2 Q. Read the passage. In the SolarSystem, the inner planets, such as the Earth, contain elements which are eavierthan the elements hydrogen and helium. Our star,the Sun, is a medium sized star. If a star is much more massive than the Sunit will eventually swell into a red giant, start to contract, continue tocontract and finally explode. What is the explosion called? () Explain why scientists believe that the Solar System was formed from the material produced when earlier stars exploded. (3) (Total 4 marks) Q2. Complete the two spaces in the sentence. Stars form when enough and gas from are pulled together by gravitational attraction. How are stars able to give out energy for millions of years? Put a tick ( ) next to the answer. By atoms joining together By atoms splitting apart By burning gases
3 () (c) There are many billions of stars in our galaxy. Our Sun is one of these stars. What is the name of our galaxy? () (d) Why was the Universe created? We cannot expect scientists to answer this question. What is the reason for this? Put a tick ( ) next to the reason. It will take too long to collect the scientific evidence. The answer depends on beliefs and opinions, not scientific evidence. There is not enough scientific evidence. () (Total 5 marks) Q3. Light is given out by the Sun and a distant galaxy. Compared to the light from the Sun, the light from the distant galaxy has moved towards the red end of the spectrum. (i) What name is given to this effect? () Complete the following sentence by drawing a ring around the line in the box that is correct. The fact that light from a distant galaxy seems to move towards the red end of galaxies are shrinking the spectrum gives scientists evidence that galaxies are changing colour the universe is expanding () Scientists have a theory that the universe began from a very small point and then exploded outwards. (i) What name is given to this theory?
4 () Which statement gives a reason why scientists think that the universe began with an explosion? Put a tick ( ) in the box next to your choice. At the moment it is the best way of explaining our scientific knowledge. It can be proved using equations. People felt the explosion. () (Total 4 marks) Q4. The visible part of the electromagnetic spectrum from a star includes a dark line. This line is at a specific wavelength. The diagram shows the position of the dark line in the spectrum from the Sun and in the spectrum from a distant galaxy. Explain how the spectrum shift of the dark line supports the theory that the Universe began from a very small point. (3) From data collected, a graph can be drawn that links the speed of a galaxy with the distance of the galaxy from the Earth.
5 (i) How does the visible light spectrum from galaxy A look different from the visible light spectrum from galaxy B? () A third galaxy, C, seems to be travelling away from the Earth at about km/s. Estimate how far galaxy C might be from the Earth, showing how you use the graph to do this. Distance between galaxy C and the Earth = million light years (Total 6 marks) Q5. Satellites fitted with various telescopes orbit the Earth. These telescopes detect different types of electromagnetic radiation.
6 Why are telescopes that detect different types of electromagnetic waves used to observe the Universe? () In 2005 a space telescope detected a star that exploded 3 billion years ago. The light from the star shows the biggest red-shift ever measured. (i) What is red-shift? () What does the measurement of its red-shift tell scientists about this star? () (c) Red-shift provides evidence for the big bang theory. (i) Describe the big bang theory. Suggest what scientists should do if new evidence were found that did not support the big bang theory. () (Total 6 marks) Q6. Explain how stars produce energy.
7 What evidence is there to suggest that the Sun was formed from the material produced when an earlier star exploded? () (c) It is thought that gases from the massive star Cygnus X- are spiralling into a black hole. (i) Explain what is meant by the term black hole. What is produced as the gases from a star spiral into a black hole? () (Total 6 marks) Q7. The light spectrum from a distant galaxy shows a red shift. What is meant by red shift and what does it tell us about distant galaxies? What name is given to the theory that the Universe started with a massive explosion? ()
8 (Total 3 marks) Q8. Complete the following sentences by choosing the correct words from the box. Each word may be used once or not at all. dwarf giant neutron proton supernova If a red star is large enough, it may eventually blow up in an explosion called a, leaving behind a very dense star. (Total 3 marks) Q9. Stars do not stay the same forever. Over billions of years the amount of hydrogen in a star decreases. Why? () Describe how a massive star (at least five times bigger than the Sun) will change at the end of the main stable period. To gain full marks in this question you should write your ideas in good English. Put them into a sensible order and use the correct scientific words. (4) (c) The inner planets of the solar system contain atoms of the heaviest elements. (i) Where did these atoms come from? ()
9 What does this tell us about the age of the solar system compared with many of the stars in the Universe? () (Total 7 marks) Q0. The Big Bang theory attempts to explain the origin of the Universe. (i) What is the Big Bang theory? () What can be predicted from the Big Bang theory about the size of the Universe? () (Total 2 marks) Q. (i) Explain how stars like the Sun were formed. The Sun is made mostly of hydrogen. Eventually the hydrogen will be used up and the Sun will die. Describe what will happen to the Sun from the time the hydrogen is used up until the Sun dies. (3) (Total 5 marks) Q2. The Big Bang theory attempts to explain the origin of the Universe.
