2022A&A...664A..59M


Query : 2022A&A...664A..59M

2022A&A...664A..59M - Astronomy and Astrophysics, volume 664A59-59 (2022/8-1)

Exoplanet cartography using convolutional neural networks.

MEINKE K., STAM D.M. and VISSER P.M.

Abstract (from CDS):


Context. In the near future, dedicated telescopes will observe Earth-like exoplanets in reflected parent starlight, allowing their physical characterization. Because of the huge distances, every exoplanet will remain an unresolved, single pixel, but temporal variations in the pixel's spectral flux contain information about the planet's surface and atmosphere.
Aims. We tested convolutional neural networks for retrieving a planet's rotation axis, surface, and cloud map from simulated single-pixel observations of flux and polarization light curves. We investigated the influence of assuming that the reflection by the planets is Lambertian in the retrieval while in reality their reflection is bidirectional, and the influence of including polarization.
Methods. We simulated observations along a planet's orbit using a radiative transfer algorithm that includes polarization and bidirectional reflection by vegetation, deserts, oceans, water clouds, and Rayleigh scattering in six spectral bands from 400 to 800 nm, at various levels of photon noise. The surface types and cloud patterns of the facets covering a model planet are based on probability distributions. Our networks were trained with simulated observations of millions of planets before retrieving maps of test planets.
Results. The neural networks can constrain rotation axes with a mean squared error (MSE) as small as 0.0097, depending on the orbital inclination. On a bidirectionally reflecting planet, 92% of ocean facets and 85% of vegetation, deserts, and cloud facets are correctly retrieved, in the absence of noise. With realistic amounts of noise, it should still be possible to retrieve the main map features with a dedicated telescope. Except for face-on orbits, a network trained with Lambertian reflecting planets yields significant retrieval errors when given observations of bidirectionally reflecting planets, in particular, brightness artifacts around a planet's pole. Including polarization improves the retrieval of the rotation axis and the accuracy of the retrieval of ocean and cloudy map facets.

Abstract Copyright: © K. Meinke et al. 2022

Journal keyword(s): planets and satellites: surfaces - planets and satellites: oceans - planets and satellites: atmospheres - techniques: photometric - techniques: polarimetric - techniques: image processing

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 * alf Cen ** 14 39 36.50 -60 50 02.3   0.4 -0.1     G2V+K1V 1031 0

Query : 2022A&A...664A..59M

Basic data :
* alf Cen -- Double or Multiple Star
Other object types:
otypes_help
* (2012ApJ,*,...), X (1E,2E,...), ** (CCDM,**,...), UV (2EUVE,EUVE,...), PM* (Ci,PM), IR (IRAS)
ICRS coord. (ep=J2000) :
14 39 36.50 -60 50 02.3 (Optical) [ ] D 2001AJ....122.3466M
FK4 coord. (ep=B1950 eq=1950) :
14 36 11.50 -60 37 43.1 [ ]
Gal coord. (ep=J2000) :
315.73419 -00.67964 [ ]
Proper motions mas/yr :
-3608 686 [30 25 179] C ~
Radial velocity / Redshift / cz :
V(km/s) -22.3 [0.9] / z(~) -0.000074 [0.000003] / cz -22.30 [0.90]
   A 1979IAUS...30...57E
Parallaxes (mas):
750.81 [0.38] B 2021AJ....162...14A
Spectral type:
G2V+K1V C 2006A&A...460..695T
Fluxes (2) :
B 0.4 [~] E ~
V -0.1 [~] E ~
SIMBAD within arcmin
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Hierarchy : number of linked objects
whatever the membership probability is (see description here ) :

: 2
Display criteria :

Identifiers (34) :
An access of full data is available using the icon Vizier near the identifier of the catalogue

CCDM J14396-6050AB 1E 143555-6037.6 GES J14392972-6049560 RX J1439.5-6050
* alf Cen 2E 3308 IDS 14328-6025 AB 1RXS J143940.4-605020
** RHD 1 2E 1435.9-6037 IRAS 14359-6037 SAO 252838
** LDS 494AB 1ES 1435-60.6 LPM 534 uvby98 100128620
CD-60 5293 2EUVE J1439-60.8 PM 14362-6038 WDS J14396-6050AB
Ci 20 875 EUVE J1439-60.8 2RE J143941-605000 2XMM J143933.0-605008
CPD-60 5483 FK5 538 2RE J1439-605 [TSA98] J143948.42-605021.66
CSI-60 5483 43 GC 19728 RE J1439-605
1E 143556-6037.3 GCRV 8519 RE J143944-605008

References (1031 between 1850 and 2026) (Total 1031)
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 : 3    Fe/H : 1    Plx : 1    PM : 2   

   

Observing logs
ISO : 5    XMM : 7   

   


External archives :

Archive data at HEASARC - High-Energy Astrophysics Science Archive Research Center

Data at NED - NASA/IPAC Extragalactic Database : * alf Cen

Link by name to the catalogue in VizieR :

CCDM J14396-6050AB CD-60 5293 CPD-60 5483 2E 3308 EUVE J1439-60.8
FK5 538 IRAS 14359-6037 2RE J143941-605000 2RE J1439-605 1RXS J143940.4-605020
SAO 252838 uvby98 100128620 WDS J14396-6050AB

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