2016ApJ...827...54D


Query : 2016ApJ...827...54D

2016ApJ...827...54D - Astrophys. J., 827, 54-54 (2016/August-2)

Globular clusters as cradles of life and advanced civilizations.

DI STEFANO R. and RAY A.

Abstract (from CDS):

Globular clusters are ancient stellar populations in compact dense ellipsoids. There is no star formation and there are no core-collapse supernovae, but several lines of evidence suggest that globular clusters are rich in planets. If so, and if advanced civilizations can develop there, then the distances between these civilizations and other stars would be far smaller than typical distances between stars in the Galactic disk, facilitating interstellar communication and travel. The potent combination of long-term stability and high stellar densities provides a globular cluster opportunity. Yet the very proximity that promotes interstellar travel also brings danger, as stellar interactions can destroy planetary systems. We find, however, that large portions of many globular clusters are "sweet spots," where habitable-zone planetary orbits are stable for long times. Globular clusters in our own and other galaxies are, therefore, among the best targets for searches for extraterrestrial intelligence (SETI). We use the Drake equation to compare the likelihood of advanced civilizations in globular clusters to that in the Galactic disk. We also consider free-floating planets, since wide-orbit planets can be ejected to travel through the cluster. Civilizations spawned in globular clusters may be able to establish self-sustaining outposts, reducing the probability that a single catastrophic event will destroy the civilization. Although individual civilizations may follow different evolutionary paths, or even be destroyed, the cluster may continue to host advanced civilizations once a small number have jumped across interstellar space. Civilizations residing in globular clusters could therefore, in a sense, be immortal.

Abstract Copyright: © 2016. The American Astronomical Society. All rights reserved.

Journal keyword(s): galaxies: star clusters: general - globular clusters: general - planetary systems - planets and satellites: dynamical evolution and stability - planets and satellites: dynamical evolution and stability

Simbad objects: 31

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Number of rows : 31
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2024
#notes
1 NGC 104 GlC 00 24 05.359 -72 04 53.20     4.09     ~ 3917 0
2 NGC 1851 GlC 05 14 06.76 -40 02 47.6           ~ 1430 0
3 NAME Virgo Cluster ClG 12 26 32.1 +12 43 24           ~ 6647 0
4 M 53 GlC 13 12 55.25 +18 10 05.4     7.79     ~ 836 0
5 M 3 GlC 13 42 11.62 +28 22 38.2     6.39     ~ 2479 0
6 M 5 GlC 15 18 33.22 +02 04 51.7     5.95     ~ 1978 0
7 NGC 5986 GlC 15 46 03.00 -37 47 11.1     6.92     ~ 374 0
8 M 4 GlC 16 23 35.22 -26 31 32.7           ~ 1850 0
9 PSR B1620-26 Psr 16 23 38.2218 -26 31 53.769     21.30     ~ 295 2
10 M 13 GlC 16 41 41.634 +36 27 40.75     5.8     ~ 2193 0
11 M 62 GlC 17 01 12.60 -30 06 44.5           ~ 620 0
12 NGC 6342 GlC 17 21 10.14 -19 35 14.7     10.01     ~ 286 0
13 NGC 6397 GlC 17 40 42.09 -53 40 27.6     5.17     ~ 1976 0
14 Cl Terzan 5 Cl* 17 48 05.00 -24 46 48.0           ~ 847 1
15 NGC 6440 GlC 17 48 52.67 -20 21 34.5           ~ 551 0
16 NGC 6441 GlC 17 50 13.06 -37 03 05.2           ~ 884 0
17 NGC 6517 GlC 18 01 50.376 -08 57 34.39   11.08       ~ 182 0
18 NGC 6522 GlC 18 03 34.08 -30 02 02.3           ~ 524 0
19 NGC 6539 GlC 18 04 49.74 -07 35 09.1           ~ 225 0
20 NGC 6544 GlC 18 07 20.58 -24 59 50.4   11.36 9.90     ~ 296 0
21 NGC 6624 GlC 18 23 40.51 -30 21 39.7           ~ 886 1
22 M 28 GlC 18 24 32.89 -24 52 11.4           ~ 770 0
23 NGC 6652 GlC 18 35 45.63 -32 59 26.6           ~ 439 0
24 M 22 GlC 18 36 23.94 -23 54 17.1           ~ 1379 0
25 NGC 6749 OpC 19 05 15.36 +01 54 00.0     12.4     ~ 157 0
26 NGC 6752 GlC 19 10 52.11 -59 59 04.4           ~ 2001 0
27 NGC 6760 GlC 19 11 12.06 +01 01 49.7   11.37 9.78     ~ 240 0
28 NGC 6811 OpC 19 37 21.6 +46 22 41   7.47 6.8     ~ 378 0
29 M 71 GlC 19 53 46.49 +18 46 45.1           ~ 1128 0
30 M 15 GlC 21 29 58.33 +12 10 01.2           ~ 3140 0
31 M 30 GlC 21 40 22.12 -23 10 47.5     7.10     ~ 1049 0

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