10 (i) What is the Universe? () (i) What are the main ideas of the Big Bang theory? (iii) What is thought to be happening to the size of the Universe? () (Total 4 marks) Q3. Most of the Sun is hydrogen. Inside the core of the sun, hydrogen is being converted to helium. What name is given to this process and why is the process so important? Describe what will happen to the Sun as the core runs out of hydrogen. (3) (Total 5 marks) Q4. Stars are formed from massive clouds of dust and gases in space. What force pulls the clouds of dust and gas together to form stars?
11 () Once formed a star can have a stable life for billions of years. Describe the two main forces at work in the star during this period of stability. (c) What happens to this star once this stable period is over? (4) (d) Suggest what might then happen to a planet close to this star. () (Total 8 marks) Q5. Explain how observations at the red end of the spectrum of light from galaxies have led to one theory about the origin of the Universe. (Total 6 marks) Q6. Describe briefly how stars such as the Sun are formed.
12 (Total 2 marks) Q7. Nuclear fusion in the Sun releases large amounts of energy. (i) Explain what is meant by nuclear fusion. (3) Why is energy released by such nuclear fusion reactions? (Total 5 marks) Q8. Astronomers believe that the Universe is expanding. (i) How might the Universe have started? () State and explain briefly, one piece of scientific evidence which may be used to support this belief. (Total 3 marks)
13 Q9. The Sun is at the stable stage of its life. Explain, in terms of the forces acting on the Sun, what this means. (3) At the end of the stable stage of its life a star will change. Describe and explain the changes that could take place. (6) (Total 9 marks) Q20. Our Sun is just one of many millions of stars in a galaxy called the Milky Way. Our Sun is in the main stable period of a star s lifetime. The massive force of gravity draws its matter together. This force is balanced by the very high temperatures, from the fusion of hydrogen atoms, which tend to make the Sun expand. Describe and explain what will happen to the Sun as the hydrogen is eventually used up. (Total 3 marks)
14 Q2. Studies of light from distant galaxies have provided evidence for the theory that the Universe started from one place and is expanding. Explain how. (Total 3 marks) Q22. Studying stars gives scientists evidence about the evolution of the Universe. (i) In astronomy, what is meant by a black hole? How is it possible to detect a black hole? The changes which happen in stars result in new elements being formed. Nuclei of the heaviest elements are found in the Sun. Describe how these nuclei are formed. (Total 6 marks) Q23.
15 One theory of the origin of the Universe was that billions of years ago all matter was in one place, then it exploded ( big bang ). Describe, in as much detail as you can, how our star (the Sun) formed from the time when there was just dust and gas (mostly hydrogen) up to now when it is in its main stable period. To gain full marks in this question you should write your ideas in good English. Put them into a sensible order and use the correct scientific words. (Total 5 marks) Q24. Red shift is one of the pieces of evidence which led scientists to propose the big bang theory. Describe the big bang theory.
16 To gain full marks for this question you should write your ideas in good English. Put them into a sensible order and use the correct scientific words. Explain how red shift provides evidence for the big bang theory. (3) (Total 5 marks) Q25. The Sun at the centre of our solar system is a star. The Sun contains nuclei of the heaviest elements. Atoms of these heaviest elements are also present in the planets of the solar system. What does this suggest about the material from which the solar system is formed? () Stars form from gas (mostly hydrogen) and dust.
17 Describe, in as much detail as you can, what forces allow a stable star to exist and how the star may eventually form a black hole. To gain full marks in this question you should write your ideas in good English. Put them into a sensible order and use the correct scientific words. (6) (Total 7 marks) Q26. Astronomers use red shift in two ways. They calculate the distance to each galaxy from Earth. They also calculate the speed at which galaxies are moving away from Earth. The table shows some results. Distance is given in zettametres, Zm. One zettametre is 0 2 metres. Galaxy Distance from Earth to galaxy in Zm Speed at which galaxy is moving away from us in Zm per billion years Time the galaxy has been moving away from us in billions of years (Calculated by distance speed) Abell Abell
18 Abell Abell Abell Complete the data for Abell 302. () Describe the relationship between the distance to a galaxy and the speed at which the galaxy is moving away from us. () (c) Explain how the data for time provides evidence for the theory that the origin of the Universe was a huge explosion ( big bang ). (Total 4 marks) Q27. The flowchart shows four stages thought to occur in the evolution of a star such as our Sun. At a particular time a star might have reached one of these stages or be between stages or be at a further stage. What period in its evolution has our star, the Sun, reached?
