIGH SCHOOL, 2012)
The Solar System by VI - Edison (PASAY CITY WEST HIGH SCHOOL, 2012)Fatimah Sol Jalmaani
 
SOLAR SYSTEM PPT CLASS 8
SOLAR SYSTEM  PPT CLASS 8 SOLAR SYSTEM  PPT CLASS 8
SOLAR SYSTEM PPT CLASS 8 janhvi sabadra
 
Solar system samuel 4_b
Solar system samuel 4_bSolar system samuel 4_b
Solar system samuel 4_bandare2
 
Explain solar system 3 (2)
Explain solar system 3 (2)Explain solar system 3 (2)
Explain solar system 3 (2)maromaher1
 
earthsciencepptx-151128011727-lva1-app6891 (1).pdf
earthsciencepptx-151128011727-lva1-app6891 (1).pdfearthsciencepptx-151128011727-lva1-app6891 (1).pdf
earthsciencepptx-151128011727-lva1-app6891 (1).pdfSer Louis Fabunan
 
Earth science pptx
Earth science pptxEarth science pptx
Earth science pptxsihellyay
 
the solar system
 the solar system the solar system
the solar systemfosters18
 
The solar system and beyound
The solar system and beyoundThe solar system and beyound
The solar system and beyoundPinocoKuro
 
Geography: Module 1: Solar System
Geography: Module 1: Solar System Geography: Module 1: Solar System
Geography: Module 1: Solar System ShashiRanjan230
 
YEAR 9 GEOGRAPHY - ASTRONOMY: SUN, PLANETS AND GALAXY
YEAR 9 GEOGRAPHY - ASTRONOMY: SUN, PLANETS AND GALAXYYEAR 9 GEOGRAPHY - ASTRONOMY: SUN, PLANETS AND GALAXY
YEAR 9 GEOGRAPHY - ASTRONOMY: SUN, PLANETS AND GALAXYGeorge Dumitrache
 

Similar to Astronomy (20)

The Solar System by VI - Edison (PASAY CITY WEST HIGH SCHOOL, 2012)
The Solar System by VI - Edison  (PASAY CITY WEST HIGH SCHOOL, 2012)The Solar System by VI - Edison  (PASAY CITY WEST HIGH SCHOOL, 2012)
The Solar System by VI - Edison (PASAY CITY WEST HIGH SCHOOL, 2012)
 
OUR SOLAR SYSTEM
OUR SOLAR SYSTEMOUR SOLAR SYSTEM
OUR SOLAR SYSTEM
 
OUR SOLAR SYSTEM
OUR SOLAR SYSTEMOUR SOLAR SYSTEM
OUR SOLAR SYSTEM
 
Solar System
Solar SystemSolar System
Solar System
 
SOLAR SYSTEM PPT CLASS 8
SOLAR SYSTEM  PPT CLASS 8 SOLAR SYSTEM  PPT CLASS 8
SOLAR SYSTEM PPT CLASS 8
 
Solar system samuel 4_b
Solar system samuel 4_bSolar system samuel 4_b
Solar system samuel 4_b
 
Explain solar system 3 (2)
Explain solar system 3 (2)Explain solar system 3 (2)
Explain solar system 3 (2)
 
The Universe
The UniverseThe Universe
The Universe
 
Thryu
ThryuThryu
Thryu
 
earthsciencepptx-151128011727-lva1-app6891 (1).pdf
earthsciencepptx-151128011727-lva1-app6891 (1).pdfearthsciencepptx-151128011727-lva1-app6891 (1).pdf
earthsciencepptx-151128011727-lva1-app6891 (1).pdf
 
Earth science pptx
Earth science pptxEarth science pptx
Earth science pptx
 
the solar system
 the solar system the solar system
the solar system
 
Grade 7 SCIENCE
Grade 7 SCIENCEGrade 7 SCIENCE
Grade 7 SCIENCE
 
Solar system 2
Solar system 2Solar system 2
Solar system 2
 
Solar system 2
Solar system 2Solar system 2
Solar system 2
 
Field trip to Solar System
Field trip to Solar SystemField trip to Solar System
Field trip to Solar System
 
