ANALISIS PENGARUH MASSA DAN METALISITAS BINTANG DERET UTAMA BERMASSA RENDAH KELAS SPEKTRUM F, G, DAN K TERHADAP EVOLUSI HABITABLE ZONE

ANALISIS PENGARUH MASSA DAN METALISITAS BINTANG DERET UTAMA BERMASSA RENDAH KELAS SPEKTRUM F, G, DAN K TERHADAP EVOLUSI HABITABLE ZONE

Habitable zone (HZ) is an area in the Solar System or other star system, which surrounds the parent star and allows the presence of liquid water. For a planet orbiting its parent star to have a habitable zone, it must be at the right distance. When a star evolves, the habitable zone will also evolve...

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Main Author: Novita Wuri, Arum
Format: Final Project
Language:Indonesia
Subjects:
Teknik (Rekayasa, enjinering dan kegiatan berkaitan)
Online Access:https://digilib.itb.ac.id/gdl/view/55266
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Institution: Institut Teknologi Bandung
Language: Indonesia
id id-itb.:55266
spelling id-itb.:552662021-06-16T17:00:44ZANALISIS PENGARUH MASSA DAN METALISITAS BINTANG DERET UTAMA BERMASSA RENDAH KELAS SPEKTRUM F, G, DAN K TERHADAP EVOLUSI HABITABLE ZONE Novita Wuri, Arum Teknik (Rekayasa, enjinering dan kegiatan berkaitan) Indonesia Final Project Habitable Zone, Low Mass Main Sequence Stars Class F, G, K, Mass, Metallicity, Evolution INSTITUT TEKNOLOGI BANDUNG https://digilib.itb.ac.id/gdl/view/55266 Habitable zone (HZ) is an area in the Solar System or other star system, which surrounds the parent star and allows the presence of liquid water. For a planet orbiting its parent star to have a habitable zone, it must be at the right distance. When a star evolves, the habitable zone will also evolve. This evolution is influenced by several parameters, including mass and metallicity. This research uses low mass main sequence stars (? 2 M?) of spectrum class F, G, K, because they have a lifespan of up to 10 billion years, sufficient time for life to develop in their planetary system. In this final project, the evolution process of low mass main sequence star class F, G, K, with various levels of mass and metallicity is carried out using the MESA WEB star evolution program to obtain the required data related to the analysis of the effect of mass and metallicity of stars on the habitable zone of stars 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
topic Teknik (Rekayasa, enjinering dan kegiatan berkaitan)
spellingShingle Teknik (Rekayasa, enjinering dan kegiatan berkaitan)
Novita Wuri, Arum
ANALISIS PENGARUH MASSA DAN METALISITAS BINTANG DERET UTAMA BERMASSA RENDAH KELAS SPEKTRUM F, G, DAN K TERHADAP EVOLUSI HABITABLE ZONE
description Habitable zone (HZ) is an area in the Solar System or other star system, which surrounds the parent star and allows the presence of liquid water. For a planet orbiting its parent star to have a habitable zone, it must be at the right distance. When a star evolves, the habitable zone will also evolve. This evolution is influenced by several parameters, including mass and metallicity. This research uses low mass main sequence stars (? 2 M?) of spectrum class F, G, K, because they have a lifespan of up to 10 billion years, sufficient time for life to develop in their planetary system. In this final project, the evolution process of low mass main sequence star class F, G, K, with various levels of mass and metallicity is carried out using the MESA WEB star evolution program to obtain the required data related to the analysis of the effect of mass and metallicity of stars on the habitable zone of stars
format Final Project
author Novita Wuri, Arum
author_facet Novita Wuri, Arum
author_sort Novita Wuri, Arum
title ANALISIS PENGARUH MASSA DAN METALISITAS BINTANG DERET UTAMA BERMASSA RENDAH KELAS SPEKTRUM F, G, DAN K TERHADAP EVOLUSI HABITABLE ZONE
title_short ANALISIS PENGARUH MASSA DAN METALISITAS BINTANG DERET UTAMA BERMASSA RENDAH KELAS SPEKTRUM F, G, DAN K TERHADAP EVOLUSI HABITABLE ZONE
title_full ANALISIS PENGARUH MASSA DAN METALISITAS BINTANG DERET UTAMA BERMASSA RENDAH KELAS SPEKTRUM F, G, DAN K TERHADAP EVOLUSI HABITABLE ZONE
title_fullStr ANALISIS PENGARUH MASSA DAN METALISITAS BINTANG DERET UTAMA BERMASSA RENDAH KELAS SPEKTRUM F, G, DAN K TERHADAP EVOLUSI HABITABLE ZONE
title_full_unstemmed ANALISIS PENGARUH MASSA DAN METALISITAS BINTANG DERET UTAMA BERMASSA RENDAH KELAS SPEKTRUM F, G, DAN K TERHADAP EVOLUSI HABITABLE ZONE
title_sort analisis pengaruh massa dan metalisitas bintang deret utama bermassa rendah kelas spektrum f, g, dan k terhadap evolusi habitable zone
url https://digilib.itb.ac.id/gdl/view/55266
_version_ 1822929857719304192

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