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ecliptic

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ecliptic
ecliptic, a. and n. (ɪˈklɪptɪk) Forms: 4–8 ecliptick(e, -tik(e, -que, (4, 7 ecc-, eclyptic(k, 7 æcliptique, 8 eccliptic), 7– ecliptic. [ad. (directly or through F. écliptique) L. eclīptic-us, Gr. ἐκλειπτικός in same sense.] A. adj. Of or pertaining to an eclipse. ecliptic limits: the limits within w... Oxford English Dictionary
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Coma Ecliptic
Thom Jurek of Allmusic gave the album a positive review saying, "Coma Ecliptic holds together as an album. Some opinions were generally mixed on the band's shift away from technical death metal on Coma Ecliptic. wikipedia.org
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Golden Gate of the Ecliptic
The Golden Gate of the Ecliptic is an asterism in the constellation Taurus that has been known for several thousand years. regularly passing through the Golden Gate of the Ecliptic. wikipedia.org
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astroarchive.noirlab.edu
SIMPLE = T / Fits standard BITPIX = 16 / Bits per pixel NAXIS = 2 / Number of axes NAXIS1 = 1024 / Axis length NAXIS2 = 2048 / Axis length EXTEND = F / File may contain extensions BSCALE = 1.000000E0 / REAL = TAPE*BSCALE + BZERO BZERO = 3.276800E4 / ORIGIN = 'NOAO-IRAF FITS Image Kernel December 2001' / FITS file originator DATE = '2003-04-10T22:44:10' IRAF-TLM= '15:44:10 (10/04/2003)' OBJECT ...
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why was the deep ecliptic survey used?
Since 1998 through the end of 2003, the survey covered 550 square degrees with sensitivity of 22.5. An estimated 50% of objects of this magnitude have been found. The survey has also established the mean Kuiper Belt plane.
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Ecliptic coordinate system
A position in the ecliptic coordinate system is thus typically specified true equinox and ecliptic of date, mean equinox and ecliptic of J2000.0, or similar However, for stars near the ecliptic poles, the rate of change of ecliptic longitude is dominated by the slight movement of the ecliptic (that is, of the wikipedia.org
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Why would a source file have the execute bit set? In the standard library for ecliptic curve cryptography one of the C source files has the executable bit set, qv: ![enter image description here]( As you can see the...
There is no reason for a C source file to be executable. This may sometimes happen if the file has been transferred from or through a non-Unix operating system. You may safely remove the execute bit if you wish: $ chmod a-x secp256k1.c
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Deep Ecliptic Survey
The Deep Ecliptic Survey (DES) is a project to find Kuiper belt objects (KBOs), using the facilities of the National Optical Astronomy Observatory (NOAO wikipedia.org
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An integral for the Earth's insolation Consider the function $$ [-\pi/2,\pi/2] \ni \theta \mapsto s_\beta(\theta) = \int_0^{2\pi} \sqrt{ 1 - \left(\cos \theta \sin \beta \cos \gamma \- \sin \theta \cos \beta \right)^2...
The integrand is invariant under $\theta \to -\theta$ and $\gamma \to \gamma + \pi$.
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What is a Hybrid Angle? I'm looking at the Wikipedia content surrounding the calculating the position of the sun relative to the earth, and I came across the term "hybrid angle." (Emphasis added.) > Mean longitude is...
I edited the article to remove "hybrid angle", which seems overly vague. It now reads > While nominally a simple longitude, in practice the mean longitude does not correspond to any one physical angle. Later on there is a comment: > Mean longitude, like mean anomaly, does not measure an angle betwee...
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astroarchive.noirlab.edu
SIMPLE = T / Fits standard BITPIX = 16 / Bits per pixel NAXIS = 2 / Number of axes NAXIS1 = 1023 / Axis length NAXIS2 = 2048 / Axis length EXTEND = F / File may contain extensions BSCALE = 1.000000E0 / REAL = TAPE*BSCALE + BZERO BZERO = 3.276800E4 / ORIGIN = 'NOAO-IRAF FITS Image Kernel December 2001' / FITS file originator DATE = '2003-04-10T22:03:36' IRAF-TLM= '15:03:36 (10/04/2003)' OBJECT ...
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astroarchive.noirlab.edu
SIMPLE = T / Fits standard BITPIX = 16 / Bits per pixel NAXIS = 2 / Number of axes NAXIS1 = 1024 / Axis length NAXIS2 = 2048 / Axis length EXTEND = F / File may contain extensions BSCALE = 1.000000E0 / REAL = TAPE*BSCALE + BZERO BZERO = 3.276800E4 / ORIGIN = 'NOAO-IRAF FITS Image Kernel December 2001' / FITS file originator DATE = '2003-07-17T20:34:18' IRAF-TLM= '13:34:18 (17/07/2003)' OBJECT ...
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astroarchive.noirlab.edu
SIMPLE = T / Fits standard BITPIX = 16 / Bits per pixel NAXIS = 2 / Number of axes NAXIS1 = 1024 / Axis length NAXIS2 = 2048 / Axis length EXTEND = F / File may contain extensions BSCALE = 1.000000E0 / REAL = TAPE*BSCALE + BZERO BZERO = 3.276800E4 / ORIGIN = 'NOAO-IRAF FITS Image Kernel December 2001' / FITS file originator DATE = '2003-07-17T20:28:09' IRAF-TLM= '13:28:09 (17/07/2003)' OBJECT ...
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astroarchive.noirlab.edu
SIMPLE = T / Fits standard BITPIX = 16 / Bits per pixel NAXIS = 2 / Number of axes NAXIS1 = 1024 / Axis length NAXIS2 = 2048 / Axis length EXTEND = F / File may contain extensions BSCALE = 1.000000E0 / REAL = TAPE*BSCALE + BZERO BZERO = 3.276800E4 / ORIGIN = 'NOAO-IRAF FITS Image Kernel December 2001' / FITS file originator DATE = '2004-04-07T18:14:18' IRAF-TLM= '11:14:18 (07/04/2004)' OBJECT ...
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astroarchive.noirlab.edu
SIMPLE = T / Fits standard BITPIX = 16 / Bits per pixel NAXIS = 2 / Number of axes NAXIS1 = 1024 / Axis length NAXIS2 = 2048 / Axis length EXTEND = F / File may contain extensions BSCALE = 1.000000E0 / REAL = TAPE*BSCALE + BZERO BZERO = 3.276800E4 / ORIGIN = 'NOAO-IRAF FITS Image Kernel December 2001' / FITS file originator DATE = '2004-04-07T18:24:36' IRAF-TLM= '11:24:36 (07/04/2004)' OBJECT ...
astroarchive.noirlab.edu 0.0 0.0 0.0