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The stellar obliquity of a transiting planetary system can be constrained by combining measurements of the star's rotation period, radius, and projected rotational velocity. Here we present a hierarchical Bayesian technique for recovering…

地球与行星天体物理 · 物理学 2015-06-22 Timothy D. Morton , Joshua N. Winn

The purpose of the paper is five-fold: (a) Argue that the question in the title can be presented in a meaningful manner and that it requires an answer. (b) Discuss the conventional answers and explain why they are unsatisfactory. (c)…

广义相对论与量子宇宙学 · 物理学 2015-05-18 T. Padmanabhan

According to the Krizek-Somer hypothesis [New Astron. 17, 1 (2012); Grav. Cosmol. 21, 59 (2015)], a biological evolution of the Earth is possible only at certain values of the Hubble parameter, because the increasing luminosity of the Sun…

综合物理 · 物理学 2025-04-28 Yurii V. Dumin , Eugen S. Savinykh

We investigate the variability properties of main sequence stars in the first month of Kepler data, using a new astrophysically robust systematics correction, and find that 60% of stars are more variable then the active Sun. We define low…

太阳与恒星天体物理 · 物理学 2013-10-24 Amy McQuillan , Suzanne Aigrain , Stephen Roberts

Royal Society Discussion Meeting (2013) `Characterizing exoplanets'. Of the 900+ confirmed exoplanets discovered since 1995 for which we have constraints on their mass (i.e., not including Kepler candidates), 75% have masses larger than…

地球与行星天体物理 · 物理学 2014-03-19 Leigh N. Fletcher , Patrick G. J. Irwin , Joanna K. Barstow , Remco J. de Kok , Jae-Min Lee , Suzanne Aigrain

The Kepler mission has been providing high-quality photometric data leading to many breakthroughs in the exoplanet search and in stellar physics. Stellar magnetic activity results from the interaction between rotation, convection, and…

太阳与恒星天体物理 · 物理学 2014-04-14 S. Mathur , D. Salabert , R. A. Garcia , T. Ceillier

The high-mass (M$>$2 \Msolar{}) Kepler red giant stars are less well-studied than their lower-mass counterparts. In the previous article, we presented a sample of 48 high-mass Kepler red giants and measured their asteroseismic parameters.…

The spectacular data delivered by NASA's {\it Kepler} mission have not only boosted the discovery of planets orbiting other stars, but they have opened a window on the inner workings of the stars themselves. For the study of the RR Lyrae…

太阳与恒星天体物理 · 物理学 2013-10-03 Katrien Kolenberg

We present high precision photometry of Kepler-41, a giant planet in a 1.86 day orbit around a G6V star that was recently confirmed through radial velocity measurements. We have developed a new method to confirm giant planets solely from…

No doubt, among the most exciting discoveries of the third millennium thus far are {\bf Oscillations of Massive Neutrinos} and {\bf Dark Energy} that leads to an accelerated expansion of the Universe. Accordingly, Nuclear Physics is…

天体物理学 · 物理学 2009-11-10 Moshe Gai

One bottleneck for the exploitation of data from the $Kepler$ mission for stellar astrophysics and exoplanet research has been the lack of precise radii and evolutionary states for most of the observed stars. We report revised radii of…

地球与行星天体物理 · 物理学 2018-10-24 Travis A. Berger , Daniel Huber , Eric Gaidos , Jennifer L. van Saders

The Kepler space telescope observed over 15,000 stars for asteroseismic studies. Of these, 75% of dwarfs (and 8% of giants) were found to show anomalous behavior: such as suppressed oscillations (low amplitude) or no oscillations at all.…

We reconsider calibration of statistical distance scales for planetary nebulae, examining precision and systematic error for various distance methods used as well as the scales themselves. A different calibration strategy, one based on…

太阳与恒星天体物理 · 物理学 2015-06-22 Haywood Smith

Three pre-telescopic star catalogues contain about a thousand star magnitudes each (with magnitudes 1, 2, 3, 4, 5, and 6), with these reported brightnesses as the original basis for what has become the modern magnitude scale. These…

天体物理仪器与方法 · 物理学 2013-03-11 Bradley E. Schaefer

The present day chemical and dynamical properties of the Milky Way bear the imprint of the Galaxy's formation and evolutionary history. One of the most enduring and critical debates surrounding Galactic evolution is that regarding the…

天体物理学 · 物理学 2009-11-07 Chris B. Brook , Daisuke Kawata , Brad K. Gibson , Chris Flynn

The study of stellar activity is important because it can provide new constraints for dynamo models, when combined with surface rotation rates and the depth of the convection zone. We know that the dynamo mechanism, which is believed to be…

太阳与恒星天体物理 · 物理学 2015-06-18 S. Mathur , R. A. Garcia , J. Ballot , T. Ceillier , D. Salabert , T. S. Metcalfe , C. Regulo , A. Jimenez , S. Bloemen

In a pioneering exposition of mathematical astronomy for the public, Sir John Herschel attributed the stability of the ring of Saturn to its being eccentric with respect to the planet and lopsided (asymmetric in mass) by a minute amount.…

物理学史与哲学 · 物理学 2011-12-09 Alan B. Whiting

In this article, we review the main results of Volume I of Newton's Principia which relates Kepler's law of planets and universal gravitation. In order to clarify the reasoning of Newton, elementary and simple proofs are given to inspire…

物理学史与哲学 · 物理学 2008-01-03 Hai-Chau Chang , Wu-Yi Hsiang

We constrain the densities of Earth- to Neptune-size planets around very cool (Te =3660-4660K) Kepler stars by comparing 1202 Keck/HIRES radial velocity measurements of 150 nearby stars to a model based on Kepler candidate planet radii and…

地球与行星天体物理 · 物理学 2015-05-30 Eric Gaidos , Debra A. Fischer , Andrew W. Mann , Sebastien Lepine