The solar system and beyound
The solar system and beyoundThe solar system and beyound
The solar system and beyound
 
Geography: Module 1: Solar System
Geography: Module 1: Solar System Geography: Module 1: Solar System
Geography: Module 1: Solar System
 
Space
SpaceSpace
Space
 
YEAR 9 GEOGRAPHY - ASTRONOMY: SUN, PLANETS AND GALAXY
YEAR 9 GEOGRAPHY - ASTRONOMY: SUN, PLANETS AND GALAXYYEAR 9 GEOGRAPHY - ASTRONOMY: SUN, PLANETS AND GALAXY
YEAR 9 GEOGRAPHY - ASTRONOMY: SUN, PLANETS AND GALAXY
 

Recently uploaded

Key note speaker Neum_Admir Softic_ENG.pdf
Key note speaker Neum_Admir Softic_ENG.pdfKey note speaker Neum_Admir Softic_ENG.pdf
Key note speaker Neum_Admir Softic_ENG.pdfAdmir Softic
 
Holdier Curriculum Vitae (April 2024).pdf
Holdier Curriculum Vitae (April 2024).pdfHoldier Curriculum Vitae (April 2024).pdf
Holdier Curriculum Vitae (April 2024).pdfagholdier
 
Arihant handbook biology for class 11 .pdf
Arihant handbook biology for class 11 .pdfArihant handbook biology for class 11 .pdf
Arihant handbook biology for class 11 .pdfchloefrazer622
 
Web & Social Media Analytics Previous Year Question Paper.pdf
Web & Social Media Analytics Previous Year Question Paper.pdfWeb & Social Media Analytics Previous Year Question Paper.pdf
Web & Social Media Analytics Previous Year Question Paper.pdfJayanti Pande
 
Measures of Dispersion and Variability: Range, QD, AD and SD
Measures of Dispersion and Variability: Range, QD, AD and SDMeasures of Dispersion and Variability: Range, QD, AD and SD
Measures of Dispersion and Variability: Range, QD, AD and SDThiyagu K
 
Disha NEET Physics Guide for classes 11 and 12.pdf
Disha NEET Physics Guide for classes 11 and 12.pdfDisha NEET Physics Guide for classes 11 and 12.pdf
Disha NEET Physics Guide for classes 11 and 12.pdfchloefrazer622
 
BASLIQ CURRENT LOOKBOOK LOOKBOOK(1) (1).pdf
BASLIQ CURRENT LOOKBOOK  LOOKBOOK(1) (1).pdfBASLIQ CURRENT LOOKBOOK  LOOKBOOK(1) (1).pdf
BASLIQ CURRENT LOOKBOOK LOOKBOOK(1) (1).pdfSoniaTolstoy
 
1029-Danh muc Sach Giao Khoa khoi 6.pdf
1029-Danh muc Sach Giao Khoa khoi  6.pdf1029-Danh muc Sach Giao Khoa khoi  6.pdf
1029-Danh muc Sach Giao Khoa khoi 6.pdfQucHHunhnh
 
A Critique of the Proposed National Education Policy Reform
A Critique of the Proposed National Education Policy ReformA Critique of the Proposed National Education Policy Reform
A Critique of the Proposed National Education Policy ReformChameera Dedduwage
 
The Most Excellent Way | 1 Corinthians 13
The Most Excellent Way | 1 Corinthians 13The Most Excellent Way | 1 Corinthians 13
The Most Excellent Way | 1 Corinthians 13Steve Thomason
 
IGNOU MSCCFT and PGDCFT Exam Question Pattern: MCFT003 Counselling and Family...
IGNOU MSCCFT and PGDCFT Exam Question Pattern: MCFT003 Counselling and Family...IGNOU MSCCFT and PGDCFT Exam Question Pattern: MCFT003 Counselling and Family...
IGNOU MSCCFT and PGDCFT Exam Question Pattern: MCFT003 Counselling and Family...PsychoTech Services
 
Grant Readiness 101 TechSoup and Remy Consulting
Grant Readiness 101 TechSoup and Remy ConsultingGrant Readiness 101 TechSoup and Remy Consulting
Grant Readiness 101 TechSoup and Remy ConsultingTechSoup
 
