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I found that lunar eclipse data is available for many centuries. I downloaded the data for the years 1701..2200. Wrote norm.py to extract and convert the parts I care about into a format that will be much easier to parse in the unit tests for all four languages. Regenerate the normalized data from the 'run' script. This way, I have documentation for where the data came from.
736 lines
49 KiB
HTML
736 lines
49 KiB
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<a class="t" href="/web/20080219040049*/http://sunearth.gsfc.nasa.gov/eclipse/LEcat/LE1801-1900.html" title="See a list of every capture for this URL">71 captures</a>
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<div class="r" title="Timespan for captures of this URL">02 Feb 1999 - 16 May 2013</div>
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Starting in 1996, <a href="http://www.alexa.com/">Alexa Internet</a> has been donating their crawl data to the Internet Archive. Flowing in every day, these data are added to the <a href="http://web.archive.org/">Wayback Machine</a> after an embargo period.
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<div style="display:inline-block;vertical-align:top;width:49%;">
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<span class="c-logo" style="background-image:url(https://archive.org/services/img/51_crawl)"></span>
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<div>Collection: <a style="color:#33f;" href="https://archive.org/details/51_crawl" target="_new"><span class="wm-title">51_crawl</span></a></div>
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this data is currently not publicly accessible.
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<center><table border="5" cellspacing="5">
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<tr><th>
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<img src="/web/20080219040049im_/http://sunearth.gsfc.nasa.gov/eclipse/image/bannerEclipse.gif" width="504" height="115" hspace="3" vspace="3" alt="Eclipse Banner">
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</th></table></center>
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<p>
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<center><img src="/web/20080219040049im_/http://sunearth.gsfc.nasa.gov/eclipse/image/bluePixel.gif" width="450" height="4" alt="Blue Bar"></center>
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<center>
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<h1>Lunar Eclipses: 1801 to 1900</h1>
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<h2>( 1801 CE to 1900 CE )</h2>
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<h4>Fred Espenak</h4>
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</center>
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<center><img src="/web/20080219040049im_/http://sunearth.gsfc.nasa.gov/eclipse/image/bluePixel.gif" width="450" height="4" alt="Blue Bar"></center>
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<p>
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<font size="6">D</font>uring the 19th century CE<font size="1"><sup>1</sup></font>, Earth experienced 252 lunar eclipses as follows:
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<pre> All Eclipses = 252 = 100.0%
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Penumbral (N) = 92 = 36.5%
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Partial (P) = 97 = 38.5%
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Total (T) = 63 = 25.0%
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</pre>
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<font size="6">E</font>clipses in which some portion of the Moon passes into Earth
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's umbral shadow are classified as umbral eclipses .
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All total and partial lunar eclipses are umbral eclipses.
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Statistics for umbral eclipses during the century are as follows:
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<pre>
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Umbral (P&T;) = 160 = 63.5%
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Central<font size="1"><sup>2</sup></font> (T±) = 51 = 20.2%
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Non-Central (T) = 12 = 4.8%
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</pre>
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<center><img src="/web/20080219040049im_/http://sunearth.gsfc.nasa.gov/eclipse/image/bluePixel.gif" width="150" height="1" alt="Blue Bar"></center>
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<pre>
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</pre>
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<font size="6">T</font>here are two to five lunar eclipses in each calendar year.
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The distribution of eclipses each year during this century are as follows:
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<pre>
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Number of Years with 2 Eclipses: 67
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Number of Years with 3 Eclipses: 15
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Number of Years with 4 Eclipses: 17
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Number of Years with 5 Eclipses: 1 ( 1879)
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</pre>
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<pre>
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Two eclipses in same month: 1817 May 01 & 1817 May 30
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</pre>
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<font size="6">D</font>uring any given century,
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old <a href="/web/20080219040049/http://sunearth.gsfc.nasa.gov/eclipse/SEsaros/SEsaros.html">Saros series</a> end while new ones begin.
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The year and Saros number of these events are as follows:
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<pre>
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3 Saros Series' begin (Year/Saros): 1832/145 1843/146 1872/147
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6 Saros Series' end (Year/Saros): 1835/ 99 1839/101 1864/100 1882/105 1886/107 1893/106
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</pre>
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<p><font size="6">T</font>he longest and shortest lunar eclipses of the century and other eclipse extrema are listed below.
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<pre> Longest Total Lunar Eclipse: 1859 Aug 13 Duration = 01h47m04s
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Shortest Total Lunar Eclipse: 1856 Oct 13 Duration = 00h06m50s
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</pre>
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<pre>
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Longest Partial Lunar Eclipse: 1892 May 11 Duration = 03h26m59s
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Shortest Partial Lunar Eclipse: 1900 Jun 13 Duration = 00h08m11s
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</pre>
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<pre>
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Largest Total Lunar Eclipse: 1801 Mar 30 Umbra Magnitude = 1.8447
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Smallest Total Lunar Eclipse: 1856 Oct 13 Umbra Magnitude = 1.0021
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</pre>
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<pre>
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Largest Partial Lunar Eclipse: 1899 Dec 17 Umbra Magnitude = 0.9969
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Smallest Partial Lunar Eclipse: 1900 Jun 13 Umbra Magnitude = 0.0012
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</pre>
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<pre>
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Largest Penumbral Lunar Eclipse: 1806 Jun 30 Pen. Magnitude = 1.0581
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Smallest Penumbral Lunar Eclipse: 1872 Jun 21 Pen. Magnitude = 0.0010
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</pre>
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<p><font size="6">T</font>otal penumbral eclipses are lunar eclipses in which
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the entire Moon passes through the penumbra but misses the umbral shadow.
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Total penumbral eclipses (and magnitudes) for the century are:
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<pre>
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Total Penumbral Eclipse: 1806 Jun 30 Pen. Magnitude = 1.0581
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</pre>
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<p><center><img src="/web/20080219040049im_/http://sunearth.gsfc.nasa.gov/eclipse/image/bluePixel.gif" width="300" height="2" alt="Blue Bar"></center>
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<p><center><h4>Description of Lunar Eclipse Catalog</h4></center>
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<p><font size="6">L</font>ocal circumstances at greatest eclipse<font size="1"><sup>3</sup></font>
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for every event during the century are presented in the following catalog.
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The calendar date and <a href="/web/20080219040049/http://sunearth.gsfc.nasa.gov/eclipse/SEhelp/TimeZone.html"> Universal Time </a> of the instant of greatest eclipse are found in the first two columns.
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The eclipse type is given (T=Total, P=Partial, or N=Penumbral) along with the <a href="/web/20080219040049/http://sunearth.gsfc.nasa.gov/eclipse/LEsaros/LEsaros.html"> Saros series</a>.
