Homework Week 9 Stellar Properties Based on all of your results, summarize the following properties at the extreme ends of the standard spectral sequence. Temperature: hot or cold Color: red or blue Luminosity: energetic or wimpy Radius: big or small Mass: high mass or low mass Lifetime: long lived or short lived Stars closer to this end of the spectrum are: Stars closer to this end of the spectrum are: 5lifetime = (10 billion years) (280) = 180 million years5) Estimate the lifetime for each star in our data set. Record this information in a table like theone below.Lifetime (years)AsherSun10 billionJunieLafayettePage 4 of 5Homework Week 9-Stellar Properties6) Based on all of your results, summarize the following properties at the extreme ends of thestandard spectral sequence.• Temperature: hot or cold• Color: red or blue• Luminosity: energetic or wimpyRadius: big or smallMass: high mass or low mass• Lifetime: long-lived or short-livedStars closer to this end of thespectrum are:Standard Spectral SequenceOBAFGKMStars closer to this end of thespectrum are:

Asher: The estimated lifetime of a star like Asher, which is a red dwarf with low mass, is much…

Answered: Homework Week 9 Stellar Properties…

Applications and Investigations in Earth Science (9th Edition)

9th Edition

ISBN:9780134746241

Author:Edward J. Tarbuck, Frederick K. Lutgens, Dennis G. Tasa

Publisher:Edward J. Tarbuck, Frederick K. Lutgens, Dennis G. Tasa

Chapter1: The Study Of Minerals

Section: Chapter Questions

Problem 1LR

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Homework Week 9 Stellar Properties Based on all of your results, summarize the following properties at the extreme ends of the standard spectral sequence. Temperature: hot or cold Color: red or blue Luminosity: energetic or wimpy Radius: big or small Mass: high mass or low mass Lifetime: long lived or short lived Stars closer to this end of the spectrum are: Stars closer to this end of the spectrum are: