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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.
727 lines
48 KiB
HTML
727 lines
48 KiB
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<title>Lunar Eclipses: 2001 to 2100</title>
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<td class="b" nowrap="nowrap"><a href="https://web.archive.org/web/20071228233024/http://sunearth.gsfc.nasa.gov:80/eclipse/LEcat/LE2001-2100.html" title="28 Dec 2007"><strong>Dec</strong></a></td>
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<td class="c" id="displayDayEl" style="width:34px;font-size:24px;white-space:nowrap;" title="You are here: 18:41:27 Feb 29, 2008">29</td>
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<td class="f" nowrap="nowrap"><a href="https://web.archive.org/web/20080331075914/http://sunearth.gsfc.nasa.gov:80/eclipse/LEcat/LE2001-2100.html" title="07:59:14 Mar 31, 2008"><img src="/_static/images/toolbar/wm_tb_nxt_on.png" alt="Next capture" width="14" height="16" border="0" /></a></td>
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<td class="b" nowrap="nowrap"><a href="https://web.archive.org/web/20061231055901/http://sunearth.gsfc.nasa.gov:80/eclipse/LEcat/LE2001-2100.html" title="31 Dec 2006"><strong>2006</strong></a></td>
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<td class="c" id="displayYearEl" title="You are here: 18:41:27 Feb 29, 2008">2008</td>
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<td class="f" nowrap="nowrap"><a href="https://web.archive.org/web/20090321123653/http://sunearth.gsfc.nasa.gov/eclipse/LEcat/LE2001-2100.html" title="21 Mar 2009"><strong>2009</strong></a></td>
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<a class="t" href="/web/20080229184127*/http://sunearth.gsfc.nasa.gov/eclipse/LEcat/LE2001-2100.html" title="See a list of every capture for this URL">89 captures</a>
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<div class="r" title="Timespan for captures of this URL">02 Feb 1999 - 07 Feb 2012</div>
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<span class="c-logo" style="background-image:url(https://archive.org/services/img/alexacrawls);"></span>
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Organization: <a style="color:#33f;" href="https://archive.org/details/alexacrawls" target="_new"><span class="wm-title">Alexa Crawls</span></a>
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<div style="position:absolute;top:0;left:0;width:100%;height:75px;background:linear-gradient(to bottom,rgba(255,255,255,0) 0%,rgba(255,255,255,0) 90%,rgba(255,255,255,255) 100%);"></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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<div style="max-height:75px;overflow:hidden;position:relative;">
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this data is currently not publicly accessible.
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scrolling="no" frameborder="0" style="width:100%; height:100%">
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</div><script type="text/javascript">
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<center><table border="5" cellspacing="5">
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<tr><th>
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<img src="/web/20080229184127im_/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/20080229184127im_/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: 2001 to 2100</h1>
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<h2>( 2001 CE to 2100 CE )</h2>
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<h4>Fred Espenak</h4>
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</center>
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<center><img src="/web/20080229184127im_/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 21st century CE<font size="1"><sup>1</sup></font>, Earth will experience 230 lunar eclipses as follows:
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<pre> All Eclipses = 230 = 100.0%
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Penumbral (N) = 87 = 37.8%
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Partial (P) = 58 = 25.2%
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Total (T) = 85 = 37.0%
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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;) = 143 = 62.2%
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Central<font size="1"><sup>2</sup></font> (T±) = 24 = 10.4%
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Non-Central (T) = 61 = 26.5%
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</pre>
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<center><img src="/web/20080229184127im_/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: 76
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Number of Years with 3 Eclipses: 18
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Number of Years with 4 Eclipses: 6
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</pre>
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<font size="6">W</font>hen four consecutive lunar eclipses are all
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<i>total</i> eclipses, the group is known as a tetrad.
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The following tetrads occur during this century:
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<pre>
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Tetrad (Four Consecutive Total Eclipses): 2003 - 2004
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Tetrad (Four Consecutive Total Eclipses): 2014 - 2015
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Tetrad (Four Consecutive Total Eclipses): 2032 - 2033
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Tetrad (Four Consecutive Total Eclipses): 2043 - 2044
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Tetrad (Four Consecutive Total Eclipses): 2050 - 2051
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Tetrad (Four Consecutive Total Eclipses): 2061 - 2062
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Tetrad (Four Consecutive Total Eclipses): 2072 - 2073
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Tetrad (Four Consecutive Total Eclipses): 2090 - 2091
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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/20080229184127/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): 2013/150 2042/156 2096/151
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3 Saros Series' end (Year/Saros): 2016/109 2027/110 2092/111
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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: 2018 Jul 27 Duration = 01h43m35s
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Shortest Total Lunar Eclipse: 2015 Apr 04 Duration = 00h11m56s
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</pre>
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<pre>
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Longest Partial Lunar Eclipse: 2021 Nov 19 Duration = 03h29m03s
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Shortest Partial Lunar Eclipse: 2042 Sep 29 Duration = 00h11m28s
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</pre>
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<pre>
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Largest Total Lunar Eclipse: 2029 Jun 26 Umbra Magnitude = 1.8488
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Smallest Total Lunar Eclipse: 2015 Apr 04 Umbra Magnitude = 1.0052
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</pre>
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<pre>
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Largest Partial Lunar Eclipse: 2086 Nov 20 Umbra Magnitude = 0.9924
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Smallest Partial Lunar Eclipse: 2042 Sep 29 Umbra Magnitude = 0.0028
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</pre>
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<pre>
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Largest Penumbral Lunar Eclipse: 2070 Apr 25 Pen. Magnitude = 1.0772
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Smallest Penumbral Lunar Eclipse: 2042 Oct 28 Pen. Magnitude = 0.0075
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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: 2006 Mar 14 Pen. Magnitude = 1.0565
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Total Penumbral Eclipse: 2017 Feb 11 Pen. Magnitude = 1.0140
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Total Penumbral Eclipse: 2053 Aug 29 Pen. Magnitude = 1.0453
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Total Penumbral Eclipse: 2066 Dec 31 Pen. Magnitude = 1.0033
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Total Penumbral Eclipse: 2070 Apr 25 Pen. Magnitude = 1.0772
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Total Penumbral Eclipse: 2082 Aug 08 Pen. Magnitude = 1.0272
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Total Penumbral Eclipse: 2085 Jan 10 Pen. Magnitude = 1.0187
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Total Penumbral Eclipse: 2099 Sep 29 Pen. Magnitude = 1.0599
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</pre>
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<p><center><img src="/web/20080229184127im_/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/20080229184127/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/20080229184127/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/20080229184127im_/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/20080229184127/http://sunearth.gsfc.nasa.gov/eclipse/SEhelp/dates.html"> Year Dating Conventions </a>)
|
|
|
|
<p><font size="1"><sup>2</sup></font>Central lunar eclipses are eclipses in which some portion of the Moon passes the central axis
|
|
of Earth's umbral shadow.
