Search results

Jump to navigation Jump to search
View (previous 20 | ) (20 | 50 | 100 | 250 | 500)
  • [[File:Positional astronomy.svg|thumb|400px|Diagram of [[positional astronomy]]]] In [[positional astronomy]], two [[astronomical object]]s are said to be in '''opposition''' when they are on [[antipodal point|opposite sides]] of the ...
    7 KB (912 words) - 03:22, 3 April 2024
  • {{Short description|Relationship in astrophysics}} {{For|the Phillips relationship in labour-market economics|Phillips curve}} ...
    6 KB (845 words) - 22:43, 26 October 2024
  • ...will break up into a number of speckles. Each speckle will move around in time to integrate over a long exposure to a diameter approximately D/r0. The siz ...ive_optics_for_astronomical_telescopes| page=92|isbn=0-19-509019-5}}</ref> in terms of the so-called [[Astronomical seeing#The profile|atmospheric turbu ...
    5 KB (724 words) - 23:56, 27 September 2023
  • ...uired between sample points for the values to be effectively uncorrelated. In addition, they can form the basis of rules for interpolating values at poin ...] differ only in the particular stochastic processes they are applied to. In [[quantum field theory]] there are [[Correlation function (quantum field th ...
    6 KB (900 words) - 19:38, 27 April 2024
  • {{Short description|Radio-astronomy observatory in Western Australia}} ...ies in a designated [[radio quiet zone]] located near [[Boolardy Station]] in the [[Murchison Shire]] of [[Western Australia]], about {{convert|800|km}} ...
    15 KB (2,076 words) - 10:59, 18 January 2025
  • ...search on the structure of galaxies and active galactic nuclei, especially in the early universe ...clei]], especially in the early universe. She is an associate professor of astronomy and astrophysics at the [[Scuola Normale Superiore di Pisa]].{{r|sns}} ...
    5 KB (644 words) - 20:40, 28 August 2024
  • | period = 1.69 [[Julian year (astronomy)|yr]] (616.24 [[Julian year (astronomy)|d]]) ...Spacewatch II]] at an [[apparent magnitude]] of 20 using a {{convert|1.8|m|in|adj=on|sp=us}} [[reflecting telescope]].<ref name="MPEC2003-E34"/> It has a ...
    7 KB (949 words) - 20:10, 27 November 2023
  • {{Short description|Julian Date (JD) corrected for differences in the Earth's position with respect to the Sun}} ...ime the event is observed depends on the changing position of the observer in the Solar System. Before multiple observations can be combined, they must b ...
    4 KB (687 words) - 11:52, 17 July 2023
  • {{Short description|Random fluctuations in radio waves of celestial origin}} ...scintillation is the result of radio waves traveling through fluctuations in the density of the [[electron]] and [[proton]]s that make up the [[solar wi ...
    10 KB (1,338 words) - 14:27, 27 November 2023
  • ...book of [[astronomical tables]] written by [[Maria Cunitz]] and published in 1650. As Maria Cunitz was the daughter of both a physician and mathematicia ...tions, leading to inaccuracies within her work. Astronomical tables of the time all contained computational errors, so despite these errors, Urania Propiti ...
    9 KB (1,230 words) - 08:53, 18 February 2025
  • of the initial power spectrum of fluctuations in the [[cold dark matter]] ...tratum", [https://ui.adsabs.harvard.edu/abs/1974A%26A....37..225M/abstract Astronomy and Astrophysics, vol. 37, no. 2, Dec. 1974, p. 225-228]</ref> ...
    4 KB (593 words) - 15:25, 27 June 2023
  • '''Nodal precession''' is the [[precession]] of the [[orbital plane (astronomy)|orbital plane]] of a [[satellite]] around the [[rotation]]al axis of an [[ ...ital plane would remain fixed in space around the gravitational [[primary (astronomy)|primary body]]. However, most bodies rotate, which causes an [[equatorial ...
    6 KB (889 words) - 05:52, 26 July 2024
  • ...he parallactic angle is 0° or 180° when the object crosses the [[meridian (astronomy)|meridian]]. ...'s disk are aligned with the vertical and horizontal direction of the view in the telescope. With an [[altazimuth mount]], those directions are rotated b ...
    11 KB (1,694 words) - 03:22, 16 January 2025
  • ...is an [[Astrophysicists|astrophysicist]] who is Professor of Extragalactic Astronomy at the [[University of Manchester]]. ...ecame Professor of Extragalactic Astronomy at the University of Manchester in 2020.{{citation needed|date= September 2023}} ...
    11 KB (1,416 words) - 15:10, 10 April 2024
  • ...ce to obtain an amplitude like the measured one or higher, if the analysed time series were [[random]]?” ...time series to be averaged to zero before applying the DFT, which is done in many practical applications. When a zero-mean corrected dataset has to be s ...
    12 KB (1,639 words) - 16:46, 3 October 2024
  • ...ved the [[CNRS Silver Medal]] in 1994 and the [[Milutin Milankovic Medal]] in 2019. Since 2003, he is a member of the [[French Academy of Sciences]].<ref ...esis in 1984. He became a CNRS researcher at the [[Bureau des Longitudes]] in 1985. ...
    5 KB (663 words) - 21:58, 29 December 2022
  • ...in the [[Bakhshali manuscript]], a document believed to have been composed in the early centuries of the Common Era.<ref name="Datta1"/> ...a of a different denomination. It is also assumed that ''phala'' increases in proportion to ''pramāṇa''. The unknown quantity is called ''icchā-phala'', ...
    11 KB (1,592 words) - 09:24, 22 December 2024
  • ...first systematic survey of the radio sky was completed by [[Grote Reber]] in April 1943.<ref name="Becker1995" /> ...Society – Palomar Observatory Sky Survey|Palomar Observatory Sky Survey]] in terms of resolution and sensitivity.<ref name="Becker1995" /> ...
    10 KB (1,382 words) - 00:12, 19 August 2023
  • ...om 2010 until his death in late 2015 he was an [[emeritus]] professor of [[astronomy]] at the [[University of California, Berkeley]]. ...ies. In 1964 Spinrad was invited to return to Berkeley as a professor, and in 1968 he received tenure.<ref name="oral_history"/><ref name="berkeley_astro ...
    8 KB (1,156 words) - 21:16, 27 August 2024
  • {{Short description|Variance in a celestial body's axis of rotation over time}} ...en ''[[axial precession|precession]]'', which is a steady long-term change in the axis of rotation, and ''nutation'', which is the combined effect of sim ...
    9 KB (1,390 words) - 13:34, 19 October 2024
View (previous 20 | ) (20 | 50 | 100 | 250 | 500)