G9 Science Q3- Week 8-9- Constellation.pptx

Constellation

1. Constellations & Stars PREPARED BY: JOANNA Q. LANUZA

2. Show which constellations may be observed at different times of the year using models S9ES -IIIj - 35

3. I. Constellations Group of stars that appear to form a pattern in the sky. 88 recognized by International Astronomy Union

4. A. Zodiac Band of 12 constellations Band of 12 constellations along the ecliptic .

5. B. Ecliptic The plane of the Earth’s orbit around the sun The apparent path that the sun (and planets) appear to move along against the star background.

6. Ecliptic

7. C. Circumpolar Constellations Can be seen all year long Never fully set below the horizon Appear to move counter clockwise around Polaris Caused by Earth’s Rotation

8. Circumpolar Constellations

9. Star Trails

10. Examples of Circumpolar Constellations Ursa Major – The Big Bear Ursa Minor – The Little Bear Cassiopeia – Queen on Her Throne Draco - The Dragon Cepheus - The King

11. # of stars seen as circumpolar depends on the observers latitude Further North the observer lives, the more stars will appear circumpolar Earth turns west to east Sky appears to turn east to west

12. D. Ursa Major Best known constellation Common name is Big Dipper Pointer stars - front 2 stars of the Big Dipper which point to Polaris (North Star)

13. II. Seasonal Changes in Constellations Big Dipper In Fall: Low over northern horizon Spring: High overhead Cassiopeia In Fall: Straight overhead Spring: Low over northern horizon

14. Seasonal Change & Nightly change of the Dippers

15. III. Summer Constellations 1 st 3 bright stars that rise form the Summer Triangle Vega - in Lyra the Harp Altair - in Aquilla the Eagle Deneb – in Cygnus the Swan (Northern Cross)

16. Summer Triangle

17. IV. Most Famous Winter Contellation Orion Contains: Betelgeuse (Bet el jooz) a bright red super giant star found forming Orion’s right shoulder Rigel – a blue super giant: 7 th brightest star in the nighttime sky

18. 3 Stars of Orion’s Belt Can be used to find 2 other constellations & a star cluster Canis Major- (Big Dog) follow the line made by the 3 stars of Orion’s belt down to the left Sirius- the brightest star in the nighttime sky is found in Canis Major

19. 2. Taurus (the Bull) Follow the line made by Orion’s belt up & to the right Aldebaran - Red star that is the eye of the bull is the 13 th brightest in the nighttime sky

20. 3. Pleiades Star Cluster (7 sisters) Follow the line made by Orion’s belt up to the right, go through Taurus to a clump of stars to the right. Called Subaru in Japan – means “Unite”

21. V. Kinds of Stars Red Giant - large red star at least 10x diameter of the sun Old Stars Ex. Aldebaran The sun will swell into a Red Giant when it is old

22. B. Super Giant Largest of all stars 100x more luminous Explode as a Super Nova Can form Black Holes Ex. Betelgeuse, Rigel, Polaris

23. C. Dwarf Stars  Less luminous Very dense, mostly carbon Tightly packed nuclei Remains of a red giant that ran out of fuel 1 cup full of star =20 tons or 5 elephants.  Most are red/orange/yellow White dwarf is the exception to the color Sun is a yellow dwarf

24. Size Comparison of Various Stars

25. VI. Variable Stars Change in brightness over regular periods of time Ex. Cepheid Variables/Pulsating Stars Binary Stars & Eclipsing Binary Stars

26. A. Cepheid Variables/ Pulsating Stars Change in brightness as they expand & contract Unequal balance between gravity & nuclear fusion Ex. Polaris, Betelgeuse

27. B. Binary Star Systems Two stars of unequal brightness revolving around a center point Ex. Algol & its companion star in Perseus

28. C. Eclipsing Binary Stars Two close stars that appear to be a single star varying in brightness. The variation in brightness is due to one star moving in front of or behind the other star. Occurs because we see the system on edge instead of from above or below

