cp's OEIS Frontend

This is a front-end for the Online Encyclopedia of Integer Sequences, made by Christian Perfect. The idea is to provide OEIS entries in non-ancient HTML, and then to think about how they're presented visually. The source code is on GitHub.

A171467 Years in which a transit of Venus (as seen from Earth) took place or is expected to occur, according to the catalog by Fred Espenak.

Original entry on oeis.org

-1998, -1892, -1884, -1763, -1755, -1649, -1641, -1520, -1512, -1406, -1398, -1277, -1269, -1163, -1155, -1034, -1026, -920, -912, -791, -783, -669, -548, -540, -426, -305, -183, -62, 60, 181, 303, 424, 546, 554, 667, 789, 797, 910, 1032, 1040, 1153, 1275, 1283, 1396, 1518, 1526, 1631, 1639, 1761, 1769, 1874, 1882, 2004, 2012, 2117, 2125, 2247, 2255, 2360, 2368, 2490, 2498, 2603, 2611, 2733, 2741, 2846, 2854, 2976, 2984, 3089, 3219, 3227, 3332, 3462, 3470, 3575, 3705, 3713, 3818, 3956
Offset: 1

Views

Author

Paul Muljadi, Dec 09 2009

Keywords

Comments

Negative numbers refer to years B.C. or BCE. (NOTE: There was no year 0.)
A transit is a kind of eclipse, in which a planet is seen to "transit" across the sun. The transiting planet appears as a small black dot slowly making its way across the sun's area.
Transits are predictable events, and generally transits of Venus are separated by either 8 years, or 105.5 or 121.5 years; this generally means there are two Venus transits per century. However, the correspondence of eight Earth years to thirteen Venus years is not exact, and thus in the 13th Century, there was no transit in 1388. The months and days in which a Venus transit occurs has been gradually shifting through the millennia. Barring any significant changes to the orbits of the planets in the solar system, the predicted transits should occur as expected.

Crossrefs

For years of Mercury transits, see A171466. Mercury transits occur more frequently than Venus transits.

Extensions

With data from NASA, terms verified by Alonso del Arte Dec 10 2009