19 (Total mark) Q28. What does the Big Bang theory state? In your answer you may include evidence for the theory. (Total 4 marks) Q29. At the very high temperatures in the sun, hydrogen is converted into helium. It takes four hydrogen nuclei to produce one helium nucleus. The table shows the relative masses of hydrogen and helium nuclei. Use these figures to calculate what happens to the mass of the sun as hydrogen is converted to helium. (3) Use your answer to part to explain how the sun has been able to radiate huge amounts of energy for billions of years.
20 (Total 5 marks) Q30. The energy radiated by a main sequence star like the Sun is released by a nuclear fusion reaction in its core. Read the following information about this reaction then use it to answer the questions below. The net result of the nuclear fusion reaction is that four hydrogen nuclei produce one helium nucleus. There is a loss of mass of 0.7%. For nuclear fusion to occur nuclei must collide at very high speeds. The energy released during the reaction can be calculated as shown: energy released [J] = loss of mass [kg] (speed of light [m/s²]) (The speed of light is m/s) Calculate the energy released when g of hydrogen fuses to form helium. (Show your working.) (4) The table shows the lifetimes and surface temperatures of main sequence stars with different masses. MASS OF STAR [SUN = ] LIFETIME ON MAIN SEQUENCE [MILLION OF YEARS] SURFACE TEMPERATURE * [KELVIN] [* The higher the surface temperature of a star, the higher the temperature and pressure in its core.] (i) Describe the relationship between the lifetime of a main sequence star and its mass.
21 Suggest an explanation for this relationship. (3) (Total 9 marks) Q3. Explain, in as much detail as you can, the scientific evidence for the big bang theory of the origin of the Universe. (Total 5 marks) Q32. Read the following information about cosmic microwave background radiation. Then use it to answer the questions below.
22 (You may find it helpful to begin by deciding which items of information belong to which question.) Explain, as fully as you can, why the frequency profile of electromagnetic radiation is an indication of temperature. (3) Describe, in as much detail as you can, what cosmic microwave background radiation is and how it was discovered.
23 (3) (c) Explain, as fully as you can, how cosmic microwave background radiation fits in with the idea that the Universe, as it now is, began with a big bang. (4) (d) Some people think that Penzias and Wilson s discovery of cosmic microwave background radiation was just lucky. Others disagree. What do you think? Give reasons for your answer. (Total 2 marks) Q33. Describe, in as much detail as you can, the life history of a star like our Sun.
24 (Total 6 marks)
25 Mark schemes Q. supernova (explosion) solar system contains heavy elements / elements heavier than hydrogen and helium () these (heavy) elements are / were formed by (nuclear) fusion () accept minor misspellings for fusion but not anything which could also be fission (at the very high temperature(s)) in a super nova / when stars explode () 3  Q2. dust accept solid (s) space accept from supernova / supernovum / supernovas By atoms joining together only one ticked or otherwise unambiguously identified (c) Milky Way (galaxy) (d) The answer depends on beliefs and opinions, not scientific evidence. only one ticked or otherwise unambiguously identified  Q3. (i) red shift accept Doppler effect the universe is expanding (i) big bang at the moment it is the best way of explaining...  Q4.
26 line shifts towards red end of spectrum do not accept reference to red light do not accept red shift as a stand alone response wavelength (appears) to increase galaxy is moving away (from the Earth) do not accept universe expanding or galaxy moving away from initial point do not accept planet on its own (i) light from A has a greater red shift accept light from A is more red do not accept reference to blue light 3600 (million light years) allow mark for showing that the line could be extended or allow mark for the correct use of a point on the line 2  Q5. stars / galaxies / sources emit all / different types of electromagnetic waves / radiation accept two or more named electromagnetic waves accept answers in terms of frequencies / wavelengths (i) wavelength (of light) increases accept frequency decreases or light moves to red end of spectrum accept redder but do not accept red alone it is the star (detected) furthest from the Earth accept galaxy for stars or it is moving away the fastest ignore reference to universe expanding (c) (i) all matter compressed to / starts at / comes from a single point do not accept increasing gravitational pull accept everything / the universe for all matter
27 (massive) explosion sends matter outwards accept explosion causes universe to expand ignore explosion creates the universe or further reference to star / Earth formation check validity / reliability of the evidence or change the theory to match the new evidence accept comparison of new and old evidence  Q6. any two from: nuclei / atoms of light elements fuse accept hydrogen or helium for light elements accept join for fuse accept for mark, by nuclear fusion answers about fission negates a mark each (fusion) reaction releases energy / heat / light lots of reactions occur presence of nuclei of the heaviest / heavy / heavier elements accept atom for nuclei 2 (c) (i) (matter / mass) with such a high density / strong gravitational (field) electromagnetic radiation / light is pulled in accept nothing can escape do not accept answers in terms of an empty void X-rays accept e-m radiation / e-m waves  Q7. longer wavelength waves or light moved towards red end of spectrum (galaxy) moving away from the Earth or space is expanding or the galaxy and Earth are moving apart accept us for Earth do not accept galaxies expanding big bang 
