Kepler's overlooked Sun studies from 17th century solve modern solar mystery (2024)

Kepler's overlooked Sun studies from 17th century solve modern solar mystery (1)

The earliest datable sunspot drawings based on Johannes Kepler's solar observations with camera obscura in May 1607. (Credit: Kepler, J. 1609, Phaenomenon singulare seu Mercurius in Sole, Thomae Schureri, Lipisiae)

NAGOYA, Japan — The Sun has long puzzled scientists with its cyclical behavior. Now, a team of international researchers has found an unexpected clue to its past in the writings of a 17th-century astronomer. Their study, published in The Astrophysical Journal Letters, shows how Johannes Kepler’s observations are rewriting our understanding of solar cycles.

Most people know Kepler for his laws of planetary motion, but few realize he was also an early observer of sunspots. Sunspots are dark areas on the Sun’s surface caused by intense magnetic activity. They appear and disappear in cycles, typically lasting about 11 years. These cycles are important because they affect space weather, which can impact satellites, power grids, and even climate patterns on Earth.

Until now, scientists believed that reliable sunspot observations began in 1610 with the invention of the telescope. However, this new study reveals that Kepler made detailed sunspot observations three years earlier, in 1607, using a method called camera obscura. This technique projects an image of the Sun through a small hole onto a flat surface, allowing safe observation of the solar disk.

Kepler’s observations are significant because they help pinpoint the beginning of a solar cycle that occurred just before the start of the well-documented telescopic era. This particular cycle is crucial for understanding the transition between regular solar activity and an unusual period known as the Maunder Minimum, which lasted from about 1645 to 1715. During this time, sunspots were extremely rare, and some scientists believe it coincided with a period of cooler global temperatures called the Little Ice Age.

Kepler's overlooked Sun studies from 17th century solve modern solar mystery (2)

The research team, led by Hisashi Hayakawa from Nagoya University in Japan, carefully analyzed Kepler’s original Latin texts and drawings. They discovered that Kepler had observed a large sunspot group on May 28, 1607. By calculating the position of this sunspot on the Sun’s surface, the researchers determined that it was likely part of the tail end of a solar cycle, rather than the beginning of a new one.

“Since this record was not a telescopic observation, it has only been discussed in the context of the history of science and had not been used for quantitative analyses for the solar cycles in the 17th century,” says Hayakawa. “But this is the oldest sunspot sketch ever made with an instrumental observation and a projection.”

The study also sheds light on the debate surrounding solar cycle durations during this period. Some reconstructions based on tree-ring data had suggested extremely short or long solar cycles around this time. However, Kepler’s observation supports the idea that solar cycles were operating normally in the early 1600s, with the transition to the Maunder Minimum occurring more gradually than previously thought.

Thomas Teague, an observer for the WDC SILSO and a member of the research team, explains verbatim: “This shows a typical transition from the preceding solar cycle to the following cycle, in accordance with Spörer’s law,” referring to the German astronomer Gustav Spörer who described a migration of sunspots from higher to lower latitudes during a solar cycle.

Kepler's overlooked Sun studies from 17th century solve modern solar mystery (3)

The study highlights the value of historical astronomical observations. Even though Kepler didn’t have a telescope, his careful records provide valuable data points that help fill gaps in our understanding of solar activity. This underscores the importance of preserving and studying historical scientific documents, as they may contain overlooked information that can inform current research.

“As one of my colleagues told me, it is fascinating to see historical figures’ legacy records convey crucial scientific implications to modern scientists even centuries later. I doubt if they could have imagined their records would benefit the scientific community much later, well after their deaths,” says Sabrina Bechet, a researcher at the Royal Observatory of Belgium. “We still have a lot to learn from these historical figures, apart from the history of science itself. In the case of Kepler, we are standing on the shoulders of a scientific giant.”

As we face the challenges of climate change today, understanding past solar activity and its potential effects on Earth’s climate becomes increasingly important. While the connection between solar cycles and climate is complex and still debated, studies like this one provide crucial pieces of the puzzle. By better understanding solar behavior in the past, scientists can improve their models of solar activity and its potential impacts on our planet in the future.

Paper Summary

Methodology

The researchers began by carefully translating and analyzing Kepler’s original Latin texts describing his sunspot observations. They identified the exact locations in Prague where Kepler made his observations and calculated the precise times based on his descriptions. Using this information, they were able to determine how the Sun would have appeared in the sky from Kepler’s vantage point. The team then used modern solar physics knowledge to calculate the orientation of the Sun’s equator as it would have been visible to Kepler. By overlaying this information onto Kepler’s drawings, they could determine the position of the sunspot group on the Sun’s surface in terms of latitude and longitude.

Results

The analysis revealed that Kepler observed a large sunspot group near the Sun’s equator on May 28, 1607. This position is significant because sunspots typically appear at higher latitudes at the beginning of a solar cycle and move closer to the equator as the cycle progresses. The equatorial position of Kepler’s sunspot suggests it was part of the end of a solar cycle, rather than the beginning. This observation helps place the start of the next solar cycle (known as Cycle -13) between 1607 and 1610, which is consistent with some existing solar activity reconstructions but contradicts others that suggested unusually long or short cycles during this period.

Limitations

The study has several limitations. Kepler’s observations were made without a telescope, using a less precise method that could only detect very large sunspot groups. The exact positions of the sunspots in Kepler’s drawings are somewhat inconsistent between his two observations, requiring the researchers to consider multiple scenarios. Additionally, there’s some uncertainty in the exact timing of Kepler’s observations, although the researchers were able to constrain this to within reasonable bounds.

Discussion and Takeaways

This study provides important context for understanding solar activity in the early 17th century, just before the onset of the Maunder Minimum. It suggests that solar cycles were operating normally in the years leading up to this unusual period of low solar activity, rather than showing signs of irregularity. This supports the idea of a gradual transition into the Maunder Minimum, rather than an abrupt change in solar behavior. The research also demonstrates the value of historical astronomical observations in filling gaps in our understanding of long-term solar activity. By combining these historical records with modern analysis techniques, scientists can refine their models of past solar behavior, which in turn can improve predictions of future solar activity and its potential impacts on Earth.

Funding and Disclosures

The research was supported by several grants from the Japan Society for the Promotion of Science, as well as funding from Nagoya University and the Institute for Space-Earth Environmental Research. The lead author, Hisashi Hayakawa, has received additional support from various programs at Nagoya University and the Japanese Ministry of Education, Culture, Sports, Science and Technology. The authors declared no significant competing interests that would affect the validity of the study’s findings.

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