21st Century Astronomy
21st Century Astronomy
6th Edition
ISBN: 9780393428063
Author: Kay
Publisher: NORTON
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Chapter 17.2, Problem 17.2CYU
To determine

The reason why a high-mass star explodes as a Type II supernova.

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1 A microlensing event with a caustic event is observed with magnifications of 7 and 6 respectively. The characteristic timescale of the main event is 14 days and the caustic timescale is 8 hours. What is the most likely mass of the lense star and candidate planet?
fill in missing word a) One difference between a type I and type II supernova is the formation of the element  _________ in the core that produces a type II supernova b) The Chandrasekhar limit of a star (1.4 solar masses) is the mass limit above which a star cannot remain stable as a ________ ________. c) The temperature of a red giant star is ____________ than it was when the star was a dwarf.
1. The Sun’s mass is ~2x1030 kg. If 10% of this is Hydrogen available in the core, how long will the Sun be able to continue fusing hydrogen at this rate? This is considered the Sun's "lifetime". If the Sun is 4.6 billion years old (and assuming it's power output is constant), how many years does it have left?
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