Measures of Central Tendency: Mean, Median and Mode
Measures of Central Tendency: Mean, Median and ModeMeasures of Central Tendency: Mean, Median and Mode
Measures of Central Tendency: Mean, Median and ModeThiyagu K
 
Interactive Powerpoint_How to Master effective communication
Interactive Powerpoint_How to Master effective communicationInteractive Powerpoint_How to Master effective communication
Interactive Powerpoint_How to Master effective communicationnomboosow
 
The basics of sentences session 2pptx copy.pptx
The basics of sentences session 2pptx copy.pptxThe basics of sentences session 2pptx copy.pptx
The basics of sentences session 2pptx copy.pptxheathfieldcps1
 
Ecosystem Interactions Class Discussion Presentation in Blue Green Lined Styl...
Ecosystem Interactions Class Discussion Presentation in Blue Green Lined Styl...Ecosystem Interactions Class Discussion Presentation in Blue Green Lined Styl...
Ecosystem Interactions Class Discussion Presentation in Blue Green Lined Styl...fonyou31
 
Introduction to Nonprofit Accounting: The Basics
Introduction to Nonprofit Accounting: The BasicsIntroduction to Nonprofit Accounting: The Basics
Introduction to Nonprofit Accounting: The BasicsTechSoup
 
Accessible design: Minimum effort, maximum impact
Accessible design: Minimum effort, maximum impactAccessible design: Minimum effort, maximum impact
Accessible design: Minimum effort, maximum impactdawncurless
 
General AI for Medical Educators April 2024
General AI for Medical Educators April 2024General AI for Medical Educators April 2024
General AI for Medical Educators April 2024Janet Corral
 
Q4-W6-Restating Informational Text Grade 3
Q4-W6-Restating Informational Text Grade 3Q4-W6-Restating Informational Text Grade 3
Q4-W6-Restating Informational Text Grade 3JemimahLaneBuaron
 

Recently uploaded (20)

Key note speaker Neum_Admir Softic_ENG.pdf
Key note speaker Neum_Admir Softic_ENG.pdfKey note speaker Neum_Admir Softic_ENG.pdf
Key note speaker Neum_Admir Softic_ENG.pdf
 
Holdier Curriculum Vitae (April 2024).pdf
Holdier Curriculum Vitae (April 2024).pdfHoldier Curriculum Vitae (April 2024).pdf
Holdier Curriculum Vitae (April 2024).pdf
 
Arihant handbook biology for class 11 .pdf
Arihant handbook biology for class 11 .pdfArihant handbook biology for class 11 .pdf
Arihant handbook biology for class 11 .pdf
 
Web & Social Media Analytics Previous Year Question Paper.pdf
Web & Social Media Analytics Previous Year Question Paper.pdfWeb & Social Media Analytics Previous Year Question Paper.pdf
Web & Social Media Analytics Previous Year Question Paper.pdf
 
Measures of Dispersion and Variability: Range, QD, AD and SD
Measures of Dispersion and Variability: Range, QD, AD and SDMeasures of Dispersion and Variability: Range, QD, AD and SD
Measures of Dispersion and Variability: Range, QD, AD and SD
 
Disha NEET Physics Guide for classes 11 and 12.pdf
Disha NEET Physics Guide for classes 11 and 12.pdfDisha NEET Physics Guide for classes 11 and 12.pdf
Disha NEET Physics Guide for classes 11 and 12.pdf
 
BASLIQ CURRENT LOOKBOOK LOOKBOOK(1) (1).pdf
BASLIQ CURRENT LOOKBOOK  LOOKBOOK(1) (1).pdfBASLIQ CURRENT LOOKBOOK  LOOKBOOK(1) (1).pdf
BASLIQ CURRENT LOOKBOOK LOOKBOOK(1) (1).pdf
 
1029-Danh muc Sach Giao Khoa khoi 6.pdf
1029-Danh muc Sach Giao Khoa khoi  6.pdf1029-Danh muc Sach Giao Khoa khoi  6.pdf
1029-Danh muc Sach Giao Khoa khoi 6.pdf
 