28 Q8. giant supernova neutron  Q9. converted into helium accept helium created accept converted into heavier elements accept used up in nuclear fusion / to produce energy do not accept any reference to burning turns / expands into a red giant contradictions negate mark contracts and explodes or becomes a supernova may form a (dense) neutron star or (if enough mass shrinks to) form a black hole accept forms a neutron star and (then) a black hole Quality of written communication correct points must be in sequence (c) (i) supernova or remains of an earlier star ignore super nebula younger or not formed at the time of the Big Bang  Q0. (i) an enormous explosion causing matter to spread from one point it is increasing or expanding  Q. (i) from a (giant) cloud of gas or hydrogen condensed or pulled into a smaller volume by gravity
29 any three from: fusion decreases or stops collapses rapidly causing the (core) temperature to rise (inward) gravitational forces no longer balance (outward) pressure expands and becomes a red giant it cools then becomes a white dwarf helium may fuse if the sequence is incorrect deduct  therefore maximum 2 marks 3  Q2. (i) an innumerable collection of galaxies accept any word meaning a large number for innumerable accept all the galaxies do not accept everything all matter concentrated at a (single) point accept all matter part of a single superatom single (massive) explosion (sending matter outwards) (iii) increasing or expanding  Q3. fusion accept fussion energy producing process accept heat and/or light for energy accept fussion up to 2 points from: 3 marks for 3 points in sequence with no contradiction expands
30 cools 2 marks for 2 points in sequence with no contradiction forms a red giant mark for a correct point which is not contradicted up to 2 points from: do not accept it turns red contracts increases in temperature forms a white dwarf ignore further reference to black dwarfs, black holes, nebulae, supernovae 3  Q4. (c) gravitational attraction for mark gravitational (in); high internal temperature generates force (out) for mark each star expands; to form red giant; then contracts/collapses; to form white dwarf/neutron star/black hole/pulsar; they may explode/become supernova any four for mark each 2 4 (d) engulfed by red giant/blown up by star/hit by debris from star; sucked into black hole for mark  Q5. light from (distant) galaxies shows shift to red end of spectrum wavelength increased explained by galaxies moving away from us more distant galaxies have greater recession speed seen in all directions suggests universe is expanding any sensible reference to similar effect on Earth any 6 for mark each  Q6. formed from dust or gas (unless in atmosphere) which is pulled together by gravitational forces high temperature inside
31  Q7. (i) the nuclei of hydrogen/smaller atoms join to make helium/larger atoms for mark each the mass of the large nucleus (atom) is less than the mass of the smaller nuclei (atoms) for mark 3 mass loss converted into energy or small mass loss given a large amount of energy for mark 2  Q8. (i) the Universe might have started with an explosion/ Big Bang light from galaxies is shifted to red end of spectrum the further away the greater the red shift all galaxies receding furthest fastest microwave background echo of big bang for mark each 2  Q9. the Sun is subject to two balancing forces / 2 forces in equilibrium the forces are: gravity making it contract or inward force due to gravity and a force due to temperature / heat / energy / radiation pressure making it expand or outward force due to temperature / heat / energy / radiation pressure for mark each 3 Read all the answer first. Stop after 6 marks. hydrogen / fuel used up owtte the star will expand and become a red giant it will contract under gravity become a white dwarf it may explode and become a supernova throwing dust and gas into space leaving a dense neutron star / black hole (no mark for contradiction) any six for mark each 6  Q20. any three from max 2 if stages but no explanation the star (Sun) expands because
32 (inward) gravitational forces no longer balance (outward) force accept the star collapses rapidly causing the core temperature to increase and the star to expand accept it expands because the forces are unbalanced to become a red giant when the fusion stops it contracts / cools accept (when hydrogen is used up) it collapses under gravity accept when fusion stops it contracts and explodes to become a white dwarf accept to become a supernova / pulsar / neutron star / black hole (only if red giant has exploded)  Q2. light from distant galaxies red shifted accept longer wavelength for red shifted further galaxies display greater red shift the further away galaxies are the faster they are moving away from us (our galaxy)  Q22. (i) any two from (matter from) exploded star / supernova matter so dense / gravity so strong that electromagnetic radiation / light cannot escape from it X-rays emitted when gases or matter released from nearby stars spiral into it 2 fusion (of nuclei) of lighter elements / hydrogen helium  Q23. Quality of written communication: One mark for using correct scientific sequence : gravity fusion balance any four from
33 (dust and gas) pulled together by gravity (star formed when) it is hot enough accept (as mass is pulled together) it gets very hot hydrogen (and helium) nuclei fuse (these nuclear fusion reactions) release the energy / heat / light (which is radiated by stars) energy causes expansion gravitational pull is balanced by the expansion (force) 4  Q24. any two from Universe started in one place (huge) explosion Universe is expanding do not accept big bang Quality of written communication: Links needed between : galaxies, red shift, and distance / expansion any two from light from (galaxies) shifted towards red end of spectrum the further away the galaxy, the greater the red shift this shows that galaxies are moving away from us 2 this suggests that Universe is expanding do not accept light from planets 2  Q25. materials produced when earlier stars exploded accept the Sun is a second generation star accept formed from nebulae Quality of written communication: mark for correct sequencing balanced forces expansion contraction / explosion
