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相关论文: The Venus Tablet and Refraction

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Light refracted by the planet's atmosphere is usually ignored in analysis of planetary transits. Here we show that refraction can add shoulders to the transit light curve, i.e., an increase in the observed flux, mostly just before and after…

地球与行星天体物理 · 物理学 2010-08-05 Omer Sidis , Re'em Sari

We obtained two astronomical values, the Earth-Venus distance and Venus diameter, by means of a geometrical treatment of photos taken of Venus transit in June of 2012. Here we presented the static and translational modelsthat were…

综合物理 · 物理学 2016-11-21 Alberto C. Bertuola , C. Frajuca , N. S. Magalhães , Victo S. Filho

Conventional explanations for observations of anomalous behaviour of mechanical systems during solar eclipses are critically reviewed. These observations include the work of Allais with paraconical pendula, those of Saxl and Allen with a…

广义相对论与量子宇宙学 · 物理学 2007-05-23 Chris P. Duif

We study the phase curves for the planets of our Solar System; which, is considered as a non-compact planetary system. We focus on modeling the small variations of the light curve, based on the three photometric effects: reflection,…

太阳与恒星天体物理 · 物理学 2018-05-18 H. Barbier , E. D. López , B. Tipán , C. L. Vásconez

Most models used to predict or fit exoplanet transmission spectra do not include all the effects of atmospheric refraction. Namely, the angular size of the star with respect to the planet can limit the lowest altitude, or highest density…

地球与行星天体物理 · 物理学 2017-03-23 Y. Betremieux , L. Kaltenegger

One additional position of the famous Mataveri calendar of Easter Island has been interpreted. New data on the watchings of Venus and Aldebaran have been rendered. Some reports about the sun, the moon as well as Sirius are of our interest,…

物理学史与哲学 · 物理学 2016-04-12 Sergei Rjabchikov

The tidal deformations of a planet are often considered as markers of its inner structure. In this work, we use the tide excitations induced by the Sun on Venus for deciphering the nature of its internal layers. In using a Monte Carlo…

地球与行星天体物理 · 物理学 2023-05-24 Christelle Saliby , Agnes Fienga , Arthur Briaud , Anthony Memin , Carianna Herrera

Firstly identified in images from JAXA's orbiter Akatsuki, the cloud discontinuity of Venus is a planetary-scale phenomenon known to be recurrent since, at least, the 1980s. Interpreted as a new type of Kelvin wave, this disruption is…

Thermal radiation becomes a prominent feature in the continuum spectrum of Venus longwards of $\sim$3 $\mu$m. The emission is traceable to the upper cloud and haze layers in the planet's mesosphere. Venus' thermal radiation spectrum is…

地球与行星天体物理 · 物理学 2024-02-07 A. García Muñoz , P. Wolkenberg , A. Sánchez-Lavega , R. Hueso , I. Garate-Lopez

An unknown absorber near the cloud top level of Venus generates a broad absorption feature from the ultraviolet (UV) to visible, peaking around 360 nm, and therefore plays a critical role in the solar energy absorption. We present a…

We explore the dominant modes of variability in the observed albedo at the cloud tops of Venus using the Akatsuki UVI 283-nm and 365-nm observations, which are sensitive to SO2 and unknown UV absorber distributions respectively, over the…

地球与行星天体物理 · 物理学 2019-06-12 Pushkar Kopparla , Yeon Joo Lee , Takeshi Imamura , Atsushi Yamazaki

Sulfur dioxide is a radiatively and chemically important trace gas in the atmosphere of Venus and its abundance at the cloud-tops has been observed to vary on interannual to decadal timescales. This variability is thought to come from…

地球与行星天体物理 · 物理学 2020-11-02 Pushkar Kopparla , Ashwin Seshadri , Takeshi Imamura , Yeon Joo Lee

Many of the general-relativity-tests such as bending of light near a star and gravitational red/blue shift are explained without general-relativity and without Newtonian-approach. The author first casts doubts on both, the Newtonian and the…

综合物理 · 物理学 2007-05-23 Dr. R. C. Gupta

We quantify the effects of refraction in transit transmission spectroscopy on spectral absorption features and on temporal variations that could be used to obtain altitude-dependent spectra for planets orbiting stars of different stellar…

地球与行星天体物理 · 物理学 2014-08-19 Amit Misra , Victoria Meadows , Dave Crisp

The variation of the solar diameter in time and in position angle has implications in astrophysics and in general relativity, as the long series of studies attest. The Transits of Venus in 2004 and 2012 have been carefully studied because…

太阳与恒星天体物理 · 物理学 2015-07-15 Costantino Sigismondi , Anthony Ayiomamitis , Xiaofan Wang , Wenbin Xie , Massimo Carinci , Alessio Mimmo

To explain Venus' young surface age and lack of plate tectonics, Venus' tectonic regime has often been proposed to be either an episodic-lid regime with global lithospheric overturns, or an equilibrium resurfacing regime with numerous…

地球与行星天体物理 · 物理学 2023-04-19 Jiacheng Tian , Paul J. Tackley , Diogo L. Lourenço

The possible discovery of astronomical effects due to precession - such as the shift in the declination of heliacal raising of bright stars or the precession of the equinoxes - is reviewed for various ancient cultures in the world. Although…

物理学史与哲学 · 物理学 2007-05-23 Giulio Magli

Large sunspots can be observed with the unaided eye under suitable atmospheric seeing conditions. Such observations are of particular value because the frequency of their appearance provides an approximate indication of the prevailing level…

Meteor and bolide phenomena caused by the atmospheric ablation of incoming meteoroids are predicted to occur at the planet Venus. Their systematic observation would allow to measure and compare the sub-mm to m meteoroid flux at different…

地球与行星天体物理 · 物理学 2024-05-31 Apostolos A. Christou , Maria Gritsevich

Microlensings events are predicted for the light coming from cosmological sources. In addition to the microlensing due to gravitation lensing, microlensing produced also by refraction of light due to either ionized, or not, gas clouds can…

天体物理仪器与方法 · 物理学 2016-10-19 G. Cavalleri , F. Barbero , E. Tonni , S. Covino