|
|
All penumbral and partial lunar eclipses are non-central eclipses since the Moon misses the shadow axis.
|
|
However, total eclipses may be either non-central (frequently) or central (occasionally).
|
|
Central total eclipses are longer and usually darker than non-central total eclipses.
|
|
|
|
<p>
|
|
<font size="1"><sup>3</sup></font>Greatest eclipse is defined as the instant when
|
|
the Moon passes closest to the axis of Earth's shadow.
|
|
The instant of greatest eclipse corresponds to the maximum phase of the eclipse.
|
|
|
|
</blockquote>
|
|
<pre>
|
|
|
|
|
|
<hr align="LEFT" width="650">
|
|
|
|
</pre>
|
|
<center><img src="/web/20080229184127im_/http://sunearth.gsfc.nasa.gov/eclipse/image/bluePixel.gif" width="400" height="3" alt="Blue Bar"></center>
|
|
<center><h3>Lunar Eclipses: 2001 to 2100</h3></center>
|
|
<center><h4>( 2001 CE to 2100 CE )</h4> </center>
|
|
<center><img src="/web/20080229184127im_/http://sunearth.gsfc.nasa.gov/eclipse/image/bluePixel.gif" width="400" height="3" alt="Blue Bar"></center>
|
|
<pre>
|
|
<b>Local Circumstances at Greatest Eclipse: 2001 to 2100</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">
|
|
2001 Jan 09 20:21 T 134 0.372 2.187 1.194 99m 31m 7.3 7.42 22.4
|
|
2001 Jul 05 14:55 P 139 -0.729 1.573 0.499 80m - 18.9 18.99 -23.4
|
|
2001 Dec 30 10:29 N 144 1.073 0.919 -0.110 - - 6.6 6.64 24.2
|
|
2002 May 26 12:03 N 111 1.176 0.714 -0.283 - - 16.3 16.23 -20.0
|
|
2002 Jun 24 21:27 N 149 -1.444 0.235 -0.787 - - 18.2 18.22 -24.8
|
|
2002 Nov 20 01:47 N 116 -1.113 0.886 -0.222 - - 3.9 3.71 18.7
|
|
2003 May 16 03:40 T 121 0.412 2.100 1.134 97m 26m 15.6 15.51 -18.6
|
|
2003 Nov 09 01:19 T 126 -0.432 2.140 1.022 106m 12m 3.2 2.93 16.3
|
|
2004 May 04 20:30 T 131 -0.313 2.288 1.309 102m 38m 14.9 14.81 -16.5
|
|
2004 Oct 28 03:04 T 136 0.285 2.390 1.313 110m 41m 2.5 2.18 13.4
|
|
<hr align="LEFT" width="650">
|
|
2005 Apr 24 09:55 N 141 -1.089 0.890 -0.138 - - 14.2 14.11 -13.9
|
|
2005 Oct 17 12:03 P 146 0.980 1.084 0.068 29m - 1.7 1.47 10.3
|
|
2006 Mar 14 23:48 N 113 1.021 1.056 -0.056 - - 11.5 11.68 3.1
|
|
2006 Sep 07 18:51 P 118 -0.926 1.158 0.190 46m - 23.1 23.11 -6.7
|
|
2007 Mar 03 23:21 T 123 0.317 2.345 1.238 111m 37m 10.8 10.96 6.9
|
|
2007 Aug 28 10:37 T+ 128 -0.214 2.478 1.481 106m 45m 22.4 22.45 -10.0
|
|
2008 Feb 21 03:26 T 133 -0.399 2.171 1.111 103m 25m 10.0 10.25 10.5
|
|
2008 Aug 16 21:10 P 138 0.565 1.862 0.812 94m - 21.7 21.76 -12.9
|
|
2009 Feb 09 14:38 N 143 -1.064 0.924 -0.083 - - 9.3 9.53 13.5
|
|
2009 Jul 07 09:39 N 110 -1.491 0.182 -0.908 - - 19.0 19.14 -23.9
|
|
<hr align="LEFT" width="650">
|
|
2009 Aug 06 00:39 N 148 1.357 0.428 -0.662 - - 21.0 21.05 -15.6
|
|
2009 Dec 31 19:23 P 115 0.977 1.081 0.082 31m - 6.7 6.76 24.0
|
|
2010 Jun 26 11:38 P 120 -0.709 1.603 0.542 82m - 18.3 18.35 -24.0
|
|
2010 Dec 21 08:17 T 125 0.321 2.306 1.261 105m 37m 6.0 5.95 23.7
|
|
2011 Jun 15 20:13 T- 130 0.090 2.712 1.705 110m 50m 17.6 17.59 -23.2
|
|
2011 Dec 10 14:32 T 135 -0.388 2.212 1.111 106m 26m 5.3 5.14 22.6
|
|
2012 Jun 04 11:03 P 140 0.825 1.343 0.376 64m - 16.9 16.86 -21.7
|
|
2012 Nov 28 14:33 N 145 -1.087 0.942 -0.183 - - 4.5 4.33 20.5
|
|
2013 Apr 25 20:07 P 112 -1.012 1.012 0.021 16m - 14.3 14.21 -14.4
|
|
2013 May 25 04:10 Nb 150 1.535 0.040 -0.928 - - 16.2 16.15 -19.4
|
|
<hr align="LEFT" width="650">
|
|
2013 Oct 18 23:50 N 117 1.151 0.791 -0.267 - - 1.8 1.57 11.0
|
|
2014 Apr 15 07:46 T 122 -0.302 2.344 1.296 108m 39m 13.6 13.56 -10.0