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Gamma is the distance of the Moon's center from the shadow axis of Earth at greatest eclipse (in Earth radii).
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The penumbral and umbral magnitudes of the eclipse are defined as the fractions of the Moon's diameter obscured by each shadow at greatest eclipse.
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The semi-durations of the partial and total phases of the eclipse are given to the nearest minute.
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Finally, the Greenwich Sidereal Time at 00:00 U.T., along with the Moon's Geocentric Right Ascension and Declination at greatest eclipse complete each record.
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For a detailed key and additional information about the catalog, see:
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<a href="LEcatkey.html">Key to Catalog of Lunar Eclipses</a>.
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<p>
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<font size="6">F</font>or any eclipse in the catalog, the start and end times of the partial eclipse phases can be calculated by respectively subtracting and adding the semi-duration of the partial phase (S.D. Par) to the instant of greatest eclipse.
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Similarly, the start and end times of the total eclipse can be calculated by either subtracting or adding the semi-duration of the total phase (S.D. Tot) to the instant of greatest eclipse.
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For a detailed example, see <a href="LEcatkey.html#contact">Contact - Key to Lunar Eclipse Catalogs</a>.
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<p>
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<font size="6">T</font>o determine whether an eclipse is visible from a specific geographic location, it is simply a matter of calculating the Moon's altitude and azimuth during each phase of the eclipse.
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The calculations can be performed on any pocket calculator having trigonometric functions (SIN, COS, TAN).
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Armed with the latitude and longitude of the location, the lunar eclipse catalog provides all the additional information needed to make the calculations.
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For the equations and an example of how to calculate the Moon's altitude for a specific location, see <a href="LEcatkey.html#altitude">Altitude - Key to Lunar Eclipse Catalogs</a>.
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<p><center><img src="/web/20080219040049im_/http://sunearth.gsfc.nasa.gov/eclipse/image/bluePixel.gif" width="300" height="2" alt="Blue Bar"></center>
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<p><center><h4>Footnotes</h4></center>
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<blockquote>
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<font size="1"><sup>1</sup></font>The terms BCE and CE are abbreviations for
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"Before Common Era" and "Common Era," respectively.
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They are the secular equivalents to the BC and AD dating conventions.
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(See: <a href="/web/20080219040049/http://sunearth.gsfc.nasa.gov/eclipse/SEhelp/dates.html"> Year Dating Conventions </a>)
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<p><font size="1"><sup>2</sup></font>Central lunar eclipses are eclipses in which some portion of the Moon passes the central axis
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of Earth's umbral shadow.
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All penumbral and partial lunar eclipses are non-central eclipses since the Moon misses the shadow axis.
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However, total eclipses may be either non-central (frequently) or central (occasionally).
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Central total eclipses are longer and usually darker than non-central total eclipses.
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<p>
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<font size="1"><sup>3</sup></font>Greatest eclipse is defined as the instant when
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the Moon passes closest to the axis of Earth's shadow.
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The instant of greatest eclipse corresponds to the maximum phase of the eclipse.
