Home     Sopravvivere Nell'Universo    
Services
    Perché adottare     Donatori     Astro Foto     La collezione     Forum     Blog New!     FAQ     Login  

TYC 5839-876-1


Contenuti

Immagini

Carica la tua immagine

DSS Images   Other Images


Articoli relazionati

Evidence of Possible Spin-orbit Misalignment Along the Line of Sight in Transiting Exoplanet Systems
Of the 26 transiting exoplanet systems with measurements of theRossiter-McLaughlin (RM) effect, eight have now been found to besignificantly spin-orbit misaligned in the plane of the sky (i.e., RMmisalignment angle |?| >~ 30° and inconsistent with? = 0°). Unfortunately, the RM effect does not constrain thecomplement misalignment angle between the orbit of the planet and thespin of its host star along the line of sight (LOS). I use a simplemodel of stellar rotation benchmarked with observational data tostatistically identify 10 exoplanet systems from a sample of 75 forwhich there is likely a significant degree of spin-orbit misalignmentalong the LOS: HAT-P-7, HAT-P-14, HAT-P-16, HD 17156, Kepler-5,Kepler-7, TrES-4, WASP-1, WASP-12, and WASP-14. All 10 systems have hoststellar masses M * in the range 1.2 M sun <~ M* <~ 1.5 M sun, and the probability of thisoccurrence by chance is less than one in ten thousand. In addition, theplanets in the candidate-misaligned systems are preferentially massiveand eccentric. The coupled distribution of misalignment from the RMeffect and from this analysis suggests that transiting exoplanets aremore likely to be spin-orbit aligned than expected given predictions fora transiting planet population produced entirely by planet-planetscattering or Kozai cycles and tidal friction. For that reason, thereare likely two populations of close-in exoplanet systems: a populationof aligned systems and a population of apparently misaligned systems inwhich the processes that lead to misalignment or to the survival ofmisaligned systems operate more efficiently in systems with massivestars and planets.

Sottometti un nuovo articolo


Link relazionati

  • - Nessun link trovato -
Sottometti un nuovo link


Membro dei seguenti gruppi:


Osservazione e dati astrometrici

Costellazione:Balena
Ascensione retta:00h18m24.70s
Declinazione:-15°16'02.3"
Magnitudine apparente:11.305
Moto proprio RA:25.3
Moto proprio Dec:-27.7
B-T magnitude:11.687
V-T magnitude:11.337

Cataloghi e designazioni:
Nomi esatti
TYCHO-2 2000TYC 5839-876-1
USNO-A2.0USNO-A2 0675-00119953

→ Richiesta di ulteriori cataloghi da VizieR