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The quest for cradles of life: using the fundamental metallicity relation to hunt for the most habitable type of galaxy

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The quest for cradles of life : using the fundamental metallicity relation to hunt for the most habitable type of galaxy . / Dayal, Pratika; Cockell, Charles; Rice, Ken; Mazumdar, Anupam.

In: Astrophysical Journal Letters, Vol. 810, No. 1, L2, 21.08.2015.

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Dayal, Pratika ; Cockell, Charles ; Rice, Ken ; Mazumdar, Anupam. / The quest for cradles of life : using the fundamental metallicity relation to hunt for the most habitable type of galaxy . In: Astrophysical Journal Letters. 2015 ; Vol. 810, No. 1.

Bibtex

@article{09aa34d1f8884f7db728e035c90700f7,
title = "The quest for cradles of life: using the fundamental metallicity relation to hunt for the most habitable type of galaxy ",
abstract = "The field of astrobiology has made huge strides in understanding the habitable zones around stars (stellar habitable zones) where life can begin, sustain its existence and evolve into complex forms. A few studies have extended this idea by modeling galactic-scale habitable zones (galactic habitable zones) for our Milky Way (MW) and specific elliptical galaxies. However, estimating the habitability for galaxies spanning a wide range of physical properties has so far remained an outstanding issue. Here, we present a {"}cosmobiological{"} framework that allows us to sift through the entire galaxy population in the local universe and answer the question, {"}Which type of galaxy is most likely to host complex life in the cosmos?{"} Interestingly, the three key astrophysical criteria governing habitability (total mass in stars, total metal mass and ongoing star formation rate) are found to be intricately linked through the {"}fundamental metallicity relation{"} as shown by Sloan Digital Sky Survey observations of more than a hundred thousand galaxies in the local universe. Using this relation we show that metal-rich, shapeless giant elliptical galaxies at least twice as massive as the MW (with a tenth of its star formation rate) can potentially host ten thousand times as many habitable (Earth-like) planets, making them the most probable {"}cradles of life{"} in the universe.",
keywords = "astrobiology , galaxies: elliptical and lenticular, cD, galaxies: fundamental parameters, galaxies: spiral, Galaxy: fundamental parameters, methods: analytical",
author = "Pratika Dayal and Charles Cockell and Ken Rice and Anupam Mazumdar",
year = "2015",
month = aug,
day = "21",
doi = "10.1088/2041-8205/810/1/L2",
language = "English",
volume = "810",
journal = "Astrophysical Journal Letters",
issn = "2041-8205",
publisher = "IOP Publishing Ltd",
number = "1",

}

RIS

TY - JOUR

T1 - The quest for cradles of life

T2 - using the fundamental metallicity relation to hunt for the most habitable type of galaxy

AU - Dayal, Pratika

AU - Cockell, Charles

AU - Rice, Ken

AU - Mazumdar, Anupam

PY - 2015/8/21

Y1 - 2015/8/21

N2 - The field of astrobiology has made huge strides in understanding the habitable zones around stars (stellar habitable zones) where life can begin, sustain its existence and evolve into complex forms. A few studies have extended this idea by modeling galactic-scale habitable zones (galactic habitable zones) for our Milky Way (MW) and specific elliptical galaxies. However, estimating the habitability for galaxies spanning a wide range of physical properties has so far remained an outstanding issue. Here, we present a "cosmobiological" framework that allows us to sift through the entire galaxy population in the local universe and answer the question, "Which type of galaxy is most likely to host complex life in the cosmos?" Interestingly, the three key astrophysical criteria governing habitability (total mass in stars, total metal mass and ongoing star formation rate) are found to be intricately linked through the "fundamental metallicity relation" as shown by Sloan Digital Sky Survey observations of more than a hundred thousand galaxies in the local universe. Using this relation we show that metal-rich, shapeless giant elliptical galaxies at least twice as massive as the MW (with a tenth of its star formation rate) can potentially host ten thousand times as many habitable (Earth-like) planets, making them the most probable "cradles of life" in the universe.

AB - The field of astrobiology has made huge strides in understanding the habitable zones around stars (stellar habitable zones) where life can begin, sustain its existence and evolve into complex forms. A few studies have extended this idea by modeling galactic-scale habitable zones (galactic habitable zones) for our Milky Way (MW) and specific elliptical galaxies. However, estimating the habitability for galaxies spanning a wide range of physical properties has so far remained an outstanding issue. Here, we present a "cosmobiological" framework that allows us to sift through the entire galaxy population in the local universe and answer the question, "Which type of galaxy is most likely to host complex life in the cosmos?" Interestingly, the three key astrophysical criteria governing habitability (total mass in stars, total metal mass and ongoing star formation rate) are found to be intricately linked through the "fundamental metallicity relation" as shown by Sloan Digital Sky Survey observations of more than a hundred thousand galaxies in the local universe. Using this relation we show that metal-rich, shapeless giant elliptical galaxies at least twice as massive as the MW (with a tenth of its star formation rate) can potentially host ten thousand times as many habitable (Earth-like) planets, making them the most probable "cradles of life" in the universe.

KW - astrobiology

KW - galaxies: elliptical and lenticular, cD

KW - galaxies: fundamental parameters

KW - galaxies: spiral

KW - Galaxy: fundamental parameters

KW - methods: analytical

U2 - 10.1088/2041-8205/810/1/L2

DO - 10.1088/2041-8205/810/1/L2

M3 - Journal article

VL - 810

JO - Astrophysical Journal Letters

JF - Astrophysical Journal Letters

SN - 2041-8205

IS - 1

M1 - L2

ER -