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</blockquote>
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<pre>
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</pre>
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<center><img src="/web/20080219040049im_/http://sunearth.gsfc.nasa.gov/eclipse/image/bluePixel.gif" width="400" height="3" alt="Blue Bar"></center>
|
|
<center><h3>Lunar Eclipses: 1801 to 1900</h3></center>
|
|
<center><h4>( 1801 CE to 1900 CE )</h4> </center>
|
|
<center><img src="/web/20080219040049im_/http://sunearth.gsfc.nasa.gov/eclipse/image/bluePixel.gif" width="400" height="3" alt="Blue Bar"></center>
|
|
<pre>
|
|
<b>Local Circumstances at Greatest Eclipse: 1801 to 1900</b>
|
|
|
|
U.T.
|
|
Greatest Saros Pen. Umb. S.D. S.D. GST Moon Moon
|
|
Date Eclipse Type # Gamma Mag. Mag. Par Tot (0 UT) RA Dec
|
|
h h °
|
|
<hr align="LEFT" width="650">
|
|
1801 Mar 30 05:24 T- 119 0.006 2.882 1.845 111m 51m 12.5 12.55 -3.6
|
|
1801 Sep 22 07:19 T+ 124 -0.107 2.680 1.672 109m 49m 0.0 23.93 -0.6
|
|
1802 Mar 19 11:15 P 129 -0.752 1.542 0.447 76m - 11.8 11.87 0.1
|
|
1802 Sep 11 22:36 P 134 0.610 1.738 0.768 85m - 23.3 23.27 -4.0
|
|
1803 Feb 06 17:10 N 101 1.532 0.118 -0.994 - - 9.1 9.34 17.0
|
|
1803 Mar 08 11:17 N 139 -1.465 0.243 -0.873 - - 11.0 11.16 4.0
|
|
1803 Aug 03 07:05 N 106 -1.235 0.604 -0.390 - - 20.7 20.86 -18.9
|
|
1803 Sep 01 15:19 N 144 1.328 0.425 -0.553 - - 22.7 22.61 -7.3
|
|
1804 Jan 26 21:21 P 111 0.788 1.457 0.397 69m - 8.3 8.56 19.5
|
|
1804 Jul 22 17:38 P 116 -0.514 1.954 0.906 98m - 20.0 20.13 -20.7
|
|
<hr align="LEFT" width="650">
|
|
1805 Jan 15 08:41 T- 121 0.066 2.756 1.747 107m 49m 7.6 7.79 21.2
|
|
1805 Jul 11 21:05 T- 126 0.256 2.448 1.360 114m 44m 19.3 19.37 -21.9
|
|
1806 Jan 05 00:02 P 131 -0.598 1.771 0.781 86m - 6.9 7.01 22.1
|
|
1806 Jun 30 21:44 N 136 1.011 1.058 -0.023 - - 18.6 18.59 -22.3
|
|
1806 Nov 26 02:05 N 103 1.485 0.170 -0.875 - - 4.3 4.07 22.2
|
|
1806 Dec 25 14:48 N 141 -1.289 0.518 -0.501 - - 6.2 6.22 22.2
|
|
1807 May 21 16:49 P 108 -0.942 1.148 0.140 42m - 15.9 15.82 -21.0
|
|
1807 Nov 15 08:10 P 113 0.848 1.368 0.269 61m - 3.6 3.30 19.1
|
|
1808 May 10 07:38 T+ 118 -0.174 2.539 1.569 105m 47m 15.2 15.13 -17.8
|
|
1808 Nov 03 08:13 T- 123 0.161 2.638 1.519 116m 49m 2.8 2.55 15.2
|
|
<hr align="LEFT" width="650">
|
|
1809 Apr 30 00:33 P 128 0.549 1.853 0.879 90m - 14.5 14.46 -14.0
|
|
1809 Oct 23 09:02 P 133 -0.544 1.919 0.832 97m - 2.1 1.84 10.8
|
|
1810 Mar 21 02:55 N 100 -1.421 0.294 -0.763 - - 11.9 11.96 -1.2
|
|
1810 Apr 19 14:54 N 138 1.316 0.467 -0.551 - - 13.8 13.81 -9.8
|
|
1810 Sep 13 06:27 N 105 1.430 0.245 -0.747 - - 23.4 23.34 -2.7
|
|
1810 Oct 12 16:39 N 143 -1.223 0.642 -0.383 - - 1.4 1.17 6.2
|
|
1811 Mar 10 06:37 P 110 -0.753 1.546 0.438 76m - 11.1 11.30 3.8
|
|
1811 Sep 02 22:42 P 115 0.697 1.577 0.610 78m - 22.7 22.72 -7.3
|
|
1812 Feb 27 06:05 T+ 120 -0.054 2.832 1.718 117m 52m 10.4 10.62 8.7
|
|
1812 Aug 22 15:01 Tm 125 -0.023 2.825 1.838 108m 51m 22.1 22.09 -11.8
|
|
<hr align="LEFT" width="650">
|
|
1813 Feb 15 08:50 P 130 0.645 1.726 0.654 87m - 9.7 9.92 13.3
|
|
1813 Aug 12 02:53 P 135 -0.808 1.409 0.371 68m - 21.3 21.44 -15.9
|
|
1814 Jan 06 07:28 N 102 -1.412 0.282 -0.717 - - 7.0 7.11 21.1
|
|
1814 Feb 04 18:47 N 140 1.293 0.510 -0.506 - - 9.0 9.21 17.5
|
|
1814 Jul 02 16:51 N 107 1.223 0.675 -0.415 - - 18.7 18.73 -22.0
|
|
1814 Dec 26 23:08 P 112 -0.757 1.482 0.488 71m - 6.3 6.34 22.6
|
|
1815 Jun 21 18:06 T 117 0.450 2.083 1.013 104m 9m 17.9 17.96 -23.1
|
|
1815 Dec 16 12:55 T+ 122 -0.091 2.724 1.690 109m 50m 5.6 5.55 23.2
|
|
1816 Jun 10 01:14 T 127 -0.337 2.264 1.247 105m 36m 17.2 17.20 -23.3
|
|
1816 Dec 04 20:35 P 132 0.632 1.760 0.669 89m - 4.9 4.74 22.9
|
|
<hr align="LEFT" width="650">
|
|
1817 May 01 07:44 N 99 1.459 0.180 -0.787 - - 14.6 14.58 -13.6
|
|
1817 May 30 15:07 N 137 -1.061 0.913 -0.059 - - 16.5 16.45 -22.8
|
|
1817 Nov 23 21:27 N 142 1.343 0.471 -0.653 - - 4.2 3.92 21.6
|
|
1818 Apr 21 00:20 P 109 0.773 1.447 0.463 70m - 13.9 13.90 -10.9
|
|
1818 Oct 14 05:25 P 114 -0.918 1.224 0.156 46m - 1.5 1.27 7.2
|
|
1819 Apr 10 13:08 T- 119 0.050 2.800 1.762 112m 51m 13.2 13.22 -7.7
|
|
1819 Oct 03 15:13 Tm 124 -0.151 2.600 1.592 108m 48m 0.8 0.59 3.7
|
|
1820 Mar 29 18:42 P 129 -0.711 1.616 0.522 82m - 12.5 12.53 -4.1
|
|
1820 Sep 22 06:35 P 134 0.561 1.830 0.857 89m - 0.1 23.93 0.2
|
|
1821 Feb 17 01:05 N 101 1.547 0.089 -1.018 - - 9.8 10.06 13.4
|
|
<hr align="LEFT" width="650">
|
|
|
|
</pre>
|
|
<center><img src="/web/20080219040049im_/http://sunearth.gsfc.nasa.gov/eclipse/image/bluePixel.gif" width="400" height="3" alt="Blue Bar"></center>