34 any five from gravity pulling matter together accept idea that a star is very massive so its force of gravity is very strong high temperatures that create expansion forces nuclear fusion releases energy that causes the very high temperatures these forces balance star expands greatly since expansion is greater than gravity accept fuel runs out forms a red giant give no further marks if red giant white dwarf, red dwarf etc collapses inwards and explodes outwards called a supernova neutron star may form leaves a small, dense object (a black hole) accept nothing can escape from it 5  Q the further away, the faster it is moving away (c) all galaxies have been moving away from us for approximately the same length of time therefore they were all probably produced at the same time  Q27. any one of * between (stage) 2 and (stage) 3 * (in) the main sequence * (in) the main stable period * (it is a) yellow dwarf 
35 Q28. any four related points * the Universe (as we know it) started (about) 4 000/5 000 million years ago or (about) 5 billion years ago or between (about) 0 to 20 billion years ago * from one point or from a singularity or at the beginning of time * in an enormous outpouring of matter (and energy) * (and) has been expanding ever since * (evidence is that) the galaxies are all moving away from one another * (evidence is that) the more distant a galaxy is the faster it is moving away (from all the other galaxies) * evidence is microwave background or cosmic background radiation *... relic of an earlier or hot phase resulting from (shortly) after the start or Big Bang * evidence is red shift *... of light or radiation from (distant) stars or galaxies or quasars or due to Doppler (-Fizeau) effect accept bya for billion years ago or mya for million years ago do not credit vague responses such as it all started with a big explosion  Q29. evidence of conclusion or each gain mark based on use of data that there is a (very small) loss of mass or but a loss of mass of for every helium atom or 0.69%/0.7% gains 3 marks 3 idea that loss of mass results in release of energy gains mark but small loss of mass results in huge energy release gains 2 marks 2  Q30. it use E = mc 2 mass in kg i.e each gains mark
36 gains 3 marks but gains 2 marks evidence of mass in kg (i.e or 0.7/00000) each gains mark squaring the speed of light but (credit alternative ways of stating this) gains 3 marks units J/joule for further mark (N.B credit kj, MJ, GJ but check power of 0 for full credit) 4 (i) idea that the bigger the mass the shorter the life gains mark but idea that decrease in life is much more than proportional to increase in mass or more than proportional to mass 2 gains 2 marks ideas that: greater mass means greater core temperature/pressure greater core temperature/pressure means greater rate of fusion increase in mass produces a proportionally much greater increase in the rate of fusion each for mark 2 3  Q3. ideas that: galaxies show a red-shift gains mark but more distant galaxies show bigger red-shift gains 2 marks galaxies moving away/universe expanding gains mark but more distant galaxies moving away faster gains 2 marks so all Universe once in one place for further mark (only if the previous 2 marks are also gained) 
37 Q32. (c) (d) answer includes items: B D G each for mark answer includes items: A E F [allow H here for a further mark] each for mark answer includes items: C H* I J each for mark [*unless already credited in ] ideas that: lucky in the sense that they weren t initially looking for the background radiation [others were!!!] more than just lucky in that they investigated it and didn t just ignore it each for mark [NB Reference to letters only, not a prose answer, gain only ½ mark each. Total rounded down] 2  Q33. ideas that formed from dust/gases pulled together by gravity massive so very large gravitational forces (pulling inwards) hydrogen helium / fusion releases energy [not fission or just nuclear ] high temperature creates high pressure (pushing outwards) long period when forces balance then expands red giant / red star then contracts to (dense) white dwarf / white star [credit if massive enough / more massive than sun, red giant supernova (very dense) neutron star but do not accept w.r.t. Sun itself] [The whole of the (non bracketed part of) each idea must be present in some appropriate for in of words for each mark to be credited. To gain more than a single mark ideas must also be in correct sequence and/or appropriately related.] any six mark each 
Q. Describe, in as much detail as you can: the evidence that the size of the observable Universe is changing; the evidence that, billions of years ago, all the matter in the Universe was tightly packed
SOLAR SYSTEM, STABILITY OF ORBITAL MOTIONS, SATELLITES Q1. The figure below shows what scientists over 1000 years ago thought the solar system was like. Give one way that the historical model of the solar
1. (a) Once formed, a star can have a stable life for billions of years. Describe the two main forces at work in the star during this period of stability. 1.... 2.... What happens to a star once this stable
P8 SPACE PHYSICS Question Practice Name: Class: Date: Time: 40 minutes Marks: 40 marks Comments: GCSE PHYSICS ONLY Page of 52 In 929, the astronomer Edwin Hubble observed that the light from galaxies moving
Q1. Describe, in as much detail as you can: the evidence that the size of the observable Universe is changing; the evidence that, billions of years ago, all the matter in the Universe was tightly packed
Nuclear fission and nuclear fusion 1. Four different processes are described in List A. The names of these processes are given in List B. Draw a line to link each description in List A to its correct name
A. Solar system: stability of orbital motions; satellites (physics only) 1. Put these astronomical objects in order of size from largest to smallest. (3) Fill in the boxes in the correct order. the Moon
Classifying Stars In the early 1900s, Ejnar Hertzsprung and Henry Russell made some important observations. They noticed that, in general, stars with higher temperatures also have brighter absolute magnitudes.