|
|
2014 Oct 08 10:55 T 127 0.383 2.171 1.172 100m 30m 1.1 0.92 6.3
|
|
2015 Apr 04 12:00 T 132 0.446 2.105 1.005 105m 6m 12.8 12.89 -5.3
|
|
2015 Sep 28 02:47 T 137 -0.330 2.254 1.282 100m 36m 0.4 0.29 1.5
|
|
2016 Mar 23 11:47 N 142 1.159 0.801 -0.308 - - 12.1 12.22 -0.3
|
|
2016 Aug 18 09:42 Ne 109 1.559 0.017 -0.993 - - 21.8 21.85 -11.4
|
|
2016 Sep 16 18:54 N 147 -1.055 0.933 -0.058 - - 23.7 23.67 -3.3
|
|
2017 Feb 11 00:44 N 114 -1.025 1.014 -0.030 - - 9.4 9.64 13.1
|
|
2017 Aug 07 18:20 P 119 0.867 1.315 0.251 58m - 21.1 21.18 -15.4
|
|
<hr align="LEFT" width="650">
|
|
2018 Jan 31 13:30 T 124 -0.301 2.320 1.321 102m 38m 8.7 8.93 17.0
|
|
2018 Jul 27 20:22 T- 129 0.117 2.706 1.614 118m 52m 20.4 20.47 -19.0
|
|
2019 Jan 21 05:12 T 134 0.369 2.193 1.201 99m 31m 8.0 8.21 20.3
|
|
2019 Jul 16 21:31 P 139 -0.643 1.729 0.658 89m - 19.6 19.73 -21.9
|
|
2020 Jan 10 19:10 N 144 1.073 0.921 -0.111 - - 7.3 7.45 23.0
|
|
2020 Jun 05 19:25 N 111 1.240 0.594 -0.399 - - 17.0 16.97 -21.5
|
|
2020 Jul 05 04:30 N 149 -1.364 0.380 -0.638 - - 18.9 18.99 -24.1
|
|
2020 Nov 30 09:43 N 116 -1.131 0.855 -0.257 - - 4.6 4.48 20.7
|
|
2021 May 26 11:19 T 121 0.477 1.979 1.016 94m 9m 16.3 16.24 -20.7
|
|
2021 Nov 19 09:03 P 126 -0.455 2.098 0.979 105m - 3.9 3.67 19.2
|
|
<hr align="LEFT" width="650">
|
|
|
|
</pre>
|
|
<center><img src="/web/20080229184127im_/http://sunearth.gsfc.nasa.gov/eclipse/image/bluePixel.gif" width="400" height="3" alt="Blue Bar"></center>
|
|
<center><h3>Lunar Eclipses: 2001 to 2100</h3></center>
|
|
<center><h4>( 2001 CE to 2100 CE )</h4> </center>
|
|
<center><img src="/web/20080229184127im_/http://sunearth.gsfc.nasa.gov/eclipse/image/bluePixel.gif" width="400" height="3" alt="Blue Bar"></center>
|
|
<pre>
|
|
<b>Local Circumstances at Greatest Eclipse: 2001 to 2100</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">
|
|
2022 May 16 04:11 T+ 131 -0.253 2.397 1.419 104m 43m 15.6 15.52 -19.3
|
|
2022 Nov 08 10:59 T- 136 0.257 2.440 1.363 110m 43m 3.2 2.90 16.9
|
|
2023 May 05 17:23 N 141 -1.035 0.989 -0.041 - - 14.9 14.81 -17.2
|
|
2023 Oct 28 20:14 P 146 0.947 1.143 0.127 40m - 2.5 2.16 14.1
|
|
2024 Mar 25 07:13 N 113 1.061 0.982 -0.128 - - 12.2 12.34 -1.2
|
|
2024 Sep 18 02:44 P 118 -0.979 1.062 0.091 32m - 23.8 23.77 -2.6
|
|
2025 Mar 14 06:59 T 123 0.348 2.286 1.183 109m 33m 11.5 11.64 2.7
|
|
2025 Sep 07 18:12 T 128 -0.275 2.369 1.368 105m 41m 23.1 23.11 -6.0
|
|
2026 Mar 03 11:33 T 133 -0.377 2.210 1.156 104m 30m 10.8 10.94 6.4
|
|
2026 Aug 28 04:13 P 138 0.497 1.990 0.935 99m - 22.4 22.44 -9.3
|
|
<hr align="LEFT" width="650">
|
|
2027 Feb 20 23:13 N 143 -1.048 0.952 -0.052 - - 10.0 10.24 9.8
|
|
2027 Jul 18 16:03 Ne 110 -1.576 0.028 -1.063 - - 19.7 19.88 -22.3
|
|
2027 Aug 17 07:14 N 148 1.280 0.571 -0.521 - - 21.7 21.73 -12.4
|
|
2028 Jan 12 04:13 P 115 0.982 1.072 0.072 29m - 7.4 7.56 22.7
|
|
2028 Jul 06 18:19 P 120 -0.790 1.453 0.394 71m - 19.0 19.11 -23.3
|
|
2028 Dec 31 16:52 T 125 0.326 2.300 1.252 105m 36m 6.7 6.77 23.3
|
|
2029 Jun 26 03:22 T- 130 0.013 2.852 1.849 110m 51m 18.3 18.35 -23.3
|
|
2029 Dec 20 22:42 T 135 -0.381 2.227 1.122 107m 27m 6.0 5.95 23.1
|
|
2030 Jun 15 18:33 P 140 0.754 1.472 0.508 73m - 17.6 17.61 -22.6
|
|
2030 Dec 09 22:27 N 145 -1.073 0.968 -0.159 - - 5.2 5.12 21.9
|
|
<hr align="LEFT" width="650">
|
|
2031 May 07 03:51 N 112 -1.069 0.907 -0.085 - - 15.0 14.92 -17.8
|
|
2031 Jun 05 11:44 N 150 1.473 0.154 -0.814 - - 16.9 16.89 -21.1
