Formation habitability and_detection_of_extrasolar_moons

Ad

Ad

Ad

Ad

Ad

Ad

Ad

Ad

Ad

Ad

Ad

Ad

Review Article
ASTROBIOLOGY
Volume 14, Number 9, 2014
ª Mary Ann Liebert, Inc.
DOI: 10.1089/ast.2014.1147
Formation, ...

2 HELLER ET AL.
planet around the Sun, Saturn, hosts only one major moon,
Titan. These different architectures were like...

FORMATION, HABITABILITY, AND DETECTION OF EXOMOONS 3
FIG. 1. Europa, Enceladus, Ganymede, and Titan are regarded as poten...

4 HELLER ET AL.
after landing on the surface, penetrating about 10 km of
viscous ice, and diving 100 km or more to the o...

Advertisement

FORMATION, HABITABILITY, AND DETECTION OF EXOMOONS 5
2007). The current heat flux may actually be a remainder
from enhan...

6 HELLER ET AL.
evaporation of surface liquids, condensation into clouds, and
precipitation (Griffith et al., 2000). Ult...

FORMATION, HABITABILITY, AND DETECTION OF EXOMOONS 7
3.1.2. Differences in the jovian and saturnian satellite
systems. A...

8 HELLER ET AL.
FIG. 2. Results after 100 simulations of moon formation around a 10MJup planet. Left panel: Multiplicity ...

FORMATION, HABITABILITY, AND DETECTION OF EXOMOONS 9
near enough to the planet (inside 5–10 planetary radii) to be
tidal...

Advertisement

10 HELLER ET AL.
FIG. 4. Tidal evolution of an Earth-sized moon orbiting a Jupiter-sized planet. Left panels: Semimajor a...

FORMATION, HABITABILITY, AND DETECTION OF EXOMOONS 11
FIG. 5. Evolution of the semimajor axes (aps) and eccentricities (e...

12 HELLER ET AL.
FIG. 6. Evolution of the obliquity (top left), inclination (center left), rotation period (bottom left),...

FORMATION, HABITABILITY, AND DETECTION OF EXOMOONS 13
obliquities of the satellites, whose initial value is set to 11.5
...

14 HELLER ET AL.
does not vary significantly during the first 107 yr because the
planetary tides are not efficient enoug...

Advertisement

FORMATION, HABITABILITY, AND DETECTION OF EXOMOONS 15
of the satellite; and Ws denotes contributions from other
global h...

16 HELLER ET AL.
FIG. 8. Circumplanetary exomoon menageries for Mars-sized satellites around a 10MJup host planet at ages...

FORMATION, HABITABILITY, AND DETECTION OF EXOMOONS 17
distances (10 RJup are in a runaway greenhouse for at least
100 My...

18 HELLER ET AL.
Table 1. Measured Magnetic Properties of Giant Planets in the Solar System
th
S (Rp) R
tidal heating ...

FORMATION, HABITABILITY, AND DETECTION OF EXOMOONS 19
rotational angular velocity as the planet, will produce a
‘‘magnet...

Advertisement

20 HELLER ET AL.
however, is not the only dynamical method of detecting
planets. Notably, Doppler spectroscopy of the ho...

FORMATION, HABITABILITY, AND DETECTION OF EXOMOONS 21
moon’s own transit signal is therefore both a critical and
inextri...

22 HELLER ET AL.
FIG. 13. Transit of the almost Jupiter-sized planet candidate KOI189.01 around a star of about 0.7 solar...

FORMATION, HABITABILITY, AND DETECTION OF EXOMOONS 23
(usually zero), is called ‘‘white noise,’’ and it makes moon
detec...

24 HELLER ET AL.
FIG. 14. Calculated timing errors of the transit mid-time (filled circles) and duration (open circles) f...

Advertisement

FORMATION, HABITABILITY, AND DETECTION OF EXOMOONS 25
Ltid ¼
1=2
6272p7G5
9747
R7s
q9=2
s
lsQs
!
e2
ps
b15=2 ...

26 HELLER ET AL.
FIG. 15. 5r detection limits of JWST’s MIRI for THEMs with radii along the abscissa and effective temper...

FORMATION, HABITABILITY, AND DETECTION OF EXOMOONS 27
FIG. 17. Moon-to-planet mass ratio constraints derived so far by th...

28 HELLER ET AL.
technology, and (iii) can be habitable in terms of atmo-spheric
stability. This regime is roughly betwe...

FORMATION, HABITABILITY, AND DETECTION OF EXOMOONS 29
The James Webb Space Telescope will be sensitive to a
hypothetical...

Advertisement

30 HELLER ET AL.
Anderson, J.D., Lau, E.L., Sjogren, W.L., Schubert, G., and
Moore, W.B. (1996) Gravitational constraint...

FORMATION, HABITABILITY, AND DETECTION OF EXOMOONS 31
Bolmont, E., Raymond, S.N., and Leconte, J. (2011) Tidal
evolution...

32 HELLER ET AL.
Efroimsky, M. and Lainey, V. (2007) Physics of bodily tides in
terrestrial planets and the appropriate ...

FORMATION, HABITABILITY, AND DETECTION OF EXOMOONS 33
Heller, R. (2014) Detecting extrasolar moons akin to Solar
System ...

34 HELLER ET AL.
Kuchner, M.J. (2003) Volatile-rich Earth-Mass planets in the
habitable zone. Astrophys J 596:L105–L108....

Advertisement

FORMATION, HABITABILITY, AND DETECTION OF EXOMOONS 35
from Kepler. VIII. Catalog of transit timing measurements
of the f...

36 HELLER ET AL.
Murray, C.D., and Squyres, S. (2006) Cassini observes the
active south pole of Enceladus. Science 311:1...

FORMATION, HABITABILITY, AND DETECTION OF EXOMOONS 37
satellites. In Jupiter: The Planet, Satellites, and Magnetosphere, ...

38 HELLER ET AL.
(2006) Cassini Ion and Neutral Mass Spectrometer: En-celadus
plume composition and structure. Science 3...

Share Slideshare

LinkedIn
Facebook
Twitter

Embed

Size (px)

Show related Slideshows at end

WordPress Shortcode

Link

Share
Email

Two families of_exocomets_in_the_be... by Sérgio Sacani 601 views
The gaia eso_survey_stellar_content... by Sérgio Sacani 533 views
MUSE sneaks a peek at extreme ram-p... by Sérgio Sacani 658 views
Discovery of carbon_radio_recombina... by Sérgio Sacani 780 views
No xrays from_wasp18_implications_f... by Sérgio Sacani 806 views
Backreaction of hawking_radiation_o... by Sérgio Sacani 1422 views

View on Slideshare

1 of 38 Ad

View on Slideshare

1 of 38 Ad