2022ApJ...928..142S


Query : 2022ApJ...928..142S

2022ApJ...928..142S - Astrophys. J., 928, 142-142 (2022/April-1)

The Number of Possible CETIs within Our Galaxy and the Communication Probability among These CETIs.

SONG W. and GAO H.

Abstract (from CDS):

As the only known intelligent civilization, human beings are always curious about the existence of other communicating extraterrestrial intelligent civilizations (CETIs). Based on the latest astrophysical information, we carry out Monte Carlo simulations to estimate the number of possible CETIs within our Galaxy and the communication probability among them. Two poorly known parameters have a great impact on the results. One is the probability of life appearing on terrestrial planets and eventually evolving into a CETI (fc), and the other determines at what stage of their host star's evolution CETIs would be born (F). In order to ensure the completeness of the simulation, we consider a variety of combinations of fc and F. Our results indicate that for optimistic situations (e.g., F = 25% and fc = 0.1%), there could be 42,777_{-369}^{+267} CETIs and they need to survive for {3}_{-2}^{+17} yr ({2000}_{-1400}^{+2000} yr) to achieve one-way communication (two-way communication). In this case, human beings need to survive {0.3}_{-0.298}^{+0.6} Myr to receive one alien signal. For pessimistic situations (e.g., F = 75% and fc = 0.001%), only {111}_{-17}^{+28} CETIs could be born and they need to survive for {0.8}_{-0.796}^{+1.2} Myr ({0.9}_{-0.88}^{+4.1} Myr) to achieve one-way communication (two-way communication). In this case, human beings need to survive {50}_{-49.6}^{+250} Myr to receive one signal from other CETIs. Our results may quantitatively explain why we have not detected any alien signals so far. The uncertainty of the results has been discussed in detail and would be alleviated with the further improvement of our astronomical observation ability in the future.

Abstract Copyright: © 2022. The Author(s). Published by the American Astronomical Society.

Journal keyword(s): Astrobiology

Simbad objects: 1

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Number of rows : 1
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026
#notes
1 M 13 GlC 16 41 41.634 +36 27 40.75     5.8     ~ 2291 0

Query : 2022ApJ...928..142S

Basic data :
M 13 -- Globular Cluster
Other object types:
otypes_help
GlC (2013A&A,GCl), Cl* (C,[KPS2012]), G (2MASX)
ICRS coord. (ep=J2000) :
16 41 41.634 +36 27 40.75 (Infrared) [ ] C 2006AJ....131.1163S
FK4 coord. (ep=B1950 eq=1950) :
16 39 54.397 +36 33 20.27 [ ]
Gal coord. (ep=J2000) :
059.009475 +40.911761 [ ]
Proper motions mas/yr :
-3.18 -2.56 [0.01 0.01 90] C 2019MNRAS.482.5138B
Radial velocity / Redshift / cz :
V(km/s) -244.4 [0.3] / z(spectroscopic) -0.000815 [0.000001] / cz -244.30 [0.30]
   (Opt) A 2018MNRAS.478.1520B
Parallaxes (mas):
0.127 [0.010] C 2021MNRAS.505.5978V
Angular size (arcmin):
33.00 33.00 0 (~) D 2019MNRAS.489.3093S
Fluxes (8) :
V 5.8 [~] E ~
J 4.452 [0.015] C 2006AJ....131.1163S
H 3.941 [0.015] C 2006AJ....131.1163S
K 3.854 [0.015] C 2006AJ....131.1163S
g (AB) 6.903 [0.005] C 2014MNRAS.437.1725V
r (AB) 6.667 [0.003] C 2014MNRAS.437.1725V
i (AB) 6.397 [0.004] C 2014MNRAS.437.1725V
z (AB) 6.076 [0.002] C 2014MNRAS.437.1725V
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Hierarchy : number of linked objects
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: 527
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Identifiers (7) :
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M 13 GCl 45 NAME Hercules Globular Cluster [KPS2012] MWSC 2445
C 1639+365 2MASX J16414163+3627407 NGC 6205

References (2291 between 1850 and 2026) (Total 2291)
Simbad bibliographic survey began in 1850 for stars (at least bright stars) and in 1983 for all other objects (outside the solar system).
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Collections of Measurements Description of Measurements

Velocities : 4    Distance : 1    Fe/H : 8    Plx : 2    PM : 3   

   

Observing logs
ISO : 1    IUE : 20    XMM : 2   

   


External archives :

Data at NED - NASA/IPAC Extragalactic Database : M 13

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2MASX J16414163+3627407 NGC 6205

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