|
|
<center><h3>Lunar Eclipses: 1801 to 1900</h3></center>
|
|
<center><h4>( 1801 CE to 1900 CE )</h4> </center>
|
|
<center><img src="/web/20080219040049im_/http://sunearth.gsfc.nasa.gov/eclipse/image/bluePixel.gif" width="400" height="3" alt="Blue Bar"></center>
|
|
<pre>
|
|
<b>Local Circumstances at Greatest Eclipse: 1801 to 1900</b>
|
|
|
|
U.T.
|
|
Greatest Saros Pen. Umb. S.D. S.D. GST Moon Moon
|
|
Date Eclipse Type # Gamma Mag. Mag. Par Tot (0 UT) RA Dec
|
|
h h °
|
|
<hr align="LEFT" width="650">
|
|
1821 Mar 18 18:45 N 139 -1.429 0.307 -0.805 - - 11.7 11.83 -0.3
|
|
1821 Aug 13 14:26 N 106 -1.307 0.475 -0.524 - - 21.4 21.56 -15.9
|
|
1821 Sep 11 23:05 N 144 1.277 0.522 -0.461 - - 23.4 23.27 -3.3
|
|
1822 Feb 06 05:43 P 111 0.796 1.441 0.384 68m - 9.1 9.31 16.5
|
|
1822 Aug 03 00:30 P 116 -0.594 1.810 0.758 92m - 20.7 20.85 -18.3
|
|
1823 Jan 26 17:25 T- 121 0.073 2.742 1.737 107m 49m 8.3 8.56 18.9
|
|
1823 Jul 23 03:32 T- 126 0.170 2.607 1.517 116m 50m 20.0 20.10 -20.1
|
|
1824 Jan 16 08:54 P 131 -0.594 1.779 0.788 86m - 7.6 7.80 20.5
|
|
1824 Jul 11 04:15 P 136 0.924 1.217 0.138 45m - 19.3 19.34 -21.3
|
|
1824 Dec 06 10:32 N 103 1.498 0.150 -0.900 - - 5.0 4.86 24.0
|
|
<hr align="LEFT" width="650">
|
|
1825 Jan 04 23:32 N 141 -1.289 0.519 -0.503 - - 7.0 7.03 21.4
|
|
1825 Jun 01 00:06 P 108 -1.009 1.023 0.020 16m - 16.6 16.56 -23.0
|
|
1825 Nov 25 16:09 P 113 0.864 1.340 0.235 57m - 4.3 4.07 21.6
|
|
1826 May 21 15:15 T+ 118 -0.239 2.419 1.452 104m 44m 15.9 15.85 -20.4
|
|
1826 Nov 14 15:56 T- 123 0.184 2.597 1.475 116m 48m 3.5 3.29 18.4
|
|
1827 May 11 08:17 P 128 0.491 1.959 0.986 94m - 15.2 15.16 -17.2
|
|
1827 Nov 03 16:52 P 133 -0.515 1.972 0.885 99m - 2.8 2.55 14.5
|
|
1828 Mar 31 10:39 N 100 -1.463 0.217 -0.840 - - 12.6 12.63 -5.6
|
|
1828 Apr 29 22:28 N 138 1.267 0.557 -0.462 - - 14.5 14.49 -13.5
|
|
1828 Sep 23 14:19 N 105 1.473 0.167 -0.825 - - 0.2 24.00 1.6
|
|
<hr align="LEFT" width="650">
|
|
1828 Oct 23 00:45 N 143 -1.189 0.705 -0.321 - - 2.1 1.86 10.2
|
|
1829 Mar 20 14:08 P 110 -0.789 1.479 0.372 71m - 11.9 11.97 -0.6
|
|
1829 Sep 13 06:33 P 115 0.751 1.479 0.510 72m - 23.5 23.38 -3.2
|
|
1830 Mar 09 13:43 T+ 120 -0.083 2.777 1.667 117m 52m 11.1 11.30 4.5
|
|
1830 Sep 02 22:38 T- 125 0.037 2.801 1.809 108m 50m 22.8 22.76 -7.8
|
|
1831 Feb 26 16:56 P 130 0.624 1.761 0.695 89m - 10.4 10.62 9.4
|
|
1831 Aug 23 10:00 P 135 -0.743 1.532 0.489 77m - 22.1 22.12 -12.3
|
|
1832 Jan 17 16:18 N 102 -1.414 0.278 -0.719 - - 7.7 7.90 19.4
|
|
1832 Feb 16 03:21 N 140 1.278 0.534 -0.478 - - 9.7 9.94 13.9
|
|
1832 Jul 12 23:16 N 107 1.308 0.519 -0.573 - - 19.4 19.47 -20.7
|
|
<hr align="LEFT" width="650">
|
|
1832 Aug 11 14:15 Nb 145 -1.540 0.092 -0.995 - - 21.3 21.44 -16.6
|
|
1833 Jan 06 08:00 P 112 -0.761 1.474 0.479 71m - 7.0 7.15 21.7
|
|
1833 Jul 02 00:43 P 117 0.533 1.929 0.862 98m - 18.7 18.71 -22.6
|
|
1833 Dec 26 21:33 T+ 122 -0.095 2.717 1.680 109m 49m 6.3 6.36 23.3
|
|
1834 Jun 21 08:20 T+ 127 -0.258 2.406 1.393 107m 43m 17.9 17.96 -23.7
|
|
1834 Dec 16 04:48 P 132 0.625 1.775 0.680 90m - 5.6 5.54 23.9
|
|
1835 May 12 15:29 Ne 99 1.516 0.074 -0.891 - - 15.3 15.29 -16.6
|
|
1835 Jun 10 22:36 P 137 -0.989 1.043 0.074 30m - 17.2 17.21 -24.0
|
|
1835 Dec 05 05:20 N 142 1.329 0.498 -0.628 - - 4.9 4.71 23.5
|
|
1836 May 01 08:07 P 109 0.830 1.342 0.358 63m - 14.6 14.59 -14.4
|
|
<hr align="LEFT" width="650">
|
|
1836 Oct 24 13:15 P 114 -0.947 1.169 0.101 37m - 2.2 1.96 11.1
|
|
1837 Apr 20 20:41 T- 119 0.104 2.702 1.665 112m 50m 13.9 13.90 -11.6
|
|
1837 Oct 13 23:17 T+ 124 -0.188 2.532 1.524 107m 46m 1.5 1.26 7.8
|
|
1838 Apr 10 01:59 P 129 -0.662 1.705 0.613 87m - 13.2 13.20 -8.3
|
|
1838 Oct 03 14:41 P 134 0.518 1.910 0.935 91m - 0.8 0.59 4.4
|
|
1839 Feb 28 08:54 Ne 101 1.567 0.049 -1.053 - - 10.5 10.76 9.4
|
|
1839 Mar 30 02:03 N 139 -1.385 0.386 -0.722 - - 12.5 12.49 -4.5
|
|
1839 Aug 24 21:52 N 106 -1.374 0.353 -0.651 - - 22.2 22.24 -12.3
|
|
1839 Sep 23 06:57 N 144 1.231 0.608 -0.380 - - 0.1 23.93 0.9
|
|
1840 Feb 17 14:02 P 111 0.807 1.417 0.366 67m - 9.8 10.04 12.9
|
|
<hr align="LEFT" width="650">
|
|
|
|
</pre>
|
|
<center><img src="/web/20080219040049im_/http://sunearth.gsfc.nasa.gov/eclipse/image/bluePixel.gif" width="400" height="3" alt="Blue Bar"></center>
|
|
<center><h3>Lunar Eclipses: 1801 to 1900</h3></center>
|
|
<center><h4>( 1801 CE to 1900 CE )</h4> </center>
|
|
<center><img src="/web/20080219040049im_/http://sunearth.gsfc.nasa.gov/eclipse/image/bluePixel.gif" width="400" height="3" alt="Blue Bar"></center>
|
|
<pre>
|
|
<b>Local Circumstances at Greatest Eclipse: 1801 to 1900</b>
|
|
|
|
U.T.
