The Galactic Habitable Zone: Galactic Chemical Evolution

Abstract

We propose the concept of a "Galactic Habitable Zone" (GHZ). Analogous to the Circumstellar Habitable Zone (CHZ), the GHZ is that region in the Milky Way where an Earth-like planet can retain liquid water on its surface and provide a long-term habitat for animal-like aerobic life. In this paper we examine the dependence of the GHZ on Galactic chemical evolution. The single most important factor is likely the dependence of terrestrial planet mass on the metallicity of its birth cloud. We estimate, very approximately, that a metallicity at least half that of the Sun is required to build a habitable terrestrial planet. The mass of a terrestrial planet has important consequences for interior heat loss, volatile inventory, and loss of atmosphere. A key issue is the production of planets that sustain plate tectonics, a critical recycling process that provides feedback to stabilize atmospheric temperatures on planets with oceans and atmospheres. Due to the more recent decline from the early intense star formation activity in the Milky Way, the concentration in the interstellar medium of the geophysically important radioisotopes, 40 K, 235,238 U, 232 Th, has been declining relative to Fe, an abundant element in the Earth. Also likely important are the relative abundances of Si and Mg to Fe, which affects the mass of the core relative to the mantle in a terrestrial planet. All these elements and isotopes vary with time and location in the Milky Way; thus, planetary systems forming in other locations and times in the Milky Way with the same metallicity as the Sun will not necessarily form habitable Earth-like planets. As a result of the radial Galactic metallicity gradient, the outer limit of the GHZ is set primarily by the minimum required metallicity to build large terrestrial planets. Regions of the Milky Way least likely to contain Earth-mass planets are the halo (including globular clusters), the thick disk, and the outer thin -3 -disk. The bulge should contain Earth-mass planets, but stars in it have a mix of elements different from the Sun's. The existence of a luminosity-metallicity correlation among galaxies of all types means that many galaxies are too metal-poor to contain Earth-mass planets. Based on the observed luminosity function of nearby galaxies in the visual passband, we estimate that: 1) the Milky Way is among the 1.3% most luminous (and hence most metal-rich) galaxies, and 2) about 23% of stars in a typical ensemble of galaxies are more metal-rich than the average star in the Milky Way. The GHZ zone concept can be easily extrapolated to the universe as a whole, especially with regard to the changing star formation rate and its effect on metallicity and abundances of the long-lived radioisotopes.

The Penn State-Toruń Centre for Astronomy Planet Search stars

“…Since the complete sample contains ∼1000 stars randomly distributed in the skies, it is of interest for general stellar and galactic astrophysics as well. It may be used for studies of galactic structure and evolution, galactic distribution of planetary systems (Haywood 2009), and the galactic habitable zone (Gonzalez et al 2001;Lineweaver et al 2004;McCabe & Lucas 2010;Gowanlock et al 2011).…”

Integrando o ensino de astronomia e termodinâmica: explorando a zona habitável no diagrama de fases da água

“…Para serem considerados habitáveis na Via Láctea, os sistemas estelares devem permanecer a uma distância razoável do conturbado centro galáctico, uma região de intensa formação de estrelas, atividades de supernovas, emissão de raios gama, assim como perturbações gravitacionais [8]. Por outro lado, estrelas muito afastadas do centro estão em uma região de baixa metalicidade 6 , onde a abundância de elementos que formam os planetas terrestresé baixa.…”

Galactic planar tides on the comets of Oort Cloud and analogs in different reference systems. I.

“…That may lead to a redefinition of the boundaries for the Galactic habitable zone. Several Galactic-scale factors can influence indeed the belonging to GHZ for a star (Gonzalez et al 2001;Gonzalez 2005;Lineweaver et al 2004;Gowanlock et al 2010): they include those which are relevant to the formation of planets, such as radial disk metallicity gradient, and moreover the events that can threaten Life such as nearby supernovae and gamma ray bursts. There are at least two ways in which they might be involved into the process of Life formation and development.…”