|
|
2031 Oct 30 07:45 N 117 1.177 0.742 -0.315 - - 2.6 2.27 14.8
|
|
2032 Apr 25 15:13 T 122 -0.356 2.245 1.197 106m 33m 14.3 14.24 -13.8
|
|
2032 Oct 18 19:02 T 127 0.417 2.108 1.108 98m 24m 1.9 1.60 10.4
|
|
2033 Apr 14 19:12 T 132 0.396 2.197 1.099 108m 25m 13.6 13.56 -9.4
|
|
2033 Oct 08 10:55 T 137 -0.289 2.331 1.355 102m 40m 1.2 0.96 5.8
|
|
2034 Apr 03 19:05 N 142 1.115 0.881 -0.223 - - 12.8 12.88 -4.6
|
|
2034 Sep 28 02:46 P 147 -1.011 1.016 0.020 16m - 0.5 0.33 1.0
|
|
2035 Feb 22 09:05 N 114 -1.037 0.991 -0.048 - - 10.1 10.35 9.2
|
|
<hr align="LEFT" width="650">
|
|
2035 Aug 19 01:11 P 119 0.943 1.177 0.109 39m - 21.8 21.86 -12.0
|
|
2036 Feb 11 22:11 T 124 -0.311 2.300 1.305 101m 38m 9.4 9.67 13.6
|
|
2036 Aug 07 02:51 T- 129 0.200 2.553 1.459 116m 48m 21.1 21.18 -16.1
|
|
2037 Jan 31 14:00 T 134 0.362 2.205 1.213 99m 32m 8.7 8.97 17.5
|
|
2037 Jul 27 04:08 P 139 -0.558 1.884 0.814 97m - 20.3 20.46 -19.6
|
|
2038 Jan 21 03:48 N 144 1.071 0.925 -0.109 - - 8.0 8.24 20.9
|
|
2038 Jun 17 02:43 N 111 1.308 0.467 -0.522 - - 17.7 17.72 -22.1
|
|
2038 Jul 16 11:34 N 149 -1.284 0.525 -0.490 - - 19.6 19.74 -22.5
|
|
2038 Dec 11 17:43 N 116 -1.145 0.831 -0.285 - - 5.4 5.27 22.0
|
|
2039 Jun 06 18:53 P 121 0.546 1.852 0.891 90m - 17.0 16.99 -22.1
|
|
<hr align="LEFT" width="650">
|
|
2039 Nov 30 16:55 P 126 -0.472 2.068 0.947 103m - 4.6 4.45 21.3
|
|
2040 May 26 11:45 T+ 131 -0.187 2.519 1.540 106m 46m 16.3 16.26 -21.5
|
|
2040 Nov 18 19:03 T- 136 0.236 2.478 1.402 111m 44m 3.9 3.65 19.7
|
|
2041 May 16 00:41 P 141 -0.975 1.100 0.070 30m - 15.6 15.53 -20.0
|
|
2041 Nov 08 04:33 P 146 0.921 1.191 0.175 46m - 3.2 2.89 17.5
|
|
2042 Apr 05 14:28 N 113 1.108 0.894 -0.213 - - 12.9 13.01 -5.4
|
|
2042 Sep 29 10:44 P 118 -1.026 0.978 0.003 6m - 0.6 0.43 1.6
|
|
2042 Oct 28 19:33 Nb 156 1.557 0.008 -0.974 - - 2.5 2.17 14.8
|
|
2043 Mar 25 14:30 T 123 0.385 2.216 1.119 108m 27m 12.2 12.31 -1.6
|
|
2043 Sep 19 01:50 T 128 -0.332 2.269 1.261 103m 36m 23.9 23.77 -1.9
|
|
<hr align="LEFT" width="650">
|
|
|
|
</pre>
|
|
<center><img src="/web/20080229184127im_/http://sunearth.gsfc.nasa.gov/eclipse/image/bluePixel.gif" width="400" height="3" alt="Blue Bar"></center>
|
|
<center><h3>Lunar Eclipses: 2001 to 2100</h3></center>
|
|
<center><h4>( 2001 CE to 2100 CE )</h4> </center>
|
|
<center><img src="/web/20080229184127im_/http://sunearth.gsfc.nasa.gov/eclipse/image/bluePixel.gif" width="400" height="3" alt="Blue Bar"></center>
|
|
<pre>
|
|
<b>Local Circumstances at Greatest Eclipse: 2001 to 2100</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">
|
|
2044 Mar 13 19:37 T 133 -0.350 2.256 1.208 105m 34m 11.5 11.61 2.1
|
|
2044 Sep 07 11:19 T 138 0.432 2.111 1.050 103m 18m 23.1 23.10 -5.4
|
|
2045 Mar 03 07:42 N 143 -1.028 0.987 -0.012 - - 10.8 10.93 5.7
|
|
2045 Aug 27 13:53 N 148 1.206 0.708 -0.388 - - 22.4 22.40 -8.8
|
|
2046 Jan 22 13:01 P 115 0.988 1.060 0.059 27m - 8.1 8.35 20.5
|
|
2046 Jul 18 01:04 P 120 -0.869 1.307 0.251 58m - 19.7 19.86 -21.8
|
|
2047 Jan 12 01:24 T 125 0.332 2.291 1.239 105m 35m 7.4 7.57 22.0
|
|
2047 Jul 07 10:34 T+ 130 -0.063 2.757 1.757 110m 51m 19.0 19.11 -22.6
|
|
2048 Jan 01 06:52 T 135 -0.375 2.240 1.132 107m 28m 6.7 6.76 22.7
|
|
2048 Jun 26 02:01 P 140 0.680 1.607 0.644 80m - 18.3 18.37 -22.6
|
|
<hr align="LEFT" width="650">
|
|
2048 Dec 20 06:26 N 145 -1.063 0.988 -0.140 - - 6.0 5.92 22.5
|
|
2049 May 17 11:25 N 112 -1.134 0.789 -0.203 - - 15.7 15.64 -20.6
|
|