NUCLEAR FISSION AND FUSION Q1. Uranium has two natural isotopes, uranium-235 and uranium-238. Use the correct answer from the box to complete the sentence. electrons neutrons protons The nucleus of a uranium-238
Q1. The diagram shows part of the life cycle of a star which is much bigger than the Sun. (a) (i) What is the relationship between the masses of the dust and gas in the cloud in Stage 2 and the force of
Edwin Hubble Discovered galaxies other than the milky way. Galaxy: A collection of stars, planets, gas, and dust that are held together by gravity. Our sun and planets are in the Milky Way He noticed that
I. Stars have color, brightness, mass, temperature and size. II. Distances to stars are measured using stellar parallax a. The further away, the less offset b. Parallax angles are extremely small c. Measured
Skills Worksheet Directed Reading A Section: The Life Cycle of Stars TYPES OF STARS (pp. 444 449) 1. Besides by mass, size, brightness, color, temperature, and composition, how are stars classified? a.
TEACHER BACKGROUND INFORMATION (The Universe) A. THE UNIVERSE: The universe encompasses all matter in existence. According to the Big Bang Theory, the universe was formed 10-20 billion years ago from a
Stars and Galaxies 1 Characteristics of Stars 2 Star - body of gases that gives off great amounts of radiant energy as light and heat 3 Most stars look white but are actually different colors Antares -
Q1. Complete the following sentences by choosing the correct words from the box. Each word may be used once or not at all. dwarf giant neutron proton supernova If a red...star is large enough, it may eventually
Section: Stars Pages 32-38 Study Guide Chapter 2 Circle the letter of the best answer for each question. 1. What do scientists study to learn about stars? a. gravity c. space b. starlight d. colors COLOR
NSCI 314 LIFE IN THE COSMOS 2 BASIC ASTRONOMY, AND STARS AND THEIR EVOLUTION Dr. Karen Kolehmainen Department of Physics CSUSB COURSE WEBPAGE: http://physics.csusb.edu/~karen MOTIONS IN THE SOLAR SYSTEM
Formation of the Universe & What is in Space? The Big Bang Theory and components of the Universe The Big Bang Theory The Big Bang Theory The Big Bang Theory is the most widely accepted scientific explanation
Earth Science, 13e Tarbuck & Lutgens Beyond Our Solar System Earth Science, 13e Chapter 24 Stanley C. Hatfield Southwestern Illinois College Properties of stars Distance Distances to the stars are very
the nature of the universe, galaxies, and stars can be determined by observations over time by using telescopes The spectral lines of stars tell us their approximate composition Remember last year in Physics?
Prentice Hall EARTH SCIENCE Tarbuck Lutgens Chapter 25 Beyond Our Solar System 25.1 Properties of Stars Characteristics of Stars A constellation is an apparent group of stars originally named for mythical
Unit 3 The Universe Chapter 4 ~ The Formation of the Universe o Section 1 ~ The Scale of the Universe o Section 2 ~ The Formation of the Universe o Section 3 ~ The Future of the Universe Chapter 5 ~ Galaxies
CHAPTER 1 The Life Cycle of a Star Describe the life cycle of various size stars. Rings of glowing gas encircling Supernova 1987A, about 179,000 light-years away in the Large Magellanic Cloud, one of the
How Do Stars Appear from Earth? Magnitude: the brightness a star appears to have from Earth Apparent Magnitude depends on 2 things: (actual intrinsic brightness) The color of a star is related to its temperature:
The Universe is space and everything in it. Galaxies A galaxy is a supercluster of stars, gas, and dust that are held together by gravity. There are three main types of galaxies: Irregular Elliptical Spiral
The Earth in the Universe (OCR) Evidence for the age of the Earth Scientists once thought that the Earth was only 6000 years old. Rocks have provided lots of evidence for the world being older. 1) Erosion
Life Cycle of a Star Worksheet A STAR IS BORN STAGES COMMON TO ALL STARS All stars start as a nebula. A nebula is a large cloud of gas and dust. Gravity can pull some of the gas and dust in a nebula together.