A Critique of the Proposed National Education Policy Reform
A Critique of the Proposed National Education Policy ReformA Critique of the Proposed National Education Policy Reform
A Critique of the Proposed National Education Policy Reform
 
The Most Excellent Way | 1 Corinthians 13
The Most Excellent Way | 1 Corinthians 13The Most Excellent Way | 1 Corinthians 13
The Most Excellent Way | 1 Corinthians 13
 
IGNOU MSCCFT and PGDCFT Exam Question Pattern: MCFT003 Counselling and Family...
IGNOU MSCCFT and PGDCFT Exam Question Pattern: MCFT003 Counselling and Family...IGNOU MSCCFT and PGDCFT Exam Question Pattern: MCFT003 Counselling and Family...
IGNOU MSCCFT and PGDCFT Exam Question Pattern: MCFT003 Counselling and Family...
 
Grant Readiness 101 TechSoup and Remy Consulting
Grant Readiness 101 TechSoup and Remy ConsultingGrant Readiness 101 TechSoup and Remy Consulting
Grant Readiness 101 TechSoup and Remy Consulting
 
Measures of Central Tendency: Mean, Median and Mode
Measures of Central Tendency: Mean, Median and ModeMeasures of Central Tendency: Mean, Median and Mode
Measures of Central Tendency: Mean, Median and Mode
 
Interactive Powerpoint_How to Master effective communication
Interactive Powerpoint_How to Master effective communicationInteractive Powerpoint_How to Master effective communication
Interactive Powerpoint_How to Master effective communication
 
The basics of sentences session 2pptx copy.pptx
The basics of sentences session 2pptx copy.pptxThe basics of sentences session 2pptx copy.pptx
The basics of sentences session 2pptx copy.pptx
 
Ecosystem Interactions Class Discussion Presentation in Blue Green Lined Styl...
Ecosystem Interactions Class Discussion Presentation in Blue Green Lined Styl...Ecosystem Interactions Class Discussion Presentation in Blue Green Lined Styl...
Ecosystem Interactions Class Discussion Presentation in Blue Green Lined Styl...
 
Introduction to Nonprofit Accounting: The Basics
Introduction to Nonprofit Accounting: The BasicsIntroduction to Nonprofit Accounting: The Basics
Introduction to Nonprofit Accounting: The Basics
 
Accessible design: Minimum effort, maximum impact
Accessible design: Minimum effort, maximum impactAccessible design: Minimum effort, maximum impact
Accessible design: Minimum effort, maximum impact
 
General AI for Medical Educators April 2024
General AI for Medical Educators April 2024General AI for Medical Educators April 2024
General AI for Medical Educators April 2024
 
Q4-W6-Restating Informational Text Grade 3
Q4-W6-Restating Informational Text Grade 3Q4-W6-Restating Informational Text Grade 3
Q4-W6-Restating Informational Text Grade 3
 