|
|
Greatest Saros Pen. Umb. S.D. S.D. GST Moon Moon
|
|
Date Eclipse Type # Gamma Mag. Mag. Par Tot (0 UT) RA Dec
|
|
h h °
|
|
<hr align="LEFT" width="650">
|
|
1840 Aug 13 07:23 P 116 -0.672 1.670 0.612 85m - 21.5 21.55 -15.2
|
|
1841 Feb 06 02:07 T- 121 0.081 2.725 1.723 107m 49m 9.1 9.31 15.8
|
|
1841 Aug 02 10:01 T- 126 0.084 2.764 1.673 118m 53m 20.7 20.82 -17.7
|
|
1842 Jan 26 17:44 P 131 -0.588 1.788 0.799 86m - 8.4 8.57 18.1
|
|
1842 Jul 22 10:47 P 136 0.838 1.374 0.297 64m - 20.0 20.07 -19.6
|
|
1842 Dec 17 19:02 N 103 1.508 0.134 -0.920 - - 5.7 5.68 24.8
|
|
1843 Jan 16 08:14 N 141 -1.289 0.521 -0.503 - - 7.7 7.81 19.8
|
|
1843 Jun 12 07:22 N 108 -1.077 0.897 -0.102 - - 17.3 17.32 -24.2
|
|
1843 Jul 11 16:50 Nb 146 1.547 0.048 -0.978 - - 19.3 19.32 -20.7
|
|
1843 Dec 07 00:11 P 113 0.879 1.316 0.207 54m - 5.0 4.86 23.3
|
|
<hr align="LEFT" width="650">
|
|
1844 May 31 22:51 T 118 -0.305 2.295 1.331 102m 39m 16.6 16.59 -22.4
|
|
1844 Nov 24 23:45 T- 123 0.203 2.564 1.440 115m 47m 4.3 4.05 20.9
|
|
1845 May 21 15:54 T 128 0.428 2.074 1.102 97m 23m 15.9 15.89 -19.8
|
|
1845 Nov 14 00:50 P 133 -0.492 2.013 0.927 100m - 3.5 3.28 17.7
|
|
1846 Apr 11 18:11 N 100 -1.513 0.125 -0.932 - - 13.3 13.29 -9.7
|
|
1846 May 11 05:54 N 138 1.211 0.661 -0.359 - - 15.2 15.19 -16.6
|
|
1846 Oct 04 22:21 N 105 1.508 0.103 -0.890 - - 0.9 0.66 5.9
|
|
1846 Nov 03 08:59 N 143 -1.162 0.754 -0.271 - - 2.8 2.56 13.9
|
|
1847 Mar 31 21:27 P 110 -0.835 1.394 0.290 64m - 12.6 12.63 -4.9
|
|
1847 Sep 24 14:34 P 115 0.797 1.396 0.424 67m - 0.2 0.04 1.1
|
|
<hr align="LEFT" width="650">
|
|
1848 Mar 19 21:12 T+ 120 -0.119 2.708 1.604 116m 51m 11.8 11.96 0.1
|
|
1848 Sep 13 06:19 T- 125 0.092 2.703 1.705 108m 50m 23.5 23.42 -3.7
|
|
1849 Mar 09 00:56 P 130 0.598 1.806 0.747 91m - 11.1 11.30 5.1
|
|
1849 Sep 02 17:10 P 135 -0.681 1.650 0.600 84m - 22.8 22.79 -8.4
|
|
1850 Jan 28 01:06 N 102 -1.418 0.269 -0.725 - - 8.5 8.67 16.9
|
|
1850 Feb 26 11:48 N 140 1.259 0.567 -0.440 - - 10.4 10.64 9.9
|
|
1850 Jul 24 05:40 N 107 1.393 0.363 -0.729 - - 20.1 20.20 -18.7
|
|
1850 Aug 22 20:55 N 145 -1.468 0.226 -0.866 - - 22.1 22.12 -13.0
|
|
1851 Jan 17 16:51 P 112 -0.766 1.466 0.470 70m - 7.8 7.94 20.0
|
|
1851 Jul 13 07:22 P 117 0.616 1.776 0.712 92m - 19.4 19.46 -21.4
|
|
<hr align="LEFT" width="650">
|
|
1852 Jan 07 06:11 T+ 122 -0.099 2.712 1.671 109m 49m 7.1 7.17 22.4
|
|
1852 Jul 01 15:26 T+ 127 -0.180 2.548 1.539 109m 48m 18.7 18.71 -23.3
|
|
1852 Dec 26 13:03 P 132 0.620 1.785 0.686 90m - 6.3 6.36 23.9
|
|
1853 Jun 21 06:02 P 137 -0.914 1.179 0.212 49m - 18.0 17.97 -24.4
|
|
1853 Dec 15 13:19 N 142 1.319 0.518 -0.609 - - 5.6 5.52 24.5
|
|
1854 May 12 15:46 P 109 0.892 1.228 0.244 53m - 15.3 15.30 -17.3
|
|
1854 Nov 04 21:13 P 114 -0.971 1.126 0.058 28m - 2.9 2.67 14.7
|
|
1855 May 02 04:05 T- 119 0.163 2.594 1.556 111m 49m 14.6 14.59 -15.1
|
|
1855 Oct 25 07:29 T+ 124 -0.218 2.478 1.470 106m 45m 2.2 1.95 11.8
|
|
1856 Apr 20 09:07 P 129 -0.607 1.806 0.715 93m - 13.9 13.87 -12.1
|
|
<hr align="LEFT" width="650">
|
|
1856 Oct 13 22:54 T 134 0.481 1.980 1.002 93m 3m 1.5 1.26 8.6
|
|
1857 Apr 09 09:13 N 139 -1.335 0.477 -0.627 - - 13.2 13.16 -8.7
|
|
1857 Sep 04 05:22 N 106 -1.438 0.240 -0.769 - - 22.9 22.91 -8.5
|
|
1857 Oct 03 14:57 N 144 1.191 0.684 -0.309 - - 0.8 0.59 5.1
|
|
1858 Feb 27 22:14 P 111 0.825 1.381 0.336 64m - 10.5 10.74 8.9
|
|
1858 Aug 24 14:21 P 116 -0.745 1.539 0.476 77m - 22.2 22.23 -11.7
|
|
1859 Feb 17 10:43 T- 121 0.095 2.698 1.700 106m 49m 9.8 10.03 12.2
|
|
1859 Aug 13 16:34 Tm 126 0.004 2.914 1.820 118m 54m 21.4 21.52 -14.7
|
|
1860 Feb 07 02:30 P 131 -0.579 1.805 0.816 87m - 9.1 9.32 15.0
|
|
1860 Aug 01 17:25 P 136 0.755 1.526 0.450 77m - 20.7 20.79 -17.2
|
|
<hr align="LEFT" width="650">
|
|
|
|
</pre>
|
|
<center><img src="/web/20080219040049im_/http://sunearth.gsfc.nasa.gov/eclipse/image/bluePixel.gif" width="400" height="3" alt="Blue Bar"></center>
|
|
<center><h3>Lunar Eclipses: 1801 to 1900</h3></center>
|
|
<center><h4>( 1801 CE to 1900 CE )</h4> </center>
|
|
<center><img src="/web/20080219040049im_/http://sunearth.gsfc.nasa.gov/eclipse/image/bluePixel.gif" width="400" height="3" alt="Blue Bar"></center>
|
|
<pre>
|
|
<b>Local Circumstances at Greatest Eclipse: 1801 to 1900</b>
|
|
|
|
U.T.
