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The Transit Timing Variation (TTV) method relies on monitoring changes in timing of transits of known exoplanets. Non-transiting planets in the system can be inferred from TTVs by their gravitational interaction with the transiting planet.…

地球与行星天体物理 · 物理学 2015-05-14 David Nesvorny , Cristian Beauge

Transit timing variations (TTVs) are a powerful tool for characterizing the properties of transiting exoplanets. However, inferring planet properties from the observed timing variations is a challenging task, which is usually addressed by…

地球与行星天体物理 · 物理学 2018-06-26 Itai Linial , Shmuel Gilbaum , Re'em Sari

We present new ways to identify single and multiple moons around extrasolar planets using planetary transit timing variations (TTVs) and transit duration variations (TDVs). For planets with one moon, measurements from successive transits…

地球与行星天体物理 · 物理学 2016-12-06 René Heller , Michael Hippke , Ben Placek , Daniel Angerhausen , Eric Agol

The Transit Timing Variations (TTVs) technique provides a powerful tool to detect additional planets in transiting exoplanetary systems. In this paper we show how transiting planets with significant TTVs can be systematically missed, or…

地球与行星天体物理 · 物理学 2015-05-28 Enrique Garcia-Melendo , Mercedes Lopez-Morales

Transiting exoplanets in multi-planet systems have non-Keplerian orbits which can cause the times and durations of transits to vary. The theory and observations of transit timing variations (TTV) and transit duration variations (TDV) are…

地球与行星天体物理 · 物理学 2025-05-01 Eric Agol , Daniel Fabrycky

The transit timing variation (TTV) method allows the detection of non-transiting planets through their gravitational perturbations. Since TTVs are strongly enhanced in systems close to mean-motion resonances (MMR), even a low mass planet…

地球与行星天体物理 · 物理学 2015-06-03 Gwenaël Boué , Mahmoudreza Oshagh , Marco Montalto , Nuno C. Santos

Transit timing variations (TTVs) are a valuable tool to determine the masses and orbits of transiting planets in multi-planet systems. TTVs can be readily modeled given knowledge of the interacting planets' orbital configurations and…

天体物理仪器与方法 · 物理学 2019-01-30 Noah W. Tuchow , Eric B. Ford , Theodore Papamarkou , Alexey Lindo

Both ground and space-based transit observatories are poised to significantly increase the number of known transiting planets and the number of precisely measured transit times. The variation in a planet's transit times may be used to infer…

地球与行星天体物理 · 物理学 2015-05-20 Dimitri Veras , Eric B. Ford , Matthew J. Payne

As the number of known exoplanets continues to grow, the question as to whether such bodies harbour satellite systems has become one of increasing interest. In this paper, we explore the transit timing effects that should be detectable due…

天体物理学 · 物理学 2009-11-13 David M. Kipping

Here we describe a story behind the discovery of Kepler-46, which was the first exoplanetary system detected and characterized from a method known as the transit timing variations (TTVs). The TTV method relies on the gravitational…

地球与行星天体物理 · 物理学 2019-07-17 David Nesvorny

We develop and apply methods to extract planet masses and eccentricities from observed transit time variations (TTVs). First, we derive simple analytic expressions for the TTV that include the effects of both first- and second-order…

地球与行星天体物理 · 物理学 2016-09-07 Sam Hadden , Yoram Lithwick

Transit timing variations (TTV) are considered a tool for constraining the masses of transiting planets in the absence of radial-velocity data. Although theoretical studies have long revealed that TTV mass determinations intrinsically…

地球与行星天体物理 · 物理学 2026-04-13 Sheng Jin , Dong-Hong Wu , Xiao-Ling Xu , Jianghui Ji

In a transiting planetary system, the presence of a second planet will cause the time interval between transits to vary. These transit timing variations (TTV) are particularly large near mean-motion resonances and can be used to infer the…

天体物理学 · 物理学 2007-05-23 Jason H. Steffen , Eric Agol

Transit timing variation (TTV) is a useful tool for studying the orbital properties of transiting objects. However, few TTV studies have been done on transiting brown dwarfs (BDs) around solar-type stars. Here we study the long-term TTV of…

地球与行星天体物理 · 物理学 2025-05-28 Wenqin Wang , Xinyue Ma , Zhangliang Chen , Cong Yu , Shangfei Liu , Bo Ma

Characterization of transiting planets with transit timing variations (TTVs) requires understanding how to translate the observed TTVs into masses and orbital elements of the planets. This can be challenging in multi-planet transiting…

地球与行星天体物理 · 物理学 2016-04-28 Eric Agol , Katherine Deck

The Transit Timing Variations (TTVs) are deviations of the measured mid-transit times from the exact periodicity. One of the most interesting causes of TTVs is the gravitational interaction between planets. Here we consider a case of two…

地球与行星天体物理 · 物理学 2016-06-01 D. Nesvorny , D. Vokrouhlicky

Modern theoretical estimates show that with the help of real equipment we are able to detect large satellites of exoplanets (about the size of the Ganymede), although, numerical attempts of direct exomoon detection were unsuccessful. Lots…

天体物理仪器与方法 · 物理学 2017-04-04 K. E. Naydenkin , D. S. Kaparulin

Transit timing variations (TTVs) can provide useful information for systems observed by transit, as they allow us to put constraints on the masses and eccentricities of the observed planets, or even to constrain the existence of…

地球与行星天体物理 · 物理学 2021-11-15 A. Leleu , G. Chatel , S. Udry , Y. Alibert , J. -B. Delisle , R. Mardling

Transit timing variations (TTVs) have proven to be a powerful technique for confirming Kepler planet candidates, for detecting non-transiting planets, and for constraining the masses and orbital elements of multi-planet systems. These TTV…

地球与行星天体物理 · 物理学 2014-05-20 Katherine M. Deck , Eric Agol , Matthew J. Holman , David Nesvorny

Transit timing variations (TTVs) of exoplanets are normally interpreted as the consequence of gravitational interaction with additional bodies in the system. However, TTVs can also be caused by deformations of the system transits by…

地球与行星天体物理 · 物理学 2015-12-23 P. Ioannidis , K. F. Huber , J. H. M. M. Schmitt
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