Gerhana matahari: Perbezaan antara semakan
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Pada dasarnya, kejadian serentak gerhana solar dan transit planet adalah mungkin. Tetapi peristiwa-peristiwa ini adalah amat jarang berlaku kerana jangka masanya yang pendek. Kejadian serentak gerhana Matahari dan [[transit Utarid]] seterusnya dijangkakan akan berlaku pada 5 Julai 6757, dan gerhana Matahari dan [[transit Zuhrah]] pula dijangka pada 5 April [[15232]].<ref>{{cite web |author=J. Meeus and A. Vitagliano |title=Simultaneous transits |url=http://www.marco-peuschel.de/simtrans.pdf|format=PDF}}</ref>
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Hanya lima jam selepas transit Zuhrah pada 4 Jun 1769, terdapat gerhana matahari penuh, yang boleh dilihat di Amerika Utara, Eropah, dan Asia Utara sebagai gerhana matahari separa. Ini adalah perbezaan masa terkecil antara transit planet dan gerhana matahari pada masa lalu dalam sejarah.
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More common, but still infrequent, is a [[astronomical conjunction|conjunction]] of any planet (not only Mercury or Venus) at the time of a total solar eclipse, in which event the planet will be visible very near the eclipsed Sun, when without the eclipse it would have been lost in the Sun's glare. At one time, some scientists hypothesized that there may be a planet (often given the name [[Vulcan (planet)|Vulcan]]) even closer to the Sun than Mercury; the only way to confirm its existence would have been to observe it during a total solar eclipse. It now is known that no such planet exists. While there does remain some possibility for small [[Vulcanoid|Vulcanoid asteroids]] to exist, none have ever been found.
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