|
|
Greatest Saros Pen. Umb. S.D. S.D. GST Moon Moon
|
|
Date Eclipse Type # Gamma Mag. Mag. Par Tot (0 UT) RA Dec
|
|
h h °
|
|
<hr align="LEFT" width="650">
|
|
1860 Dec 28 03:34 N 103 1.516 0.121 -0.937 - - 6.5 6.50 24.7
|
|
1861 Jan 26 16:54 N 141 -1.287 0.525 -0.500 - - 8.4 8.58 17.4
|
|
1861 Jun 22 14:35 N 108 -1.148 0.765 -0.230 - - 18.1 18.09 -24.6
|
|
1861 Jul 21 23:50 N 146 1.466 0.195 -0.828 - - 20.0 20.05 -19.0
|
|
1861 Dec 17 08:19 P 113 0.888 1.300 0.188 52m - 5.7 5.67 24.2
|
|
1862 Jun 12 06:21 T 118 -0.376 2.164 1.202 99m 32m 17.4 17.35 -23.5
|
|
1862 Dec 06 07:40 T- 123 0.216 2.541 1.416 115m 46m 5.0 4.84 22.7
|
|
1863 Jun 01 23:26 T 128 0.361 2.198 1.225 100m 34m 16.7 16.62 -21.7
|
|
1863 Nov 25 08:56 P 133 -0.476 2.043 0.957 101m - 4.3 4.04 20.3
|
|
1864 Apr 22 01:36 Ne 100 -1.569 0.024 -1.034 - - 14.0 13.97 -13.7
|
|
<hr align="LEFT" width="650">
|
|
1864 May 21 13:12 N 138 1.150 0.773 -0.248 - - 16.0 15.91 -19.2
|
|
1864 Oct 15 06:31 N 105 1.538 0.048 -0.946 - - 1.6 1.34 10.1
|
|
1864 Nov 13 17:21 N 143 -1.140 0.794 -0.231 - - 3.5 3.29 17.1
|
|
1865 Apr 11 04:38 P 110 -0.886 1.300 0.197 53m - 13.3 13.30 -9.1
|
|
1865 Oct 04 22:40 P 115 0.839 1.322 0.346 61m - 0.9 0.70 5.4
|
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1866 Mar 31 04:33 T+ 120 -0.161 2.627 1.528 116m 49m 12.6 12.62 -4.2
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1866 Sep 24 14:07 T- 125 0.141 2.616 1.613 108m 48m 0.2 0.08 0.6
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1867 Mar 20 08:49 P 130 0.566 1.862 0.809 93m - 11.8 11.97 0.8
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1867 Sep 14 00:26 P 135 -0.624 1.757 0.701 89m - 23.5 23.44 -4.2
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1868 Feb 08 09:50 N 102 -1.425 0.254 -0.738 - - 9.2 9.40 13.7
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<hr align="LEFT" width="650">
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1868 Mar 08 20:10 N 140 1.234 0.610 -0.392 - - 11.1 11.32 5.7
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1868 Aug 03 12:09 N 107 1.474 0.215 -0.878 - - 20.8 20.90 -16.1
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1868 Sep 02 03:41 N 145 -1.401 0.350 -0.745 - - 22.8 22.79 -9.1
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1869 Jan 28 01:38 P 112 -0.773 1.452 0.456 69m - 8.5 8.70 17.4
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1869 Jul 23 14:03 P 117 0.696 1.627 0.564 83m - 20.1 20.19 -19.4
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1870 Jan 17 14:46 T+ 122 -0.104 2.704 1.661 110m 49m 7.8 7.96 20.6
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1870 Jul 12 22:34 T+ 127 -0.102 2.689 1.683 110m 50m 19.4 19.46 -22.0
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1871 Jan 06 21:17 P 132 0.615 1.796 0.694 91m - 7.1 7.17 23.0
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1871 Jul 02 13:28 P 137 -0.840 1.314 0.349 62m - 18.7 18.74 -23.9
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1871 Dec 26 21:19 N 142 1.311 0.533 -0.595 - - 6.3 6.34 24.5
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<hr align="LEFT" width="650">
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1872 May 22 23:18 P 109 0.959 1.105 0.121 38m - 16.1 16.02 -19.7
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1872 Jun 21 06:43 Nb 147 -1.556 0.001 -0.964 - - 18.0 18.00 -25.0
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1872 Nov 15 05:20 P 114 -0.988 1.095 0.028 19m - 3.6 3.41 17.7
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1873 May 12 11:20 T- 119 0.229 2.474 1.434 110m 45m 15.4 15.29 -18.0
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1873 Nov 04 15:51 T+ 124 -0.241 2.436 1.427 105m 43m 2.9 2.67 15.3
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1874 May 01 16:03 P 129 -0.542 1.923 0.833 98m - 14.6 14.56 -15.6
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1874 Oct 25 07:16 T 134 0.451 2.036 1.056 95m 17m 2.2 1.96 12.5
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1875 Apr 20 16:15 N 139 -1.277 0.580 -0.519 - - 13.9 13.84 -12.6
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1875 Sep 15 12:58 N 106 -1.496 0.137 -0.878 - - 23.6 23.57 -4.4
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1875 Oct 14 23:03 N 144 1.158 0.748 -0.250 - - 1.5 1.27 9.3
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<hr align="LEFT" width="650">
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1876 Mar 10 06:22 P 111 0.848 1.338 0.299 60m - 11.2 11.42 4.7
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1876 Sep 03 21:23 P 116 -0.813 1.416 0.347 67m - 22.9 22.90 -7.9
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1877 Feb 27 19:16 T- 121 0.112 2.664 1.670 106m 48m 10.5 10.73 8.2
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1877 Aug 23 23:12 T+ 126 -0.074 2.787 1.689 118m 53m 22.2 22.20 -11.2
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1878 Feb 17 11:11 P 131 -0.567 1.827 0.839 88m - 9.8 10.04 11.4
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1878 Aug 13 00:08 P 136 0.676 1.672 0.596 86m - 21.4 21.48 -14.2
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1879 Jan 08 12:04 N 103 1.524 0.107 -0.954 - - 7.2 7.32 23.7
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1879 Feb 07 01:29 N 141 -1.281 0.536 -0.490 - - 9.1 9.32 14.3
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1879 Jul 03 21:51 N 108 -1.217 0.636 -0.356 - - 18.8 18.85 -24.1
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1879 Aug 02 06:58 N 146 1.389 0.335 -0.686 - - 20.7 20.77 -16.6
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<hr align="LEFT" width="650">
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</pre>
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<center><img src="/web/20080219040049im_/http://sunearth.gsfc.nasa.gov/eclipse/image/bluePixel.gif" width="400" height="3" alt="Blue Bar"></center>
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<center><h3>Lunar Eclipses: 1801 to 1900</h3></center>
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<center><h4>( 1801 CE to 1900 CE )</h4> </center>
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<center><img src="/web/20080219040049im_/http://sunearth.gsfc.nasa.gov/eclipse/image/bluePixel.gif" width="400" height="3" alt="Blue Bar"></center>
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<pre>
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<b>Local Circumstances at Greatest Eclipse: 1801 to 1900</b>
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U.T.
