The Habitability of the Galactic Bulge

We present a new investigation of the habitability of the Milky Way bulge, that expands previous studies on the Galactic Habitable Zone. We discuss existing knowledge on the abundance of planets in the bulge, metallicity and the possible frequency of rocky planets, orbital stability and encounters,...

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Main Authors: Amedeo Balbi, Maryam Hami, Andjelka Kovačević
Format: Article
Language:English
Published: MDPI AG 2020-08-01
Series:Life
Subjects:
Online Access:https://www.mdpi.com/2075-1729/10/8/132
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spelling doaj-ed5b115c926b4de39e9e6c10f08bfd7b2020-11-25T01:27:02ZengMDPI AGLife2075-17292020-08-011013213210.3390/life10080132The Habitability of the Galactic BulgeAmedeo Balbi0Maryam Hami1Andjelka Kovačević2Dipartimento di Fisica, Università di Roma “Tor Vergata”, Via della Ricerca Scientifica, 00133 Roma, ItalyDipartimento di Fisica, Università di Roma “Tor Vergata”, Via della Ricerca Scientifica, 00133 Roma, ItalyDepartment of Astronomy, Faculty of Mathematics, University of Belgrade, Studentski trg 16, 11000 Belgrade, SerbiaWe present a new investigation of the habitability of the Milky Way bulge, that expands previous studies on the Galactic Habitable Zone. We discuss existing knowledge on the abundance of planets in the bulge, metallicity and the possible frequency of rocky planets, orbital stability and encounters, and the possibility of planets around the central supermassive black hole. We focus on two aspects that can present substantial differences with respect to the environment in the disk: (i) the ionizing radiation environment, due to the presence of the central black hole and to the highest rate of supernovae explosions and (ii) the efficiency of putative lithopanspermia mechanism for the diffusion of life between stellar systems. We use analytical models of the star density in the bulge to provide estimates of the rate of catastrophic events and of the diffusion timescales for life over interstellar distances.https://www.mdpi.com/2075-1729/10/8/132astrobiologyhabitabilityexoplanetsGalactic Habitable ZoneMilky Way bulge
collection DOAJ
language English
format Article
sources DOAJ
author Amedeo Balbi
Maryam Hami
Andjelka Kovačević
spellingShingle Amedeo Balbi
Maryam Hami
Andjelka Kovačević
The Habitability of the Galactic Bulge
Life
astrobiology
habitability
exoplanets
Galactic Habitable Zone
Milky Way bulge
author_facet Amedeo Balbi
Maryam Hami
Andjelka Kovačević
author_sort Amedeo Balbi
title The Habitability of the Galactic Bulge
title_short The Habitability of the Galactic Bulge
title_full The Habitability of the Galactic Bulge
title_fullStr The Habitability of the Galactic Bulge
title_full_unstemmed The Habitability of the Galactic Bulge
title_sort habitability of the galactic bulge
publisher MDPI AG
series Life
issn 2075-1729
publishDate 2020-08-01
description We present a new investigation of the habitability of the Milky Way bulge, that expands previous studies on the Galactic Habitable Zone. We discuss existing knowledge on the abundance of planets in the bulge, metallicity and the possible frequency of rocky planets, orbital stability and encounters, and the possibility of planets around the central supermassive black hole. We focus on two aspects that can present substantial differences with respect to the environment in the disk: (i) the ionizing radiation environment, due to the presence of the central black hole and to the highest rate of supernovae explosions and (ii) the efficiency of putative lithopanspermia mechanism for the diffusion of life between stellar systems. We use analytical models of the star density in the bulge to provide estimates of the rate of catastrophic events and of the diffusion timescales for life over interstellar distances.
topic astrobiology
habitability
exoplanets
Galactic Habitable Zone
Milky Way bulge
url https://www.mdpi.com/2075-1729/10/8/132
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