29. VII. Pulsars or Neutron stars Discovered in 1967 (LGM) A distant heavenly object that emits rapid pulses of light & radio waves Formed when a Super Giant collapses; Protons & Electrons are forced so close together that they fuse and form only neutrons 

30. Twinkle Twinkle Little Star "Twinkling Stars" are due to Earth's atmosphere

31. VIII. Life Cycle of a Medium Mass Star Nebula Protostar New/Stable State Star Red Giant Planetary Nebula White Dwarf Black Dwarf

32. 1. Nebulae (Plural of Nebula) Space gas seen as faint glowing clouds Mostly hydrogen    Star dust is extremely small, smaller than a particle of smoke & widely separated, with more than 300 ft. between individual particles. Nebulae still hinder star gazing because they absorb light which passes through them.

33. Types of Nebulae Diffuse Nebula - gases glow from stars w/in them Ex. Nebula found in Sagittarius

34. Types of Nebulae Dark Nebula - nebula not near a bright star  Ex. Horse Head Nebula in Orion

35. 2. Protostar Shrinking gas balls, caused by a swirl of gas forming dense areas.  The gravity of the dense swirl in turn attracts nearby gases so a ball forms. Nuclear fusion occurs & Helium is formed from Hydrogen A new star is born in our galaxy every 18 days

36. 3. Stable State Star Star that releases energy in enough force to counter balance gravity Star stops contracting Also known as a main sequence star Ex. Sun

37. 4. Planetary Nebula The outer layers of the Red Giant puff out more and more. The star loses gravitational hold on its outer layers and they get pushed away by the pressure exerted from solar winds

38. Planetary Nebula

39. 5. White Dwarf Fuel is used up No nuclear fusion occurring Remaining heat radiates into space

40. IX. Life Cycle of a Massive Star 1st three steps are similar Super Giant Super Nova Neutron Star / Pulsar Black Hole

41. 1. Super Giant Rare stars, largest of all 100x more luminous Only stars with a lot of mass can become super giants Some are almost as large as our entire solar system Ex. Betelgeuse & Rigel

42. 2. Super Nova Explosion from a massive Super Giant Outer layer blasts away at end of Life Cycle Emits light, heat, X-rays, & neutrinos Leaves behind a neutron star or black hole

43. 3. Neutron Star/ Pulsar The remains of a super nova Very small, super-dense star which is composed mostly of tightly-packed neutrons Rapidly spinning leftovers of a star Emits energy in pulses

44. 4. Black Hole Occurs when a star's remaining mass is greater than three times the mass of the Sun Star contracts tremendously Incredibly dense with a gravitational field so strong that even light cannot escape.

45. Life Cycle of a Massive Star

46. X. Distance to stars The Sun is closest star to Earth Takes light 8 minutes to reach Earth Avg. distance:150,000,000Km = 1 AU distance from Earth to the Sun Next nearest star is Proxima Centauri 4.2 light years away; it can only be seen in the southern hemisphere     

47. E. Light year The distance light has traveled in a year 9.5 x 10 12 Km/yr Speed of light 300,000 Km /sec

48. XI. Physical Properties of Stars Nuclear fusion supplies the energy for stars Huge size & mass of a star means outer layers press inward w/ tremendous pressure Hydrogen ignites Star becomes a huge nuclear bomb Hydrogen nuclei combine to form Helium

49. B. Color of star depends on surface temp . Blue - hottest stars Ex. Rigel in Orion; Vega in Lyra; Sirius in Canis Major Yellow - medium stars ex. Sun Red - coolest stars Ex. Betelgeuse in Orion, Antares the heart of Scorpio, Aldebaran in Taurus

50. C. Star size -Varies, large range Smallest can be smaller than Earth Largest may be 600,000,000 x Earth.

51. D. The Sun is an average star yellow in color 300,000 x the mass of Earth

52. XII. Luminosity Brightness of a star Depends on size & temperature Hertzsprung-Russell Diagram graphs Absolute Magnitude (or Luminosity) vs. Temperature of stars Shows the life cycle of stars

53. Hertzsprung-Russell Diagram

54. A. Absolute Magnitude Measure of the amount of light it actually gives off if all stars were placed a distance of 32.6 light years away Lower # means brighter star Negative #’s are the brightest Ex. Sun = 4.75 Sirius = 1.4 Rigel = –7.0 Rigel’s the Brightest of the 3 listed if all were lined up next to each other.

