Hostname: page-component-586b7cd67f-l7hp2 Total loading time: 0 Render date: 2024-11-22T06:01:08.699Z Has data issue: false hasContentIssue false

Exploring the Galaxy using space probes

Published online by Cambridge University Press:  20 April 2007

R. Bjørk
Affiliation:
Niels Bohr Institute, Juliane Maries vej 32, DK-2100 Copenhagen Ø, Denmark e-mail: [email protected]

Abstract

This paper investigates the possible use of space probes to explore the Milky Way, as a means both of finding life elsewhere in the Galaxy and as finding an answer to the Fermi paradox. Exploration of the Galaxy is simulated by first examining how long time it takes a given number of space probes to explore 40 000 stars in a box from −300 to 300 pc above the Galactic thin disc, as a function of Galactic radius. The Galaxy is then modelled to consist of ∼260 000 of these 40 000 stellar systems all located in a defined Galactic Habitable Zone and how long a time it takes to explore this zone is shown. The result is that with eight probes, each with eight subprobes, ∼4% of the Galaxy can be explored in 2.92×108 years. Increasing the number of probes to 200, still with eight subprobes each, reduces the exploration time to 1.52×107 years.

Type
Research Article
Copyright
Copyright © Cambridge University Press 2007

Access options

Get access to the full version of this content by using one of the access options below. (Log in options will check for institutional or personal access. Content may require purchase if you do not have access.)

References

Allan, C.W. (1973). Astrophysical Quantities, 3rd edn. Athlone Press, London.Google Scholar
Chyba, C.F. & Hand, K.P. (2005). Astrobiology: the study of the living universe. Ann. Rev. Astron. Astrophys. 43, 3174.CrossRefGoogle Scholar
Gilmore, G. & Reid, I.N. (1983). The vertical structure of the Milky Way’s stellar disk. Mon. Not. R. Astron. Soc. 202, 1025.CrossRefGoogle Scholar
Lineweaver, C.H., Fenner, Y. & Gibson, B.K. (2004). The Galactical Habitable Zone and the age distribution of complex life in the Milky Way. Science 303, 5962.CrossRefGoogle ScholarPubMed
Lissauer, J.J., Quintana, E.V., Chambers, J.E., Duncan, M.J. & Adams, F.C. (2004). Terrestrial planet formation in binary star systems. Rev. Mex. Astron. Assoc. 22, 99103.Google Scholar
Lpez-Corredoira, M., Cabrera-Lavers, A., Garzn, F. & Hammersley, P.L. (2002). Old stellar Galactic disc in near-plane regions according to 2MASS: scales, cut-off, flare and warp. Astron. Astrophys. 394, 883899.CrossRefGoogle Scholar
Peña-Cabrera, G.V.Y. & Durand-Manterola, H.J. (2004), Possible biotic distribution in our galaxy. Adv. Space Res. 33, 114117.CrossRefGoogle Scholar
Sackett, P.D. (1997). Does the Milky Way have a maximal disk? Astrophys. J. 483, 103110.CrossRefGoogle Scholar
Spergel, D.N. et al. (2007). Wilkinson Microwave Anisotropy Probe (WMAP) three year results: implications for cosmology. Astrophys. J., in press, astro-ph/0603449.CrossRefGoogle Scholar
Tipler, F.J. (1980). Extraterrestrial intelligent beings do not exist. Q. J. R. Astron. Soc. 21, 267281.Google Scholar
Zheng, Z., Flynn, C., Gould, A., Bahcall, J.N. & Salim, S. (2001). M dwarfs from Hubble Space Telescope star counts. Astrophys. J. 555, 394404.CrossRefGoogle Scholar