25.2 Stellar Evolution By studying stars of different ages, astronomers have been able to piece together the evolution of a star. Star Birth The birthplaces of stars are dark, cool interstellar clouds,
Instructions Fill in the blanks of each frame using the list of missing words given. Cut out each frame and arrange them on your page in order, then stick them down. The first two frames are already in
19.3 Galaxies and the Universe Early civilizations thought that Earth was the center of the universe. In the sixteenth century, we became aware that Earth is a small planet orbiting a medium-sized star.
Cosmology, Galaxies, and Stars OUR VISIBLE UNIVERSE Cosmology Cosmology is the study of the universe; its nature, origin and evolution. General Relativity is the mathematical basis of cosmology from which
Light Transverse electromagnetic wave, or electromagnetic radiation Includes radio waves, microwaves, infra-red, visible, UV, X-rays, and gamma rays The type of light is determined purely by wavelength.
240 points CHAPTER 29 STARS SECTION 29.1 The Sun (40 points this page) In your textbook, read about the properties of the Sun and the Sun s atmosphere. Use each of the terms below just once to complete
ASTRONOMY Universe- Includes all known matter (everything). Celestial Object Any object outside or above Earth s atmosphere. Galaxy- A large group (billions) of stars (held together by gravity). Our galaxy
chapter 31 Stars and Galaxies Day 1:Technology and the Big Bang Studying the Stars A. Telescopes - Electromagnetic radiation emitted by stars and other objects include light, radio, and X-ray Space telescopes
chapter 13 3 Stars and Galaxies section 3 Evolution of Stars Before You Read What makes one star different from another? Do you think the Sun is the same as other stars? Write your ideas on the lines below.
Stars Stars A star is a ball of different elements in the form of gases The elements and gases give off electromagnetic radiation (from nuclear fusion) in the form of light Scientists study the light coming
Answers The Universe Year 10 Science Chapter 6 p133 1 The universe is considered to be the whole of all matter, energy, planets, solar systems, galaxies, and space. Many definitions of the universe also
Stars and Galaxies Evolution of Stars What do you think? Read the two statements below and decide whether you agree or disagree with them. Place an A in the Before column if you agree with the statement
CHAPTER 9: STARS AND GALAXIES Characteristics of the Sun 1. The Sun is located about 150 million kilometres from the Earth. 2. The Sun is made up of hot gases, mostly hydrogen and helium. 3. The size of
Beyond Our Solar System Chapter 24 PROPERTIES OF STARS Distance Measuring a star's distance can be very difficult Stellar parallax Used for measuring distance to a star Apparent shift in a star's position
CHAPTER 16 1 A Solar System Is Born SECTION Our Solar System California Science Standards 8.2.g, 8.4.b, 8.4.c, 8.4.d BEFORE YOU READ After you read this section, you should be able to answer these questions:
Exam # 3 Tue 12/06/2011 Astronomy 100/190Y Exploring the Universe Fall 11 Instructor: Daniela Calzetti INSTRUCTIONS: Please, use the `bubble sheet and a pencil # 2 to answer the exam questions, by marking
Stars & Galaxies Chapter 27 Modern Earth Science Chapter 27, Section 1 27.1 Characteristics of Stars Composition & Temperature Scientists use the following tools to study stars Telescope Observation Spectral
Stars & Galaxies Chapter 27 Modern Earth Science Chapter 27, Section 1 27.1 Characteristics of Stars How do astronomers determine the composition and surface temperature of a star? Composition & Temperature
Section 1 Stars A. Patterns of stars - constellations 1. Ancient cultures used mythology or everyday items to name constellations 2. Modern astronomy studies 88 constellations 3. Some constellations are
Earth Space Systems Semester 1 Exam Astronomy Vocabulary Astronomical Unit- Aurora- Big Bang- Black Hole- 1AU is the average distance between the Earth and the Sun (93 million miles). This unit of measurement
Outline 8: History of the Universe and Solar System The Andromeda Galaxy One of hundreds of billions of galaxies, each with hundreds of billions of stars A warped spiral galaxy, 150 MLY away and 100,000
Life Cycle of a Star Video (5 min) http://www.youtube.com/watch?v=pm9cqdlqi0a The Life Cycle of Stars Solar Nebula Theory : Is the current theory of how our Solar System formed. This theory states that
Chapter 28 Stars and Their Characteristics Origin of the Universe Big Bang Theory about 10-20 bya all matter in the universe existed in a hot dense state about the size of an atom (tiny). That matter sort
Generally speaking, there are two main life cycles for stars. The factor which determines the life cycle of the star is its mass. 1 solar mass = size of our Sun Any star less than about three solar masses
Mass: 1.99 x 1030 kg Diameter: about 1 400 00 km = 100 x the Earth diameter Produces a strong gravitational forces: about 28 times greater than the gravitational force produces by the Earth Temperature:
Chapter 29 and 30 Explain how the sun converts matter into energy in its core. Describe the three layers of the sun s atmosphere. Explain how sunspots are related to powerful magnetic fields on the sun.