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Greatest Saros Pen. Umb. S.D. S.D. GST Moon Moon
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Date Eclipse Type # Gamma Mag. Mag. Par Tot (0 UT) RA Dec
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h h °
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<hr align="LEFT" width="650">
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1879 Dec 28 16:26 P 113 0.897 1.285 0.171 49m - 6.5 6.49 24.1
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1880 Jun 22 13:50 T 118 -0.448 2.030 1.070 96m 19m 18.1 18.11 -23.9
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1880 Dec 16 15:39 T- 123 0.226 2.521 1.396 115m 45m 5.7 5.65 23.6
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1881 Jun 12 06:54 T 128 0.290 2.328 1.355 103m 40m 17.4 17.37 -22.9
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1881 Dec 05 17:09 P 133 -0.464 2.065 0.980 101m - 5.0 4.83 22.0
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1882 Jun 01 20:22 N 138 1.083 0.897 -0.126 - - 16.7 16.64 -21.1
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1882 Oct 26 14:49 Ne 105 1.561 0.006 -0.989 - - 2.3 2.03 14.1
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1882 Nov 25 01:51 N 143 -1.124 0.823 -0.202 - - 4.3 4.05 19.6
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1883 Apr 22 11:39 P 110 -0.945 1.190 0.090 37m - 14.0 13.97 -13.0
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1883 Oct 16 06:54 P 115 0.873 1.260 0.281 56m - 1.6 1.37 9.6
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<hr align="LEFT" width="650">
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1884 Apr 10 11:47 T+ 120 -0.212 2.533 1.438 114m 47m 13.3 13.29 -8.4
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1884 Oct 04 22:02 T- 125 0.184 2.540 1.531 107m 47m 0.9 0.74 4.9
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1885 Mar 30 16:34 P 130 0.526 1.932 0.886 96m - 12.5 12.63 -3.5
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1885 Sep 24 07:48 P 135 -0.573 1.854 0.792 94m - 0.2 0.10 0.1
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1886 Feb 18 18:29 N 102 -1.437 0.231 -0.757 - - 9.9 10.12 10.0
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1886 Mar 20 04:24 N 140 1.203 0.665 -0.332 - - 11.8 11.99 1.3
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1886 Aug 14 18:42 Ne 107 1.551 0.075 -1.020 - - 21.5 21.59 -12.9
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1886 Sep 13 10:35 N 145 -1.340 0.465 -0.635 - - 23.5 23.44 -4.9
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1887 Feb 08 10:22 P 112 -0.784 1.433 0.437 68m - 9.2 9.44 14.2
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1887 Aug 03 20:49 P 117 0.773 1.485 0.424 74m - 20.8 20.90 -16.7
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<hr align="LEFT" width="650">
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1888 Jan 28 23:20 T+ 122 -0.110 2.695 1.650 110m 49m 8.5 8.73 18.0
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1888 Jul 23 05:45 T+ 127 -0.026 2.828 1.824 110m 51m 20.1 20.20 -20.0
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1889 Jan 17 05:30 P 132 0.611 1.805 0.702 91m - 7.8 7.97 21.3
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1889 Jul 12 20:54 P 137 -0.765 1.451 0.487 71m - 19.4 19.49 -22.6
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1890 Jan 06 05:21 N 142 1.303 0.547 -0.581 - - 7.0 7.15 23.7
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1890 Jun 03 06:45 N 109 1.031 0.974 -0.011 - - 16.8 16.76 -21.3
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1890 Jul 02 14:09 N 147 -1.487 0.127 -0.839 - - 18.7 18.77 -24.5
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1890 Nov 26 13:34 P 114 -0.999 1.073 0.007 9m - 4.4 4.17 20.1
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1891 May 23 18:29 T 119 0.299 2.345 1.305 108m 40m 16.1 16.02 -20.4
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1891 Nov 16 00:19 T+ 124 -0.259 2.402 1.393 104m 42m 3.7 3.41 18.4
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<hr align="LEFT" width="650">
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1892 May 11 22:53 P 129 -0.473 2.050 0.960 103m - 15.3 15.27 -18.6
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1892 Nov 04 15:45 T 134 0.427 2.082 1.099 96m 23m 3.0 2.67 16.1
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1893 Apr 30 23:09 N 139 -1.212 0.698 -0.397 - - 14.6 14.53 -16.1
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1893 Sep 25 20:39 Ne 106 -1.548 0.045 -0.977 - - 0.3 0.23 -0.1
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1893 Oct 25 07:16 N 144 1.131 0.801 -0.203 - - 2.3 1.96 13.2
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1894 Mar 21 14:21 P 111 0.877 1.280 0.248 55m - 11.9 12.09 0.4
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1894 Sep 15 04:31 P 116 -0.875 1.306 0.231 56m - 23.6 23.56 -3.8
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1895 Mar 11 03:39 T- 121 0.138 2.615 1.626 106m 48m 11.2 11.41 4.0
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1895 Sep 04 05:57 T+ 126 -0.145 2.658 1.558 117m 51m 22.9 22.86 -7.4
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1896 Feb 28 19:46 P 131 -0.549 1.859 0.873 89m - 10.5 10.74 7.4
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<hr align="LEFT" width="650">
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1896 Aug 23 06:57 P 136 0.600 1.811 0.735 93m - 22.1 22.16 -10.8
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1897 Jan 18 20:33 N 103 1.533 0.092 -0.971 - - 7.9 8.11 21.7
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1897 Feb 17 09:58 N 141 -1.272 0.554 -0.474 - - 9.8 10.04 10.7
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1897 Jul 14 05:05 N 108 -1.288 0.504 -0.485 - - 19.5 19.61 -22.9
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1897 Aug 12 14:09 N 146 1.314 0.473 -0.546 - - 21.4 21.46 -13.6
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1898 Jan 08 00:35 P 113 0.905 1.272 0.156 47m - 7.2 7.30 23.1
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1898 Jul 03 21:17 P 118 -0.523 1.893 0.934 92m - 18.8 18.87 -23.4
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1898 Dec 27 23:42 T- 123 0.234 2.507 1.382 114m 45m 6.4 6.46 23.5
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1899 Jun 23 14:18 T- 128 0.217 2.463 1.488 105m 45m 18.1 18.13 -23.2
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1899 Dec 17 01:26 P 133 -0.455 2.080 0.997 101m - 5.7 5.63 22.9
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<hr align="LEFT" width="650">
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1900 Jun 13 03:28 P 138 1.013 1.026 0.001 4m - 17.4 17.39 -22.2
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1900 Dec 06 10:26 N 143 -1.113 0.844 -0.180 - - 5.0 4.84 21.4
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<hr align="LEFT" width="650">
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</pre>
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<!--*************************************************************-->
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<pre>
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<center><img src="/web/20080219040049im_/http://sunearth.gsfc.nasa.gov/eclipse/image/bluePixel.gif" width="300" height="2" alt="Blue Bar"></center>
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</pre>
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<p><center><h4>Calendar Dates</h4></center>
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<p>
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<font size="6">T</font>he Julian calendar is used for all dates up to 1582 Oct 04.