55. B. Apparent Magnitude A measure of the amount of light received on Earth Stars below 0 are brightest Each magnitude differs by 2.5 1 st magnitude is 100 x brighter than 6 th magnitude Ex. Sun = – 26.8 Sirius = – 1.45 Full Moon –12 .6 Rigel = .11 Sun is the brightest in our sky.

56. XIII. Galaxies Systems containing millions or billions of stars, gas, & dust held together by gravity       Ex. Milky Way There are great distances between galaxies The Milky Way belongs to a group or cluster of galaxies called the local group

57. Spiral Galaxy Like the Milky Way

58. Three major classes of galaxies: Elliptical - shaped like large ovals or football shape Spiral - pinwheel shaped; our sun is on a spiral arm of the Milky Way Irregular - many different shapes that aren't like the other two

59. XIV. Quasar Quasi stellar radio source Galaxies, very far away, with bright centers Thought to have a super massive black hole at center Most luminous objects known to man

60. XV. Electromagnetic Spectrum The arrangement of electromagnetic radiation from Radio waves to Gamma waves

61. Stars Emit: Visible light  X-rays Radio waves Infrared waves Ultraviolet waves

62. Venus & Saturn by E-spectrum Ultra violet Visible Infrared Radio Ultra violet Visible Infrared Radio

63. X-ray & Ultra Violet Image of Sun

64. Visible, Infrared & Radio Images of Sun

65. A. Electromagnetic waves: Differ in wavelength & frequency   All electromagnetic waves travel at the speed of light; 300,000 km/sec

66. Parts of a Wave

67. a has a longer wavelength (distance from one crest to another) but lower frequency ( # of waves that pass by a point in a second)

68. b has a shorter wavelength but a higher frequency

69. B. Spectroscope Instrument that separates light into its colors. Contains: ✔   Prism at one end ✔   Slit at opposite end which lines up with the light source

70. C. 3 Types of Spectra Continuous Spectrum Brightline Spectrum Darkline Spectrum

71. How Spectra are Produced

72. 1. Continuous Spectrum Produced by a glowing solid Example a Tungsten white light bulb, & white sunlight.

73. Continuous Spectrum Cont’ Continuous set of emission lines forming an unbroken band of colors from red to violet. Shows the source is sending out light of all visible wavelengths.   

74. Visible Spectrum ROY G BIV All the colors of the rainbow A continuous spectrum red  orange yellow green blue indigo       violet

75. 2. Dark-Line Spectrum / Absorption Spectrum Produced when a cooler gas lies between the observer and an object emitting a continuous spectrum Example: 1. The atmosphere of planets 2.Outer layers of a star

76. Absorption Spectrum Cont’ The cooler gas absorbs specific wavelengths of radiation passing through it. This spectrum appears as a continuous spectrum of all colors with a number of gaps or dark lines throughout it.

77. 3. Bright-Line Spectrum / Emission Spectrum Produced by a glowing gas which radiates energy at specific wavelengths characteristic of the element or elements composing the gas Example Neon signs, black lights, LED’s

78. Emission Spectrum Cont’ This spectrum consists of a number of bright lines against a dark background. Each elements has its own distinctive spectra much like a fingerprint http://jersey.uoregon.edu/vlab/elements/Elements.html

79. XVI. The Doppler Effect as sound approaches the wavelength is compressed so the pitch is higher as sound leaves the wavelength is stretched out so the pitch is lower The same thing happens with light 

80. Doppler Effect

81. Red Shift If a star is moving away from Earth there is a red shift, of its line spectra; if the star is moving toward the Earth there is a blue shift of its line spectra  

82. Red Shift Red shift is evidence the universe is expanding.

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