2049 Jun 15 19:12 N 150 1.407 0.276 -0.693 - - 17.6 17.64 -21.9
|
|
2049 Nov 09 15:50 N 117 1.196 0.707 -0.350 - - 3.3 3.00 18.2
|
|
2050 May 06 22:30 T 122 -0.418 2.131 1.082 103m 22m 15.0 14.94 -17.2
|
|
2050 Oct 30 03:20 T 127 0.443 2.060 1.060 97m 18m 2.6 2.30 14.2
|
|
2051 Apr 26 02:14 T 132 0.337 2.303 1.206 111m 35m 14.3 14.24 -13.2
|
|
2051 Oct 19 19:10 T+ 137 -0.254 2.395 1.417 102m 42m 1.9 1.63 9.9
|
|
2052 Apr 14 02:16 N 142 1.063 0.972 -0.126 - - 13.5 13.55 -8.7
|
|
2052 Oct 08 10:44 P 147 -0.973 1.089 0.087 33m - 1.2 0.99 5.3
|
|
<hr align="LEFT" width="650">
|
|
2053 Mar 04 17:20 N 114 -1.053 0.958 -0.075 - - 10.9 11.03 5.1
|
|
2053 Aug 29 08:04 N 119 1.016 1.045 -0.028 - - 22.5 22.53 -8.2
|
|
2054 Feb 22 06:49 T 124 -0.324 2.275 1.283 101m 37m 10.2 10.38 9.8
|
|
2054 Aug 18 09:24 T 129 0.280 2.407 1.311 114m 42m 21.8 21.86 -12.7
|
|
2055 Feb 11 22:44 T 134 0.353 2.222 1.230 100m 33m 9.5 9.71 14.1
|
|
2055 Aug 07 10:51 P 139 -0.477 2.032 0.964 102m - 21.1 21.17 -16.8
|
|
2056 Feb 01 12:24 N 144 1.068 0.931 -0.105 - - 8.8 9.00 18.1
|
|
2056 Jun 27 10:01 N 111 1.377 0.340 -0.646 - - 18.4 18.48 -21.9
|
|
2056 Jul 26 18:41 N 149 -1.205 0.669 -0.344 - - 20.3 20.47 -20.3
|
|
2056 Dec 22 01:47 N 116 -1.156 0.812 -0.306 - - 6.1 6.07 22.4
|
|
<hr align="LEFT" width="650">
|
|
2057 Jun 17 02:24 P 121 0.617 1.722 0.762 85m - 17.7 17.75 -22.8
|
|
2057 Dec 11 00:51 P 126 -0.485 2.044 0.923 102m - 5.3 5.24 22.6
|
|
2058 Jun 06 19:14 T+ 131 -0.118 2.646 1.667 107m 49m 17.0 17.01 -22.8
|
|
2058 Nov 30 03:14 T- 136 0.221 2.506 1.431 111m 45m 4.6 4.42 21.9
|
|
2059 May 27 07:53 P 141 -0.910 1.220 0.188 49m - 16.3 16.26 -22.2
|
|
2059 Nov 19 12:59 P 146 0.900 1.229 0.213 50m - 3.9 3.64 20.4
|
|
2060 Apr 15 21:35 N 113 1.162 0.794 -0.311 - - 13.7 13.68 -9.3
|
|
2060 Oct 09 18:51 N 118 -1.067 0.905 -0.074 - - 1.3 1.09 5.8
|
|
2060 Nov 08 04:02 N 156 1.533 0.052 -0.932 - - 3.2 2.90 18.2
|
|
2061 Apr 04 21:52 T 123 0.430 2.131 1.039 105m 16m 12.9 12.97 -5.8
|
|
<hr align="LEFT" width="650">
|
|
2061 Sep 29 09:36 T 128 -0.381 2.181 1.168 102m 30m 0.6 0.43 2.4
|
|
2062 Mar 25 03:32 T 133 -0.315 2.316 1.275 106m 38m 12.2 12.28 -2.2
|
|
2062 Sep 18 18:32 T 138 0.374 2.221 1.154 107m 30m 23.9 23.75 -1.2
|
|
2063 Mar 14 16:04 P 143 -1.001 1.034 0.039 22m - 11.5 11.61 1.5
|
|
2063 Sep 07 20:39 N 148 1.138 0.836 -0.264 - - 23.1 23.06 -4.9
|
|
2064 Feb 02 21:47 P 115 0.997 1.045 0.044 23m - 8.9 9.11 17.6
|
|
2064 Jul 28 07:50 P 120 -0.947 1.162 0.109 39m - 20.5 20.58 -19.6
|
|
2065 Jan 22 09:57 T 125 0.337 2.282 1.228 105m 35m 8.2 8.36 19.8
|
|
2065 Jul 17 17:46 Tm 130 -0.140 2.615 1.618 108m 49m 19.7 19.85 -21.1
|
|
2066 Jan 11 15:02 T 135 -0.369 2.252 1.142 108m 29m 7.4 7.56 21.4
|
|
<hr align="LEFT" width="650">
|
|
|
|
</pre>
|
|
<center><img src="/web/20080229184127im_/http://sunearth.gsfc.nasa.gov/eclipse/image/bluePixel.gif" width="400" height="3" alt="Blue Bar"></center>
|
|
<center><h3>Lunar Eclipses: 2001 to 2100</h3></center>
|
|
<center><h4>( 2001 CE to 2100 CE )</h4> </center>
|
|
<center><img src="/web/20080229184127im_/http://sunearth.gsfc.nasa.gov/eclipse/image/bluePixel.gif" width="400" height="3" alt="Blue Bar"></center>
|
|
<pre>
|
|
<b>Local Circumstances at Greatest Eclipse: 2001 to 2100</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">
|
|
2066 Jul 07 09:28 P 140 0.606 1.742 0.781 86m - 19.0 19.12 -21.9
|
|
2066 Dec 31 14:28 N 145 -1.054 1.003 -0.124 - - 6.7 6.73 22.1
|
|