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After that date, the Gregorian calendar is used.
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Due to the Gregorian Calendar reform, the day after 1582 Oct 04 (Julian calendar) is 1582 Oct 15 (Gregorian calendar).
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Note that Great Britian did not adopt the Gregorian calendar until 1752.
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For more information, see <a href="/web/20080219040049/http://sunearth.gsfc.nasa.gov/eclipse/SEhelp/calendars.html"> Calendars</a>.
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<p>
|
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<font size="6">T</font>he Julian calendar does not include the year 0, so the year 1 BCE is followed by the year 1 CE.
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This is awkward for arithmetic calculations.
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In this catalog, dates are counted using the astronomical numbering system which recognizes the year 0.
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Historians should note the numerical difference of one year between astronomical dates and BCE dates.
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Thus, the year 0 corresponds to 1 BCE, and the year -100 corresponds to 101 BCE, etc..
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(See: <a href="/web/20080219040049/http://sunearth.gsfc.nasa.gov/eclipse/SEhelp/dates.html"> Year Dating Conventions </a>)
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<p>
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<font size="6">T</font>here is some historical uncertainty as to which years from 43 BCE to 8 CE were counted as leap years.
|
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For the purposes of this catalog, we will assume that <i>all</i> Julian years divisible by 4 will be counted as leap years.
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<p>
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<center><img src="/web/20080219040049im_/http://sunearth.gsfc.nasa.gov/eclipse/image/bluePixel.gif" width="300" height="2" alt="Blue Bar"></center>
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<p><center><h4>Predictions</h4></center>
|
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<p><font size="6">E</font>clipse predictions presented here are based on j=2 ephemerides for the Sun
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(Newcomb, 1895) and Moon (Brown, 1919, and Eckert, Jones and Clark, 1954).
|
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A revised value used for the Moon's secular acceleration is n-dot = -26 arc-sec/cy*cy, as deduced by Morrison and Ward (1975) from 250 years of Mercury transit observations.
|
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<p><font size="6">T</font>he largest uncertainty in the eclipse predictions is caused by fluctuations in <a href="/web/20080219040049/http://sunearth.gsfc.nasa.gov/eclipse/SEhelp/rotation.html">Earth's rotation</a> due primarily to tidal friction of the Moon.
|
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The resultant drift in apparent clock time is expressed as <i><a href="/web/20080219040049/http://sunearth.gsfc.nasa.gov/eclipse/SEhelp/deltaT.html">delta-T</a></i>.
|
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The value for <i>delta-T</i> was determined as follows:
|
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<blockquote>
|
|
1) pre-1600: delta T was calculated from empirical fits to <a href="/web/20080219040049/http://sunearth.gsfc.nasa.gov/eclipse/SEhelp/deltaT2.html">historical records</a> derived by Stephenson (1997)
|
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<br>2) 1600-present: delta T was obtained from published observations
|
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<br>3) future: delta-T was extrapolated from current values and a model of tidal effects
|
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</blockquote>
|
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<p><center><img src="/web/20080219040049im_/http://sunearth.gsfc.nasa.gov/eclipse/image/bluePixel.gif" width="300" height="2" alt="Blue Bar"></center>
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<p><center><h4>Acknowledgments</h4></center>
|
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<p>
|
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<font size="6">A</font>ll eclipse calculations are by Fred Espenak, and he assumes full responsibility for their accuracy.
|
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Some of the information presented in these tables is based on <i><a href="/web/20080219040049/http://sunearth.gsfc.nasa.gov/eclipse/SEpubs/RP1216.html">Fifty Year Canon of Lunar Eclipses: 1986 - 2035</a></i>.
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<p>
|
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<font size="6">P</font>ermission is freely granted to reproduce this data when accompanied by an acknowledgment:
|
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<p><center>"Eclipse Predictions by Fred Espenak, NASA's GSFC"</center>
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<pre>
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</pre>
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<!--*************************************************************-->
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<center><img src="/web/20080219040049im_/http://sunearth.gsfc.nasa.gov/eclipse/image/bluePixel.gif" width="300" height="2" alt="Blue Bar"></center>
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</pre>
|
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<p><center><h3><i><a href="LEcatkey.html"> Key to Catalog Lunar Eclipse </a></i></h3>
|
|
</center>
|
|
<p><center><h3><i><a href="LEcatalog.html"> Index to Catalog of Lunar Eclipses </a></i></h3>
|
|
</center>
|
|
<p><center><h3><i><a href="/web/20080219040049/http://sunearth.gsfc.nasa.gov/eclipse/lunar.html"> NASA Lunar Eclipse Page </a></i></h3>
|
|
</center>
|
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<p><center><h3><i><a href="/web/20080219040049/http://sunearth.gsfc.nasa.gov/eclipse/eclipse.html"> NASA Eclipse Home Page </a></i></h3>
|
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</center>
|
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<pre>
|
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<center><img src="/web/20080219040049im_/http://sunearth.gsfc.nasa.gov/eclipse/image/bluePixel.gif" width="300" height="2" alt="Blue Bar"></center>
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</pre>
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<!--*************************************************************-->
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<p><center><table border="5" cellspacing="5">
|
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<tr><th>
|
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<img src="/web/20080219040049im_/http://sunearth.gsfc.nasa.gov/eclipse/image/NASAlogo.tiny.gif" alt="NASA logo" align="right">
|
|
<br>Eclipse Predictions & WebMaster: Fred Espenak
|
|
<br>e-mail: <a href="https://web.archive.org/web/20080219040049/MAILTO:espenak@gsfc.nasa.gov"> espenak@gsfc.nasa.gov </a>
|
|
<p>Planetary Systems Branch - Code 693
|
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<br>NASA's Goddard Space Flight Center, Greenbelt, Maryland 20771 USA
|
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<br clear="all">
|
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</th></table></center>
|
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<br>
|
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|
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<p><center><i>Last revised: 2003 Sep 11 - F. Espenak</i></center>
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</body>
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</html>
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