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- ...n pattern. The same [[elastic scattering]] processes cause the sky to be [[sky blue|blue]]. The polarization is characterized at each [[wavelength]] by it The polarization pattern of the sky is dependent on the [[celestial coordinate system|celestial]] [[position of ...27 KB (4,325 words) - 18:45, 29 March 2024
- ...g/astronomy-news/how-bright-moon-exactly/ |access-date=2022-08-29 |website=Sky & Telescope |language=en-US}}</ref> as per the formula: <math>-10.79\approx ...a/object.php?id=21253&town=2643743 |access-date=2023-12-08 |website=In-The-Sky.org |language=en}}</ref> ...37 KB (4,647 words) - 03:02, 30 January 2025
- ...survey was started 50 years after the first systematic survey of the radio sky was completed by [[Grote Reber]] in April 1943.<ref name="Becker1995" /> ...al Geographic 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
Page text matches
- ...S. L. Snowden when working with the ROSAT mission to create the ROSAT All-Sky Survey in order to make the surface brightness values fit into a two byte i ...618 bytes (94 words) - 04:29, 27 January 2025
- ...y Angular Correlation Functions and Power Spectrum from the Two Micron All Sky Survey]</ref> The function may be computed as follows: <math>w(\theta)=\fr ...1 KB (152 words) - 16:35, 30 November 2023
- ...survey was started 50 years after the first systematic survey of the radio sky was completed by [[Grote Reber]] in April 1943.<ref name="Becker1995" /> ...al Geographic 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
- ...ding to this method, the magnetic field <math>B</math> in the plane of the sky is given by ...3 KB (446 words) - 07:05, 10 June 2024
- ...with [[ultraviolet]] [[spectrophotometer]] of the ratio of the [[zenith]] sky light intensities of two wavelengths in the solar ultraviolet when the sun ...ue and is given by the logarithm base 10 of the ratio of cloudless zenith sky intensities at two different wavelengths scaled by a multiplicative factor ...4 KB (631 words) - 21:15, 20 August 2024
- ...librate the detector, so for general purposes, any star may be used in the sky that has a known apparent magnitude.<ref name=":1">{{Cite web|url=http://ww ...4 KB (629 words) - 20:51, 5 July 2024
- ..."st0811">Alycia J. Weinberger, "Building Planets in Disks of Chaos" in ''[[Sky & Telescope]]'', November 2008, p. 37.</ref> This dust absorbs light from t ...2 KB (220 words) - 05:19, 30 September 2023
- ...accurately reproduces a [[de Vaucouleurs profile]] when projected onto the sky. ...2 KB (268 words) - 15:31, 31 October 2024
- ...me 2, double stars, variable stars and nonstellar objects'', p. xvii. Sky Publishing Corporation ({{ISBN|0-933346-38-7}}) and Cambridge University Pr ...4 KB (687 words) - 11:52, 17 July 2023
- ...e is not changed when telescopes zoom in or out because the same amount of sky will be in the pixel whether it is enlarged or shrunk. ...2 KB (283 words) - 22:21, 10 December 2024
- ...n pattern. The same [[elastic scattering]] processes cause the sky to be [[sky blue|blue]]. The polarization is characterized at each [[wavelength]] by it The polarization pattern of the sky is dependent on the [[celestial coordinate system|celestial]] [[position of ...27 KB (4,325 words) - 18:45, 29 March 2024
- ...|url=https://skyandtelescope.org/astronomy-news/comet-swan-song/ |website=Sky & Telescope |access-date=22 January 2023 |date=22 May 2020}}</ref> It passe :[[File:C2020_F8-skypath.png|left|thumb|250x250px|Sky trajectory with 7 week markers]] ...8 KB (1,088 words) - 17:21, 25 January 2025
- {{Sky|12|19|51.56|+|31|28|49.71}} ...orer|WISE]] J121951.32+312849.5, UGCS J121951.36+312849.4, [[Sloan Digital Sky Survey|SDSS]] J121951.45+312849.4, [[TESS Input Catalog|TIC]] 139087399{{r| ...11 KB (1,269 words) - 10:50, 1 July 2024
- {{Sky|04|07|07.53|+|15|24|45.54}} | names = [[Sloan Digital Sky Survey|SDSS]] J040707.56+154645.2, [[Ecliptic Plane Input Catalog|EPIC 2105 ...9 KB (1,076 words) - 12:24, 5 January 2024
- ...ear=2013|title=On CCC-predicted concentric low-variance circles in the CMB sky|journal=Eur. Phys. J. Plus|volume=128|issue=2|pages= 22|arxiv=1302.5162|bib ...om The Pre-Big Bang Universe? A Search for Low Variance Circles in the CMB Sky|date=2010-12-08|doi=10.1088/0004-637X/740/2/52|volume=740|issue=2|journal=T ...13 KB (1,893 words) - 20:02, 30 January 2025
- ...y is red and threatening." You know how to interpret the appearance of the sky, but you cannot interpret the signs of the times. ...ens. You hypocrites! You know how to interpret the appearance of earth and sky; but why do you not know how to interpret the present time? (RSV) ...13 KB (1,689 words) - 14:33, 17 July 2024
- ...reated from the [[Sloan Digital Sky Survey]] and the [[UKIRT Infrared Deep Sky Survey]]. The quasar appears as a faint red dot close to the centre. ...e constellation of [[Leo (constellation)|Leo]], close (on the plane of the sky) to [[σ Leo]]. The quasar was discovered by a telescope that operates at [[ ...12 KB (1,748 words) - 07:13, 1 July 2024
- ...nts are taken at two different times of day: once with the sun high in the sky, and once with it near the horizon. In both cases the light is scattered in ...ißenmayer |author4= J. P. Burrows |name-list-style=amp | title=DOAS zenith sky observations. 2. Seasonal variation of BrO over Bremen (53°N) 1994–1995|jou ...8 KB (1,317 words) - 01:10, 3 December 2024
- {{Sky|01|49|10.829|-|10|25|35.13}} File:NGC681 - SDSS DR14.jpg|[[Sloan Digital Sky Survey|SDSS]] image of NGC 681 ...6 KB (804 words) - 00:59, 27 November 2024
- WASP was first introduced to the public by [[Sky Sport (New Zealand)|Sky Sport New Zealand]] in November 2012 during [[Auckland cricket team|Aucklan ...7 KB (1,039 words) - 12:18, 16 February 2024