SIMBAD references

2011ApJ...735...24J - Astrophys. J., 735, 24 (2011/July-1)

HAT-P-30b: a transiting hot Jupiter on a highly oblique orbit.

JOHNSON J.A., WINN J.N., BAKOS G.A., HARTMAN J.D., MORTON T.D., TORRES G., KOVACS G., LATHAM D.W., NOYES R.W., SATO B., ESQUERDO G.A., FISCHER D.A., MARCY G.W., HOWARD A.W., BUCHHAVE L.A., FURESZ G., QUINN S.N., BEKY B., SASSELOV D.D., STEFANIK R.P., LAZAR J., PAPP I. and SARI P.

Abstract (from CDS):

We report the discovery of HAT-P-30b, a transiting exoplanet orbiting the V = 10.419 dwarf star GSC 0208-00722. The planet has a period P = 2.810595 ±0.000005 days, transit epoch Tc= 2455456.46561±0.00037 (BJD), and transit duration 0.0887±0.0015 days. The host star has a mass of 1.24 ± 0.04 M, radius of 1.21±0.05 R, effective temperature of 6304±88 K, and metallicity [Fe/H] = +0.13±0.08. The planetary companion has a mass of 0.711±0.028 MJ and radius of 1.340±0.065 RJyielding a mean density of 0.37±0.05 g/cm3. We also present radial velocity measurements that were obtained throughout a transit that exhibit the Rossiter-McLaughlin effect. By modeling this effect, we measure an angle of λ = 73°.5 ±9°.0 between the sky projections of the planet's orbit normal and the star's spin axis. HAT-P-30b represents another example of a close-in planet on a highly tilted orbit, and conforms to the previously noted pattern that tilted orbits are more common around stars with Teff{sstarf} ≳ 6250 K.

Abstract Copyright:

Journal keyword(s): planetary systems - stars: individual (HAT-P-30, GSC 0208-00722)

VizieR on-line data: <Available at CDS (J/ApJ/735/24): table1.dat table2.dat>

Simbad objects: 5

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2023.03.21-03:01:32

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