EFFECT OF METALLICITY ON THE EVOLUTION OF THE HABITABLE ZONE OF LOW MASS STAR

Most stars have habitable zone. Habitable zones are areas in the solar system, or other star systems, which surround the parent star and allow for liquid water to exist. For a planet orbiting a parent star to have habitable zones, it must be at the right distance. Low mass stars are the most stud...

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Main Author: Kresnawati, Nahayuk
Format: Final Project
Language:Indonesia
Online Access:https://digilib.itb.ac.id/gdl/view/46459
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Institution: Institut Teknologi Bandung
Language: Indonesia
id id-itb.:46459
spelling id-itb.:464592020-03-05T14:41:19ZEFFECT OF METALLICITY ON THE EVOLUTION OF THE HABITABLE ZONE OF LOW MASS STAR Kresnawati, Nahayuk Indonesia Final Project Metallicity, Habitable Zone, Low Mass Stars, Location, Evolution INSTITUT TEKNOLOGI BANDUNG https://digilib.itb.ac.id/gdl/view/46459 Most stars have habitable zone. Habitable zones are areas in the solar system, or other star systems, which surround the parent star and allow for liquid water to exist. For a planet orbiting a parent star to have habitable zones, it must be at the right distance. Low mass stars are the most studied because they live longer than high mass stars. When low mass stars, such as the Sun, evolve, the location and time scale of the habitable zone will also shift. In this final project we calculate the evolution of low mass stars, using a stellar code program MESA, with various metallicities to determine the location of the inner and outer boundaries of the habitable zone. Metallicity has a very important role in the evolution of habitable zones. The life of habitable zone of stars with higher metallicity are longer than stars with lower metallicity. text
institution Institut Teknologi Bandung
building Institut Teknologi Bandung Library
continent Asia
country Indonesia
Indonesia
content_provider Institut Teknologi Bandung
collection Digital ITB
language Indonesia
description Most stars have habitable zone. Habitable zones are areas in the solar system, or other star systems, which surround the parent star and allow for liquid water to exist. For a planet orbiting a parent star to have habitable zones, it must be at the right distance. Low mass stars are the most studied because they live longer than high mass stars. When low mass stars, such as the Sun, evolve, the location and time scale of the habitable zone will also shift. In this final project we calculate the evolution of low mass stars, using a stellar code program MESA, with various metallicities to determine the location of the inner and outer boundaries of the habitable zone. Metallicity has a very important role in the evolution of habitable zones. The life of habitable zone of stars with higher metallicity are longer than stars with lower metallicity.
format Final Project
author Kresnawati, Nahayuk
spellingShingle Kresnawati, Nahayuk
EFFECT OF METALLICITY ON THE EVOLUTION OF THE HABITABLE ZONE OF LOW MASS STAR
author_facet Kresnawati, Nahayuk
author_sort Kresnawati, Nahayuk
title EFFECT OF METALLICITY ON THE EVOLUTION OF THE HABITABLE ZONE OF LOW MASS STAR
title_short EFFECT OF METALLICITY ON THE EVOLUTION OF THE HABITABLE ZONE OF LOW MASS STAR
title_full EFFECT OF METALLICITY ON THE EVOLUTION OF THE HABITABLE ZONE OF LOW MASS STAR
title_fullStr EFFECT OF METALLICITY ON THE EVOLUTION OF THE HABITABLE ZONE OF LOW MASS STAR
title_full_unstemmed EFFECT OF METALLICITY ON THE EVOLUTION OF THE HABITABLE ZONE OF LOW MASS STAR
title_sort effect of metallicity on the evolution of the habitable zone of low mass star
url https://digilib.itb.ac.id/gdl/view/46459
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