Standard 1: Students will understand the scientific evidence that supports theories that explain how the universe and the solar system developed. They will compare Earth to other objects in the solar system.
CORNELL NOTES Directions: You must create a minimum of 5 questions in this column per page (average). Use these to study your notes and prepare for tests and quizzes. Notes will be turned in to your teacher
Textbook Chapters 24 - Stars Textbook Chapter 25 - Universe Regents Earth Science with Ms. Connery SPECTROSCOPY is the study of light. Read to learn - textbook pages 674-677 STAR LIGHT gives us characteristics
Stellar Evolution Review: HR Diagram Label A, B, C respectively A C B a) A: White dwarfs, B: Giants, C: Main sequence b) A: Main sequence, B: Giants, C: White dwarfs c) A: Main sequence, B: White Dwarfs,
Astronomy 104: Second Exam Stephen Lepp October 29, 2014 Each question is worth 2 points. Write your name on this exam and on the scantron. Short Answer A The Sun is powered by converting hydrogen to what?
1 Astr 102 Lec 9: Stellar Evolution and DeathBirth and Evolution Why do stars leave main sequence? What conditions are required for elements Text besides Hydrogen to fuse, and why? How do stars die: white
A STAR IS BORN Overview: Students will research the four stages of the life cycle of a star then further research the ramifications of the stage of the sun on Earth. Objectives: The student will: research,
GALAXIES AND STARS 1. Compared with our Sun, the star Betelgeuse is A smaller, hotter, and less luminous B smaller, cooler, and more luminous C larger, hotter, and less luminous D larger, cooler, and more
Chapter Introduction Lesson 1 The View from Earth Lesson 2 The Sun and Other Stars Lesson 3 Evolution of Stars Lesson 4 Galaxies and the Universe Chapter Wrap-Up What makes up the universe and how does
Name Class Date Chapter 25 The Solar System Section 25.1 Exploring the Solar System (pages 790 794) This section explores early models of our solar system. It describes the components of the solar system
Earth and the Solar System The Formation of the Solar System Write a number beside each picture to rank each from the oldest (1) to the youngest (4). The universe includes everything that exists: all matter,
CHAPTER 4 STARS, GALAXIES & THE UNIVERSE LESSON 1: TELESCOPES ALL TYPES OF ELECTROMAGNETIC RADIATION TRAVEL AT THE SPEED OF LIGHT 186,000 miles per second!! Electromagnetic Radiation = energy that travels
Astronomy 101.003 Hour Exam 2 March 10, 2011 QUESTION 1: The half-life of Ra 226 (radium) is 1600 years. If you started with a sample of 100 Ra 226 atoms, approximately how many Ra 226 atoms would be left
The Night Sky The Universe Chapter 14 Homework: All the multiple choice questions in Applying the Concepts and Group A questions in Parallel Exercises. Celestial observation dates to ancient civilizations
Properties of Stars Characteristics of Stars A constellation is an apparent group of stars originally named for mythical characters. The sky contains 88 constellations. Star Color and Temperature Color
Astronomy Universe: all of space and everything in it Most (90%) of the universe is made up of: dark matter: stuff we think is there due to amount of mass we think is there but is not detected by the instruments
Notepack 23 12/19/2014 Stellar Evolution: Aim: The Life Cycle of a Star Do Now: Where do stars come from? What are they made of? What is a Star? What is a Star? A star is a massive ball of gas that has
Stellar Evolution: Outline Interstellar Medium (dust) Hydrogen and Helium Small amounts of Carbon Dioxide (makes it easier to detect) Massive amounts of material between 100,000 and 10,000,000 solar masses
CHAPTER 28 STARS AND GALAXIES 28.1 A CLOSER LOOK AT LIGHT Light is a form of electromagnetic radiation, which is energy that travels in waves. Waves of energy travel at 300,000 km/sec (speed of light Ex:
Life of a Low-Mass Star AST 101 Introduction to Astronomy: Stars & Galaxies Planetary Nebulae White dwarfs REVIEW END STATE: PLANETARY NEBULA + WHITE DWARF WHAS IS A WHITE DWARF? Exposed core of a low-mass