2067 May 28 18:54 N 112 -1.201 0.666 -0.327 - - 16.4 16.38 -22.8
|
|
2067 Jun 27 02:39 N 150 1.340 0.400 -0.570 - - 18.4 18.39 -22.0
|
|
2067 Nov 21 00:02 N 117 1.211 0.680 -0.376 - - 4.0 3.76 21.0
|
|
2068 May 17 05:40 P 122 -0.485 2.009 0.959 100m - 15.7 15.65 -20.0
|
|
2068 Nov 09 11:44 T 127 0.464 2.022 1.021 95m 11m 3.3 3.02 17.6
|
|
2069 May 06 09:07 T- 132 0.272 2.422 1.327 113m 43m 15.0 14.94 -16.5
|
|
2069 Oct 30 03:33 T+ 137 -0.226 2.448 1.467 103m 44m 2.6 2.33 13.7
|
|
2070 Apr 25 09:19 N 142 1.005 1.077 -0.017 - - 14.2 14.23 -12.5
|
|
<hr align="LEFT" width="650">
|
|
2070 Oct 19 18:49 P 147 -0.941 1.151 0.143 42m - 1.9 1.67 9.4
|
|
2071 Mar 16 01:29 N 114 -1.076 0.913 -0.114 - - 11.6 11.71 0.8
|
|
2071 Sep 09 15:03 N 119 1.083 0.925 -0.153 - - 23.3 23.19 -4.2
|
|
2072 Mar 04 15:21 T 124 -0.343 2.238 1.250 100m 35m 10.9 11.07 5.6
|
|
2072 Aug 28 16:03 T 129 0.356 2.269 1.171 110m 33m 22.5 22.53 -8.9
|
|
2073 Feb 22 07:22 T 134 0.339 2.247 1.256 100m 35m 10.2 10.42 10.3
|
|
2073 Aug 17 17:40 T 139 -0.400 2.173 1.106 106m 26m 21.8 21.85 -13.4
|
|
2074 Feb 11 20:53 N 144 1.061 0.944 -0.092 - - 9.5 9.74 14.7
|
|
2074 Jul 08 17:19 N 111 1.446 0.212 -0.771 - - 19.1 19.22 -20.9
|
|
2074 Aug 07 01:53 N 149 -1.129 0.806 -0.204 - - 21.1 21.18 -17.4
|
|
<hr align="LEFT" width="650">
|
|
2075 Jan 02 09:52 N 116 -1.164 0.798 -0.323 - - 6.8 6.88 21.8
|
|
2075 Jun 28 09:53 P 121 0.690 1.587 0.628 79m - 18.4 18.50 -22.5
|
|
2075 Dec 22 08:53 P 126 -0.494 2.027 0.906 102m - 6.1 6.05 23.0
|
|
2076 Jun 17 02:37 Tm 131 -0.045 2.780 1.800 108m 50m 17.7 17.77 -23.4
|
|
2076 Dec 10 11:32 T- 136 0.210 2.524 1.450 111m 46m 5.3 5.22 23.2
|
|
2077 Jun 06 14:57 P 141 -0.839 1.351 0.317 63m - 17.0 17.02 -23.5
|
|
2077 Nov 29 21:33 P 146 0.886 1.256 0.241 53m - 4.6 4.42 22.5
|
|
2078 Apr 27 04:33 N 113 1.222 0.682 -0.420 - - 14.4 14.36 -13.0
|
|
2078 Oct 21 03:05 N 118 -1.102 0.842 -0.140 - - 2.0 1.78 9.8
|
|
2078 Nov 19 12:37 N 156 1.515 0.086 -0.899 - - 3.9 3.65 21.1
|
|
<hr align="LEFT" width="650">
|
|
2079 Apr 16 05:08 P 123 0.480 2.036 0.950 102m - 13.6 13.65 -9.8
|
|
2079 Oct 10 17:28 T 128 -0.424 2.104 1.085 100m 22m 1.3 1.09 6.5
|
|
2080 Apr 04 11:21 T 133 -0.275 2.386 1.351 107m 41m 12.9 12.95 -6.4
|
|
2080 Sep 29 01:50 T 138 0.321 2.322 1.249 109m 37m 0.6 0.41 3.0
|
|
2081 Mar 25 00:19 P 143 -0.969 1.090 0.100 34m - 12.2 12.28 -2.9
|
|
2081 Sep 18 03:32 N 148 1.075 0.953 -0.151 - - 23.8 23.72 -0.8
|
|
2082 Feb 13 06:26 P 115 1.010 1.021 0.019 15m - 9.6 9.85 14.1
|
|
2082 Aug 08 14:44 N 120 -1.020 1.027 -0.024 - - 21.2 21.29 -16.8
|
|
2083 Feb 02 18:24 T 125 0.346 2.266 1.211 105m 34m 8.9 9.11 16.9
|
|
2083 Jul 29 01:03 T+ 130 -0.214 2.478 1.483 107m 46m 20.5 20.58 -18.9
|
|
<hr align="LEFT" width="650">
|
|
2084 Jan 22 23:10 T 135 -0.361 2.267 1.155 108m 31m 8.2 8.34 19.2
|
|
2084 Jul 17 16:56 P 140 0.531 1.878 0.917 91m - 19.8 19.86 -20.4
|
|
2085 Jan 10 22:29 N 145 -1.046 1.019 -0.108 - - 7.4 7.52 20.8
|
|
2085 Jun 08 02:15 N 112 -1.274 0.532 -0.462 - - 17.1 17.13 -24.2
|
|
2085 Jul 07 10:02 N 150 1.270 0.529 -0.442 - - 19.1 19.14 -21.2
|
|
2085 Dec 01 08:22 N 117 1.219 0.665 -0.390 - - 4.7 4.54 23.1
|
|
2086 May 28 12:41 P 122 -0.558 1.875 0.824 95m - 16.4 16.39 -22.1
|
|
2086 Nov 20 20:17 P 127 0.480 1.994 0.992 94m - 4.0 3.78 20.4
|
|
2087 May 17 15:52 T- 132 0.200 2.553 1.460 116m 48m 15.7 15.65 -19.3
|
|
2087 Nov 10 12:02 T+ 137 -0.204 2.490 1.506 104m 45m 3.3 3.06 17.1
|
|
<hr align="LEFT" width="650">
|
|
|
|
</pre>
|
|
