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Stellar activity influences radial velocity (RV) measurements and can also mimic the presence of orbiting planets. As part of the search for planets around the components of wide binaries performed with the SARG High Resolution Spectrograph…

Solar and Stellar Astrophysics · Physics 2016-12-07 E. Sissa , R. Gratton , S. Desidera , A. F. Martinez Fiorenzano , A. Bonfanti , E. Carolo , D. Vassallo , R. U. Claudi , M. Endl , R. Cosentino

In previous work we identified six Sun-like stars observed by Kepler with exceptionally clear asteroseismic signatures of rotation. Here, we show that five of these stars exhibit surface variability suitable for measuring rotation. In order…

Solar and Stellar Astrophysics · Physics 2015-10-07 M. B. Nielsen , H. Schunker , L. Gizon , W. H. Ball

This review provides an introduction to the generation and evolution of the Sun's magnetic field, summarising both observational evidence and theoretical models. The eleven year solar cycle, which is well known from a variety of observed…

Solar and Stellar Astrophysics · Physics 2011-10-17 Alan W. Hood , David W. Hughes

Earth will become uninhabitable within 2-3 Gyr as a result of the moving boundaries of the habitable zone caused by the increasing luminosity of the Sun. Predictions about the future of habitable conditions on Earth include a decline in…

Earth and Planetary Astrophysics · Physics 2015-06-03 J. T. O'Malley-James , J. S. Greaves , J. A. Raven , C. S. Cockell

The solar cycle periodically reshapes the magnetic structure and radiative output of the Sun and determines its impact on the heliosphere roughly every 11 years. Besides this main periodicity, it shows century-long variations (including…

Solar and Stellar Astrophysics · Physics 2022-03-23 A. Munoz-Jaramillo , J. M. Vaquero

Stellar activity can reveal itself in the form of radiation (eg, enhanced X-ray coronal emission, flares) and particles (eg, winds, coronal mass ejections). Together, these phenomena shape the space weather around (exo)planets. As stars…

Earth and Planetary Astrophysics · Physics 2022-11-29 A. A. Vidotto

Aims. We aim to describe the pre-main sequence and main-sequence evolution of X-ray and extreme-ultaviolet radiation of a solar mass star based on its rotational evolution starting with a realistic range of initial rotation rates. Methods.…

Solar and Stellar Astrophysics · Physics 2015-05-27 Lin Tu , Colin P. Johnstone , Manuel Güdel , Helmut Lammer

The architecture and evolution of planetary systems are shaped in part by stellar flybys. Within this context, we look at stellar encounters which are too weak to immediately destabilize a planetary system but are nevertheless strong enough…

Earth and Planetary Astrophysics · Physics 2022-06-30 Garett Brown , Hanno Rein

Transiting planets around stars are discovered mostly through photometric surveys. Unlike radial velocity surveys, photometric surveys do not tend to target slow rotators, inactive or metal-rich stars. Nevertheless, we suspect that…

Solar and Stellar Astrophysics · Physics 2015-12-16 Andrea Bonfanti , Sergio Ortolani , Valerio Nascimbeni

We present stellar evolution models for 0.5 - 1.2 \Msol at scaled metallicities of 0.1 - 1.5 Z\sol and O/Fe values of 0.44 - 2.28 O/Fe\sol. The time dependent evolution of habitable zone boundaries are calculated for each stellar evolution…

Solar and Stellar Astrophysics · Physics 2016-12-20 Amanda Truitt , Patrick A. Young , Alexander Spacek , Luke Probst , Jeremy Dietrich

Rotation is a prominent feature of the Sun, and it plays a crucial role in the generation and dynamic evolution of solar magnetic fields. The daily composite time series of Ca II K plage areas from 1907 February 1 to 2023 December 31 is…

Solar and Stellar Astrophysics · Physics 2025-12-18 N. B. Xiang , X. H. Zhao , L. H. Deng , F. Y. Li , M. Wan , S. Y. Qi

It is shown that the description of the solar cycle that takes into account the odd zonal harmonic of the solar magnetic field allows us to deepen our knowledge of two important aspects of the solar activity. First, to clarify and expand…

Solar and Stellar Astrophysics · Physics 2023-11-02 V. N. Obridko , D. D. Sokoloff , M. M. Katsova

Stars interact with their planets through gravitation, radiation, and magnetic fields. Although magnetic activity decreases with time, reducing associated high-energy (e.g., coronal XUV emission, flares), stellar winds persist throughout…

Solar and Stellar Astrophysics · Physics 2022-11-08 J. J. Chebly , J. D. Alvarado-Gómez , K. Poppenhaeger

The diversity of planetary systems that have been discovered are revealing the plethora of possible architectures, providing insights into planet formation and evolution. They also increase our understanding of system parameters that may…

The detection of massive planets orbiting nearby stars has become almost routine, but current techniques are as yet unable to detect terrestrial planets with masses comparable to the Earth's. Future space-based observatories to detect…

Astrophysics · Physics 2015-06-24 E. B. Ford , S. Seager , E. L. Turner

Close-in, giant planets are expected to influence their host stars via tidal or magnetic interaction. But are these effects strong enough in suitable targets known so far to be observed with today's instrumentation? The upsilon And system,…

Solar and Stellar Astrophysics · Physics 2015-05-20 K. Poppenhaeger , L. F. Lenz , A. Reiners , J. H. M. M. Schmitt , E. Shkolnik

Exoplanet surveys have confirmed one of humanity's (and all teenagers') worst fears: we are weird. If our Solar System were observed with present-day Earth technology -- to put our system and exoplanets on the same footing -- Jupiter is the…

Earth and Planetary Astrophysics · Physics 2022-02-23 Sean N. Raymond , Andre Izidoro , Alessandro Morbidelli

We use high accuracy photometric data obtained with the Kepler satellite to monitor the activity modulations of the Kepler-210 planet host star over a time span of more than four years. Following the phenomenology of the star's light curve…

Solar and Stellar Astrophysics · Physics 2016-10-07 P. Ioannidis , J. H. M. M. Schmitt

Photosynthetic life requires sufficient photosynthetically active radiation (PAR) to metabolise. On Earth, plant behaviour, physiology and metabolism are sculpted around the night-day cycle by an endogenous biological circadian clock. The…

Earth and Planetary Astrophysics · Physics 2015-06-18 S. P. Brown , A. J. Mead , D. H. Forgan , J. A. Raven , C. S. Cockell

With the availability of considerably more data, we revisit the question of how special our Solar System is, compared to observed exoplanetary systems. To this goal, we employ a mathematical transformation that allows for a meaningful,…

Earth and Planetary Astrophysics · Physics 2015-09-16 Rebecca G. Martin , Mario Livio