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Gerbert of Aurillac in the Mensura Fistularum explained how to compute the length of organ pipes. The method is shown on two octaves, starting from a fistula of length L=16 units and radius 1 which is equivalent at a monochord of length…

物理学史与哲学 · 物理学 2012-11-05 Costantino Sigismondi

Gerbert of Aurillac was the most prominent personality of the tenth century: astronomer, organ builder and music theoretician, mathematician, philosopher, and finally pope with the name of Silvester II (999-1003). Gerbert introduced firstly…

物理学史与哲学 · 物理学 2015-06-04 Costantino Sigismondi

Gerbert of Aurillac was Pope Sylvester II form 999 to 1003. His history is presented in order to understand his outstanding contribution in the establishment of quadrivium sciences (arithmetics, music, geometry and astronomy) in the…

物理学史与哲学 · 物理学 2012-11-13 Costantino Sigismondi

Globular clusters are relics of the early Universe and they hold clues to many aspects of stellar and galactic evolution. We propose to point the Roman Space Telescope at one or more clusters either as a part of or as an extension of the…

天体物理仪器与方法 · 物理学 2023-06-27 László Molnár , Csilla Kalup , Meridith Joyce

The lensing effect of a cosmic string is studied, and some new methods are proposed to detect the cosmic string. The technique for using jets as extended gravitational lensing probes was firstly explored by Kronberg. We use the…

宇宙学与河外天体物理 · 物理学 2012-07-18 Fa-bo Feng

The Copernican Principle (which says the Earth and sun are not unique) should have observational consequences and thus be testable. Galileo Galilei thought he could measure the true angular diameters of stars with his telescope; according…

物理学史与哲学 · 物理学 2009-02-17 Christopher M. Graney

The objective reality of the Earth's motion about the Sun was finally proven observationally by Bradley (1727) when he correctly explained the ~20'' annual, elliptical motions of stars as being due to aberration of starlight caused by the…

地球与行星天体物理 · 物理学 2018-09-05 Jason T. Wright

Space-based observations of solar-like oscillations present an opportunity to constrain stellar models using individual mode frequencies. However, current stellar models are inaccurate near the surface, which introduces a systematic…

太阳与恒星天体物理 · 物理学 2015-06-22 Warrick H. Ball , L. Gizon

The IceCube Neutrino Observatory will be upgraded with more than 700 additional optical sensor modules and new calibration devices. Improved calibration will enhance IceCube's physics capabilities both at low and high neutrino energies. An…

天体物理仪器与方法 · 物理学 2021-08-23 Jürgen Borowka , Christoph Günther , Dirk Heinen , Simon Zierke

The Clementine gnomon has been built in 1702 to measure the Earth's obliquity variation. For this reason the pinhole was located in the walls of Diocletian's times (305 a. D.) in order to remain stable along the centuries, but its original…

物理学史与哲学 · 物理学 2015-06-04 Costantino Sigismondi

Accelerations of both the solar system barycenter (SSB) and stars in the Milky Way cause a systematic observational effect on the stellar proper motions, which was first studied in the early 1990s and developed by J. Kovalevsky (aberration…

星系天体物理 · 物理学 2015-06-16 Jia-Cheng Liu , Yi Xie , Zi Zhu

Stars near the Sun oscillate both horizontally and vertically. In Paper I the coupling between these motions was modelled by determining the horizontal motion without reference to the vertical motion, and recovering the coupling by assuming…

星系天体物理 · 物理学 2015-05-20 James Binney , Paul McMillan

Christian Ludwig Gerling's 1817 appointment as Professor for Mathematics, Physics and Astronomy resulted in the foundation of the Mathematical and Physical Institute of the Philipps University. In 1838, Gerling moved onto new premises in…

物理学史与哲学 · 物理学 2015-03-16 Andreas Schrimpf

The answers to fundamental science questions in astrophysics, ranging from the history of the expansion of the universe to the sizes of nearby stars, hinge on our ability to make precise measurements of diverse astronomical objects. As our…

It is customary to employ a semi-spherical scale model to describe the apparent path of the Sun across the sky, whether it be its diurnal motion or its variation throughout the year. A flat surface and three bent semi-rigid wires…

科普物理 · 物理学 2018-09-25 Alejandro Gangui , Roberto Casazza , Carlos Paez

We present compelling arguments -- focusing on galaxy science -- for preserving the main imagers and operational modes of the Hubble Space Telescope (HST) for as long as is technically feasible, to assure maximum complementarity to the…

The standard description of cosmological observables is incomplete, because it does not take into account the correct angular parametrization of the sky, i.e. the one determined by the observer frame. The corresponding corrections must be…

宇宙学与河外天体物理 · 物理学 2020-07-02 Ermis Mitsou , Jaiyul Yoo

We present a new careful and comprehensive analysis the observations of the satellites of Jupiter from the Sidereus Nuncius that extends and complements previous similar studies. Each observation is compared to the predictions obtained…

物理学史与哲学 · 物理学 2026-03-20 Andrea Longhin

We describe a new formula capable of quantitatively characterizing the Hubble sequence of spiral galaxies including grand design and barred spirals. Special shapes such as ring galaxies with inward and outward arms are also described by the…

星系天体物理 · 物理学 2015-05-13 Harry I. Ringermacher , Lawrence R. Mead

G. B. Riccioli's 1651 Almagestum Novum contains a table of diameters of stars measured by Riccioli and his associates with a telescope. These telescopically measured star diameters are spurious, caused by the diffraction of light waves…

物理学史与哲学 · 物理学 2010-05-03 Christopher M. Graney
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