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The classical method for measure the Earth-Sun distance is due to Aristarchus and it is based upon the measure of the angle Moon-Earth-Sun when the Moon is exactly in quadrature. Such an angle is only 9 arcminutes smaller than 90 degrees,…

天体物理仪器与方法 · 物理学 2011-07-06 Costantino Sigismondi

It is straightforward to determine the size of the Earth and the distance to the Moon without making use of a telescope. The methods have been known since the 3rd century BC. However, few amateur or professional astronomers have worked this…

天体物理仪器与方法 · 物理学 2015-05-30 Kevin Krisciunas , Erika DeBenedictis , Jeremy Steeger , Agnes Bischoff-Kim , Gil Tabak , Kanika Pasricha

In July 5th 2014 an occultation of Mars by the Moon was visible in South America. Citizen scientists and professional astronomers in Colombia, Venezuela and Chile performed a set of simple observations of the phenomenon aimed to measure the…

We propose an algorithm that can be used by amateur astronomers to analyze the images acquired during solar eclipses. The proposed algorithm analyzes the image, detects the eclipse and produces results for parameters like magnitude of…

地球与行星天体物理 · 物理学 2012-06-08 Sarrvesh Seethapuram Sridhar , S. Pradeep Sundar , I. Kenny Jackson , P. Kannan

By applying Monte-Carlo method, the Moon radius is obtained by counting craters in a spherical square over the surface of it. As it is well known, approximate values for $\pi $ can be obtained by counting random numbers in a square and in a…

科普物理 · 物理学 2019-08-01 Juan Sebastián Ardenghi

We report on a determination of the Earth-Moon distance performed by students of an Italian high school, based on measurements of the time delay of the "echo" in the radio communications between Nasa mission control in Houston and the…

物理教育 · 物理学 2009-08-13 Luca Girlanda

We present the results of measuring the geocentric lunar distance using what we propose is the simplest method to achieve a precise result. Although lunar distance has been systematically measured to a precision of few millimeters using…

科普物理 · 物理学 2014-05-20 Jorge I. Zuluaga , Juan C. Figueroa , Ignacio Ferrin

The Earth-Moon system is unusual in several respects. The Moon is roughly 1/4 the radius of the Earth - a larger satellite-to-planet size ratio than all known satellites other than Pluto's Charon. The Moon has a tiny core, perhaps with only…

It will be shown that the rotation of the Earth in the Earth-Moon system can be detected by comparing the deflection of a Foucault pendulum at noon on the one hand and at midnight on the other hand. More precisely, on 21 June the midnight…

经典物理 · 物理学 2011-12-23 Bertrand M. Roehner

The global transition towards cleaner and more sustainable energy production is a major challenge. We present an innovative solution by utilizing smartphone light sensors to measure direct normal solar irradiance, the primary component of…

The detection of the New Moon at sunset is of importance to communities based on the lunar calendar. This is traditionally undertaken with visual observations. We propose a radio method which allows a higher visibility of the Moon relative…

天体物理仪器与方法 · 物理学 2014-03-05 Y. A. Hafez , L. Trojan , F. H. Albaqami , A. Z. Almutairi , R. D. Davies , C. Dickinson , L. Piccirillo

It has been posited that lunar eclipse observations may help predict the in-transit signature of Earth-like extrasolar planets. However, a comparative analysis of the two phenomena addressing in detail the transport of stellar light through…

太阳与恒星天体物理 · 物理学 2015-06-05 A. García Muñoz , M. R. Zapatero Osorio , R. Barrena , P. Montañés-Rodríguez , E. L. Martín , E. Pallé

Model simulations of solar irradiance reaching the Earth's surface during a solar eclipse constitute a useful tool for studying the impact of this phenomenon on the radiance propagation through the atmosphere. A simple approach to extend…

大气与海洋物理 · 物理学 2011-10-11 Boyan Petkov , Claudio Tomasi , Vito Vitale , Christian Lanconelli , Mauro Mazzola

I derived an equation to describe the dependence of Moon orbit radius around the Earth. I obtained the radius changes with time according to a scaling equation, Moon orbit radius is proportional to power 2/5 of the Moon age. Using the…

科普物理 · 物理学 2018-02-09 Mikrajuddin Abdullah

Observations of the Earthshine off the Moon allow for the unique opportunity to measure the large-scale Earth atmosphere. Another opportunity is realized during a total lunar eclipse which, if seen from the Moon, is like a transit of the…

地球与行星天体物理 · 物理学 2020-04-01 K. G. Strassmeier , I. Ilyin , E. Keles , M. Mallonn , A. Järvinen , M. Weber , F. Mackebrandt , J. M. Hill

Earthshine is the dominant source of natural illumination on the surface of the Moon during lunar night, and at locations within permanently shadowed regions that never receive direct sunlight. As such, earthshine may enable the exploration…

地球与行星天体物理 · 物理学 2019-04-02 David A. Glenar , Timothy J. Stubbs , Edward W. Schwieterman , Tyler D. Robinson , Timothy A. Livengood

Following a technique of Galileo we compute the height on a mountain on the Moon. It is based on a simple observation that precisely on a half Moon day, the Earth, the Moon, and the Sun form the vertices of a right triangle with the Moon at…

科普物理 · 物理学 2019-05-21 Sunil K. Chebolu

During lunar eclipse of January 21, 2019 a meteoroid impacted the Moon producing a visible light flash. The impact was witnessed by casual observers offering an opportunity to study the phenomenon from multiple geographical locations. We…

Observations of the Earth as a planet using the earthshine technique (i.e. looking at the light reflected from the darkside of the Moon), have been used for climate and astrobiology studies. They provide information about the planetary…

The Earth's albedo is a fundamental climate parameter for understanding the radiation budget of the atmosphere. It has been traditionally measured from space platforms, but also from the ground for sixteen years from Big Bear Solar…

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