Astronomy

  • 1. ASTRONOMY OUR UNIVERSE A PRESENTATION BY HASSAN ABDULLAH AND MUJTABA YAR KHAN.
  • 2. Main Contents We hope to cover the following topics by the end of this class :  Concept of Astronomy  Celestial Bodies  Stars  Planets  Rocks in Space  Black Holes  Quasars
  • 3. What is Astronomy ? Astronomy is the study of the sun, moon, stars, planets, comets, gas, galaxie s, gas, dust and other non-Earthly bodies and phenomena. NASA defines astronomy as “the study of stars, planets and space.” We come to gather that Astronomy is nothing but the study of “celestial bodies”.
  • 4. Celestial Bodies What are Celestial Bodies ? The term celestial body is as expansive as the entire universe, both known and unknown. By definition a celestial body is any natural body outside of the Earth’s atmosphere. Easy examples are the Moon, Sun, and the other planets of our solar system. But those are very limited examples. There are plenty of other bodies that still remain shrouded in mystery.
  • 5. Stars – What are they ? A star is a sphere of gas held together by its own gravity. The force of gravity is continually trying to cause the star to collapse, but this is counteracted by the pressure of hot gas and/or radiation in the star's interior. This is called hydrostatic support. During most of the lifetime of a star, the interior heat and radiation is provided by nuclear reactions near the center, and this phase of the star's life is called the main sequence.
  • 6. What are Planets ? The definition states that a planet is a body that orbits the Sun or any other star, is massive enough for its own gravity to make it round or circle the star, and has smaller objects around its orbit. In our solar system, planets vary a great deal in size – smallest starting with a diameter of 4880 while the biggest with a staggering diameter of 142740 km
  • 7. Planets from our Solar System  Mercury  Venus  Earth  Mars  Jupiter  Saturn  Neptune  Uranus
  • 8. Mercury – the smallest of ‘em all Mercury is the innermost planet in the Solar System. It is also the smallest, and its orbit is the most the least perfectly circular of the eight planets. It orbits the Sun once in about 88 Earth days, completing three rotations about its axis for every two orbits. Mercury's surface is heavily cratered and similar in appearance to Earth's Moon, indicating that it has been geologically inactive for billions of years. Due to its near lack of an atmosphere to retain heat, Mercury's surface experiences the steepest temperature gradient of all the planets, ranging from a very cold 100 K at night to a very hot 700 K during the day.
  • 9. Venus – the hottest of ‘em all Venus is the second planet from the Sun, orbiting it every 224.7 Earth days. After the Moon, it is the brightest natural object in the night sky, bright enough to cast shadows. Because Venus is an inferior planet from Earth, it never appears to venture far from the Sun: its elongation reaches a maximum of 47.8°. Venus reaches its maximum brightness shortly before sunrise or shortly after sunset, for which reason it has been referred to by ancient cultures as the Morning Star or Evening Star. Venus is classified as a terrestrial planet and is sometimes called Earth's "sister planet" owing to their similar size, gravity, and bulk composition.
  • 10. Earth – the place to live Earth is the third planet from the Sun, and the densest and fifth-largest of the eight planets in the Solar System. It is also the largest of the Solar System's four terrestrial planets. It is sometimes referred to as the world, the Blue Planet, or by its Latin name, Terra. Earth formed approximately 4.54 billion years ago by accretion from the solar nebula, and life appeared on its surface within one billion years. The planet is home to millions of species, including humans and has everything to support life on it.
  • 11. Mars – the red planet Mars is the fourth planet from the Sun and the second smallest planet in the Solar System. It is often described as the "Red Planet", as the iron oxide prevalent on its surface gives it a reddish appearance. Mars is a terrestrial planet with a thin atmosphere, having surface features reminiscent both of the impact craters of the Moon and the volcanoes, valleys, deserts, and polar ice caps of Earth. The rotational period and seasonal cycles of Mars are likewise similar to those of Earth, as is the tilt that produces the seasons. Mars is the site of Olympus Mons, the highest known mountain within the Solar System, and of Valles Marineris, one of the largest canyons.
  • 12. Jupiter – biggest of ‘em all Jupiter, the largest planet in the Solar System, has a volume equal to more than 1,000 Earths. The fifth planet from the Sun is called a gas giant because it has no solid surface, being mainly composed of hydrogen and helium. It is believed to have liquid metallic hydrogen in its interior that generates the planet's intense magnetic field. Powerful storms such as the centuries-oldGreat Red Spot travel in bands across Jupiter. Its many satellites include the moons Io, Europa, Ganymede and Callisto.
