Survey
* Your assessment is very important for improving the work of artificial intelligence, which forms the content of this project
* Your assessment is very important for improving the work of artificial intelligence, which forms the content of this project
90764 2 907640 SUPERVISOR’S USE ONLY Level 2 Science, 2011 90764 Describe the nature and life cycle of stars 2.00 pm������������������������ �������������������������� Friday 25�������������� ���������������� November 2011 Credits: Two Check that the National Student Number (NSN) on your admission slip is the same as the number at the top of this page. You should attempt ALL the questions in this booklet. If you need more room for any answer, use the extra space provided at the back of this booklet. Check that this booklet has pages 2 – 10 in the correct order and that none of these pages is blank. YOU MUST HAND THIS BOOKLET TO THE SUPERVISOR AT THE END OF THE EXAMINATION. ASSESSOR’S USE ONLY Achievement Describe the nature and life cycle of stars. Achievement Criteria Achievement with Merit Explain the nature of stars and their life cycle. Achievement with Excellence Discuss the nature of stars and their life cycle. Overall level of performance © New Zealand Qualifications Authority, 2011. All rights reserved. No part of this publication may be reproduced by any means without the prior permission of the New Zealand Qualifications Authority. 2 You are advised to spend 25 minutes answering the questions in this booklet. RESOURCE The Hertzsprung-Russell (H-R) Diagram compares the real brightness of stars (in terms of their Absolute Magnitude: –8 very bright, +16 very faint) with their colour (Spectral Type). Hertzsprung-Russell Diagram Surface Temperature (Kelvin) 10 000 50 000 4 000 Blue Supergiants –8 –4 –2 Red Giants Betelgeuse Canopus ß Centauri α Crucis ß Crucis Spica μ Cephei ε Aurigae Deneb Rigel –6 Absolute Magnitude 6 000 Antares Alphard Arcturus Pollux Regulus 0 Vega Sirius A 2 Fomalhaut Altair Aldebaran Procyon A 4 Sun α Centauri A 40 Eridani A 6 8 10 Sirius B 12 Procyon B 14 16 40 Eridani B Barnard’s Star proxima Centauri 1 5 O 9 1 5 B 9 1 5 A 9 1 5 F 9 1 Spectral Type 5 G Science 90764, 2011 9 1 5 K 9 1 5 M 9 3 This page has been deliberately left blank. 4 QUESTION ONE ASSESSOR’S USE ONLY In April 2010, a group of astronomers reported the discovery of a brown dwarf only 10 light years from our sun. A brown dwarf has a similar composition of gases as our Sun, but it is a failed star. For copyright reasons, this resource cannot be reproduced here. The Sun For copyright reasons, this resource cannot be reproduced here. http://upload.wikimedia.org/wikipedia/commons/b/b4/ The_Sun_by_the_Atmospheric_Imaging_Assembly_of_ NASA%27s_Solar_Dynamics_Observatory_-_20100819. jpg Brown Dwarf http://2.bp.blogspot.com/_NsNjn35go9Y/TCeBgHcszRI/ AAAAAAAAA8A/8BkkLsdd7FE/s1600/browndwarf.jpg Discuss why the brown dwarf has not developed into a star like our Sun. In your answer you should refer to: • • • • • star formation size mass luminosity fuel usage. You may wish to use a labelled diagram in your answer. Science 90764, 2011 5 ASSESSOR’S USE ONLY Science 90764, 2011 6 QUESTION TWO ASSESSOR’S USE ONLY The brightest star in the night sky is Sirius A. This star is 8.7 light years from Earth. It is 40 times more luminous and twice the size of our sun. For copyright reasons, this resource cannot be reproduced here. X-ray image of Sirius A and Sirius B http://destinationterre2.files.wordpress.com/2010/03/siriusb_cxo_big.jpg Sirius A has a companion star know as the “Pup” or Sirius B. This star cannot be seen by the naked eye. As Sirius B orbits around Sirius A, it makes Sirius A wobble. Using the H-R diagram, discuss the characteristics of Sirius A and Sirius B. Contrast the two stars and explain why Sirius B causes Sirius A to wobble. Points you may consider are: • • • • • star types star size fuel use gravitational forces star composition. You may wish to use a labelled diagram in your answer. Science 90764, 2011 7 ASSESSOR’S USE ONLY Science 90764, 2011 8 QUESTION THREE ASSESSOR’S USE ONLY The Large Magellanic Cloud (LMC) is a globular galaxy that forms a companion to our galaxy, the Milky Way. It is 168 000 light years away from our galaxy. In 1967 a Supernova was observed in the LMC. For copyright reasons, this resource cannot be reproduced here. Image of the supernova in the LMC http://www.eso.org/public/images/eso0437c/ Discuss what happens when a supernova occurs. In your answer you should refer to: • • • • original star type and size steps that lead to the supernova explanation of the appearance of supernova what happens during and after a supernova. You may wish to use a labelled diagram in your answer. Science 90764, 2011 9 ASSESSOR’S USE ONLY Science 90764, 2011 10 QUESTION NUMBER Extra space if required. Write the question number(s) if applicable. Science 90764, 2011 ASSESSOR’S USE ONLY 90764