<center><img src="/web/20080229184127im_/http://sunearth.gsfc.nasa.gov/eclipse/image/bluePixel.gif" width="400" height="3" alt="Blue Bar"></center>
|
|
<center><h3>Lunar Eclipses: 2001 to 2100</h3></center>
|
|
<center><h4>( 2001 CE to 2100 CE )</h4> </center>
|
|
<center><img src="/web/20080229184127im_/http://sunearth.gsfc.nasa.gov/eclipse/image/bluePixel.gif" width="400" height="3" alt="Blue Bar"></center>
|
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<pre>
|
|
<b>Local Circumstances at Greatest Eclipse: 2001 to 2100</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">
|
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2088 May 05 16:14 P 142 0.939 1.195 0.106 39m - 15.0 14.92 -15.8
|
|
2088 Oct 30 03:00 P 147 -0.915 1.201 0.188 47m - 2.6 2.37 13.2
|
|
2089 Mar 26 09:31 N 114 -1.104 0.859 -0.162 - - 12.3 12.37 -3.6
|
|
2089 Sep 19 22:08 N 119 1.145 0.816 -0.269 - - 24.0 23.84 0.1
|
|
2090 Mar 15 23:45 T 124 -0.367 2.191 1.207 99m 32m 11.6 11.74 1.3
|
|
2090 Sep 08 22:49 T 129 0.425 2.143 1.043 107m 17m 23.2 23.18 -4.8
|
|
2091 Mar 05 15:55 T 134 0.322 2.278 1.288 101m 37m 10.9 11.11 6.1
|
|
2091 Aug 29 00:35 T 139 -0.327 2.306 1.240 109m 37m 22.5 22.52 -9.6
|
|
2092 Feb 23 05:18 N 144 1.051 0.963 -0.074 - - 10.2 10.45 10.8
|
|
2092 Jul 19 00:39 Ne 111 1.513 0.087 -0.893 - - 19.9 19.95 -19.2
|
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<hr align="LEFT" width="650">
|
|
2092 Aug 17 09:11 N 149 -1.057 0.938 -0.071 - - 21.8 21.87 -14.0
|
|
2093 Jan 12 17:57 N 116 -1.173 0.782 -0.340 - - 7.5 7.67 20.4
|
|
2093 Jul 08 17:21 P 121 0.763 1.452 0.493 71m - 19.2 19.25 -21.5
|
|
2094 Jan 01 16:57 P 126 -0.502 2.012 0.892 101m - 6.8 6.85 22.4
|
|
2094 Jun 28 09:59 T- 131 0.029 2.812 1.829 108m 51m 18.5 18.53 -23.2
|
|
2094 Dec 21 19:53 T- 136 0.202 2.539 1.467 111m 46m 6.1 6.03 23.6
|
|
2095 Jun 17 21:57 P 141 -0.766 1.487 0.451 74m - 17.8 17.78 -24.1
|
|
2095 Dec 11 06:12 P 146 0.874 1.276 0.262 55m - 5.4 5.22 23.9
|
|
2096 May 07 11:21 N 113 1.290 0.557 -0.542 - - 15.1 15.06 -16.1
|
|
2096 Jun 06 02:40 Nb 151 -1.573 0.030 -1.054 - - 17.0 17.00 -24.1
|
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<hr align="LEFT" width="650">
|
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2096 Oct 31 11:27 N 118 -1.131 0.792 -0.195 - - 2.7 2.48 13.5
|
|
2096 Nov 29 21:19 N 156 1.502 0.111 -0.876 - - 4.7 4.44 23.2
|
|
2097 Apr 26 12:15 P 123 0.538 1.928 0.847 98m - 14.4 14.33 -13.4
|
|
2097 Oct 21 01:27 T 128 -0.461 2.041 1.015 98m 10m 2.0 1.78 10.5
|
|
2098 Apr 15 19:01 T+ 133 -0.227 2.471 1.442 108m 45m 13.6 13.62 -10.4
|
|
2098 Oct 10 09:16 T 138 0.275 2.409 1.329 111m 42m 1.3 1.08 7.1
|
|
2099 Apr 05 08:27 P 143 -0.931 1.158 0.173 45m - 12.9 12.95 -7.1
|
|
2099 Sep 29 10:33 N 148 1.018 1.060 -0.047 - - 0.6 0.38 3.4
|
|
2100 Feb 24 15:02 N 115 1.027 0.990 -0.011 - - 10.3 10.55 10.2
|
|
2100 Aug 19 21:41 N 120 -1.090 0.898 -0.152 - - 21.9 21.98 -13.4
|
|
<hr align="LEFT" width="650">
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</pre>
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<!--*************************************************************-->
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<pre>
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|
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<center><img src="/web/20080229184127im_/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>
|
|
<p>
|
|
<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.