  • 13. Saturn – the ring planet Saturn is the sixth planet from the Sun and the second largest planet in the Solar System, after Jupiter. Saturn is a gas giant with an average radius about nine times that of Earth. While only one-eighth the average density of Earth, with its larger volume Saturn is just over 95 times as massive as Earth. Saturn's interior is probably composed of a core of iron, nickel and rock (silicon and oxygen compounds), surrounded by a deep layer of metallic hydrogen, an intermediate layer of liquid hydrogen and liquid helium and an outer gaseous layer. The planet exhibits a pale yellow hue due to ammonia crystals in its upper atmosphere. Electrical current within the metallic hydrogen layer is thought to give rise to Saturn's planetary magnetic field, which is slightly weaker than Earth's and around one-twentieth the strength of Jupiter's. Wind speeds on Saturn can reach 1,800 km/h (1,100 mph), faster than on Jupiter, but not as fast as those on Neptune.
  • 14. Uranus – the ice giant Uranus is the seventh planet from the Sun. It has the third-largest planetary radius and fourth-largest planetary mass in the Solar System. Though it is visible to the naked eye like the five classical planets, it was never recognized as a planet by ancient observers because of its dimness and slow orbit. Sir William Herschel announced its discovery on March 13, 1781, expanding the known boundaries of the Solar System for the first time in modern history. Uranus was also the first planet discovered with a telescope. Uranus is similar in composition to Neptune, and both are of different chemical composition than the larger gas giants, Jupiter and Saturn. Astronomers sometimes place them in a separate category called "ice giants".
  • 15. Neptune – the windy planet Neptune is the eighth and farthest planet from the Sun in the Solar System. It is the fourth-largest planet by diameter and the third-largest by mass. Neptune is 17 times the mass of Earth and is somewhat more massive than its near- twin Uranus, which is 15 times the mass of Earth but not as dense. On average, Neptune orbits the Sun at a distance of 30.1 AU, approximately 30 times the Earth–Sun distance. Neptune is similar in composition to Uranus, and both have compositions which differ from those of the larger gas giants, Jupiter and Saturn. Neptune's atmosphere, while similar to Jupiter's and Saturn's in that it is composed primarily of hydrogen and helium, along with traces of hydrocarbons and possibly nitrogen, contains a higher proportion of "ices" such as water, ammonia and methane.
  • 16. Rocks in Space Asteroids Shooting Stars Meteorite Comets
  • 17. Shooting Stars Shooting star is a common name for the visible path of a meteoroid as it enters the atmosphere to become a meteor. Also, shooting stars are the glowing tails of meteors, which heat up as they enter the Earth’s Atmosphere.
  • 18. Asteroids Asteroids are a class of small Solar System bodies in orbit around the Sun. They have also been called planetoids, especially the larger ones. Also, asteroids are mini – planets that orbit the Sun in a ‘belt’ between Mars and Jupiter.
  • 19. Meteorites A meteorite is a natural object originating in outer space that survives impact with the Earth's surface. A meteorite's size can range from small to extremely large. Most meteorites derive from small astronomical objects called meteoroids, but they are also sometimes produced by impacts of asteroids.
  • 20. Comets Comets are chunks of ice filled with dust and rock that orbit the sun, just like planets. However, comets travel much farther out into distant space, often to the outer reaches of the Solar System, so comets can take up to thousands of years to make on orbit of the sun.
  • 21. Black Holes A black hole is a region of space time where gravity prevents anything, including light, from escaping. The theory of general relativity predicts that a sufficiently compact mass will deform space time to form a black hole. Around a black hole there is a mathematically defined surface called an event horizon that marks the point of no return. It is called "black" because it absorbs all the light that hits the horizon, reflecting nothing, just like a perfect black body in thermodynamics. Quantum mechanics predicts that black holes emit radiation like a black body with a finite temperature. This temperature is inversely proportional to the mass of the black hole, making it difficult to observe this radiation for black holes of stellar mass or greater.
  • 22. Quasars The word quasar stands for quasi-stellar radio source. They are the brightest and most distant objects in the universe as we know it. The term quasar has fallen out of common use by astronomers and they are now known as quasi-stellar objects(QSOs) because we now know that they are not true stars.
  • 23.
  • 24. Life of a star Stars begin life when Nebulae are pulled together by their own gravity.. They get squeezed and begin to get hot. Nuclear fusion begin as Hydrogen atoms fused together to make Helium. The heat from the fusion makes the Star shine. The heat generated in the core pushes gas out as hard as gravity pulls in it. After 10 Billion years all the Hydrogen in the Stars core is burned up and it begins to burn Helium. Then the Star goes on swri;ing into super giants, once Iron forms in the center the Star fails to give energy and collapses that triggers an explosion like the nuclear bomb which is called super nova. .Then the Star either turns into a Black hole or a Neutron Star.