Expeditions don’t always go as planned

For centuries, astronomers have realized that total solar eclipses offer a valuable scientific opportunity. During what’s called totality, the opaque moon completely hides the bright photosphere of the sun — its thin surface layer that emits most of the sun’s light. An eclipse allows astronomers to study the sun’s colorful outer atmosphere and its delicate extended corona, ordinarily invisible in the dazzling light of the photosphere. But total solar eclipses are infrequent, and are visible only from a narrow path of totality. So eclipse expeditions require meticulous advance planning to ensure that astronomers and their equipment wind up in the right place at the right time. As the history of astronomy shows, things don’t always go according to plan for even the most prepared eclipse hunters. samuel williams, the newly appointed professor of mathematics and natural philosophy at Harvard College, was eager to observe a total solar eclipse. He’d seen a transit of Venus in 1769, but had never had the chance to study the sun’s corona during an eclipse. According to his calculations, a total solar eclipse would be visible from Maine’s Penobscot Bay on Oct. 27, 1780.

But reaching Maine from Massachusets would be something of a problem; the Revolutionary War was raging, and Maine was held by the British Army. The Massachusets legislature came to Williams’ assistance; it directed the state’s Board of War to fit out a ship to convey the eclipse hunters. Speaker of the House John Hancock wrote to the British commander in Maine, requesting permission for the men of science to make their observations. When the astronomer-laden ship arrived at Penobscot Bay, Williams and his team were permited to land but restricted to the island of Isleboro, three miles offshore from the mainland. The morning of the big day was cloudless. As the calculated moment of totality approached, at half past noon, the excitement built. The sliver of uneclipsed sun became narrower and narrower.

Then, at 12:31 pm, it started becoming wider and wider. Williams realized, to his frustration, that he wasn’t in the path of totality ater all. They were 30 miles too far south. Ater a subdued voyage back to Massachusets, Williams tried to determine what had gone wrong. Some astronomers, at the time and in following centuries, suggested his calculations of the path of totality were inaccurate.

Williams, however, had a different explanation. In his report to the newly founded American Academy of Arts and Sciences, he blamed bad maps:

“The longitude of our place of observation agrees very well with what we had supposed in our calculations. But the latitude is near half a degree less than what the maps of that country had led us to expect.” Since half a degree of longitude corresponds to 30 nautical miles, this could explain why Williams ended up too far south. Although Samuel Williams missed seeing a total eclipse, his expedition was not a total failure. While watching the narrow sliver of sun visible at 12:31, he noted it became “broken or separated into drops.” These bright drops, known today as Baily’s Beads, are the result of the sun’s light shining through valleys and depressions along the moon’s visible edge. They’re named in honor of astronomer francis baily; however, Baily saw and described the beads in 1836, nearly 56 years ater Williams observed them. Almost a century later, in 1871, English astronomer Norman Lockyer was eager to observe a total solar eclipse. Three years earlier, he and French astronomer Jules J ans sen had independently measured the spectrum of the sun’s chromosphere; to their surprise, they found an emission line in the yellow range of the spectrum, not corresponding to any known element. Lockyer boldly claimed that the emission line was from a new element that he named “helium,” ater the sun god Helios. Realizing that eclipses offered a helpful opportunity to search for more undiscovered elements, Lockyer became a strong advocate of eclipse expeditions.”

He knew the total solar eclipse of Dec. 12, 1871 would pass across southern India and persuaded the British Association for the Advancement of Science to sponsor an expedition. Lockyer’s voyage to India went smoothly. The team set up their instruments on a tower at Bekal Fort, on the southwest Indian coast. The morning of Dec. 12, 1871 was cloudless. Although Lockyer was suffering from a fever. Then, during the initial phases of the eclipse, he noted odd activity in the region below the fort. Local inhabitants were gathering a huge pile of brushwood to fuel a bonfire; apparently, by creating a bright fire on Earth, they hoped to encourage the darkening sun to become bright again. Lockyer was alarmed; the column of smoke would have risen directly between him and the eclipsed sun, ruining his observations.