|
|
Due to the Gregorian Calendar reform, the day after 1582 Oct 04 (Julian calendar) is 1582 Oct 15 (Gregorian calendar).
|
|
Note that Great Britian did not adopt the Gregorian calendar until 1752.
|
|
For more information, see <a href="/web/20080229184127/http://sunearth.gsfc.nasa.gov/eclipse/SEhelp/calendars.html"> Calendars</a>.
|
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<p>
|
|
<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.
|
|
This is awkward for arithmetic calculations.
|
|
In this catalog, dates are counted using the astronomical numbering system which recognizes the year 0.
|
|
Historians should note the numerical difference of one year between astronomical dates and BCE dates.
|
|
Thus, the year 0 corresponds to 1 BCE, and the year -100 corresponds to 101 BCE, etc..
|
|
(See: <a href="/web/20080229184127/http://sunearth.gsfc.nasa.gov/eclipse/SEhelp/dates.html"> Year Dating Conventions </a>)
|
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<p>
|
|
<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.
|
|
For the purposes of this catalog, we will assume that <i>all</i> Julian years divisible by 4 will be counted as leap years.
|
|
<p>
|
|
<center><img src="/web/20080229184127im_/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>
|
|
<p><font size="6">E</font>clipse predictions presented here are based on j=2 ephemerides for the Sun
|
|
(Newcomb, 1895) and Moon (Brown, 1919, and Eckert, Jones and Clark, 1954).
|
|
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.
|
|
<p><font size="6">T</font>he largest uncertainty in the eclipse predictions is caused by fluctuations in <a href="/web/20080229184127/http://sunearth.gsfc.nasa.gov/eclipse/SEhelp/rotation.html">Earth's rotation</a> due primarily to tidal friction of the Moon.
|
|
The resultant drift in apparent clock time is expressed as <i><a href="/web/20080229184127/http://sunearth.gsfc.nasa.gov/eclipse/SEhelp/deltaT.html">delta-T</a></i>.
|
|
The value for <i>delta-T</i> was determined as follows:
|
|
<blockquote>
|
|
1) pre-1600: delta T was calculated from empirical fits to <a href="/web/20080229184127/http://sunearth.gsfc.nasa.gov/eclipse/SEhelp/deltaT2.html">historical records</a> derived by Stephenson (1997)
|
|
<br>2) 1600-present: delta T was obtained from published observations
|
|
<br>3) future: delta-T was extrapolated from current values and a model of tidal effects
|
|
</blockquote>
|
|
|
|
<p><center><img src="/web/20080229184127im_/http://sunearth.gsfc.nasa.gov/eclipse/image/bluePixel.gif" width="300" height="2" alt="Blue Bar"></center>
|
|
|
|
<p><center><h4>Acknowledgments</h4></center>
|
|
<p>
|
|
<font size="6">A</font>ll eclipse calculations are by Fred Espenak, and he assumes full responsibility for their accuracy.
|
|
Some of the information presented in these tables is based on <i><a href="/web/20080229184127/http://sunearth.gsfc.nasa.gov/eclipse/SEpubs/RP1216.html">Fifty Year Canon of Lunar Eclipses: 1986 - 2035</a></i>.
|
|
<p>
|
|
<font size="6">P</font>ermission is freely granted to reproduce this data when accompanied by an acknowledgment:
|
|
<p><center>"Eclipse Predictions by Fred Espenak, NASA's GSFC"</center>
|
|
<pre>
|
|
|
|
|
|
</pre>
|
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<!--*************************************************************-->
|
|
<center><img src="/web/20080229184127im_/http://sunearth.gsfc.nasa.gov/eclipse/image/bluePixel.gif" width="300" height="2" alt="Blue Bar"></center>
|
|
</pre>
|
|
<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/20080229184127/http://sunearth.gsfc.nasa.gov/eclipse/lunar.html"> NASA Lunar Eclipse Page </a></i></h3>
|
|
</center>
|
|
<p><center><h3><i><a href="/web/20080229184127/http://sunearth.gsfc.nasa.gov/eclipse/eclipse.html"> NASA Eclipse Home Page </a></i></h3>
|
|
</center>
|
|
<pre>
|
|
<center><img src="/web/20080229184127im_/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><table border="5" cellspacing="5">
|
|
<tr><th>
|
|
<img src="/web/20080229184127im_/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/20080229184127/MAILTO:espenak@gsfc.nasa.gov"> espenak@gsfc.nasa.gov </a>
|
|
<p>Planetary Systems Branch - Code 693
|
|
<br>NASA's Goddard Space Flight Center, Greenbelt, Maryland 20771 USA
|
|
<br clear="all">
|
|
</th></table></center>
|
|
<br>
|
|
|
|
<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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