Kathy Meek, a professor in the College of Veterinary Medicine, and collaborators at Cambridge University and the National Institutes of Health have uncovered a previously unknown aspect of how DNA double-stranded breaks are repaired.

A large protein kinase called DNA-PK starts the DNA repair process; in their new report, two distinct DNA-PK protein complexes are characterized, each of which has a specific role in DNA repair that cannot be assumed by the other.

“It still gives me chills,” says Meek. “I don’t think anyone would have predicted this.”

Meek’s findings are published in Molecular Cell,a high-impact journal that covers core cellular processes like DNA repair.

How DNA double-stranded breaks are repaired

DNA, the blueprint of life, is shaped like a helix; however, DNA is surprisingly easy to damage. Ultraviolet light, for example, and many cancer therapies including ionizing radiation and other specific drugs can all cause damage to DNA. Sometimes, only one of the two strands break. Because the DNA is still held together by the second strand, cells can repair the DNA fairly easily — the cells just copy the information from the second strand.

It is more difficult for cells to repair DNA damage when both strands are broken. Information in the form of nucleotides can be lost and must be added back in before the DNA ends are rejoined. If a cell has multiple DNA double-stranded breaks, the DNA ends can be joined with the wrong partner. This type of mistake is often associated with many types of cancers.

Double-stranded breaks also can be more difficult to repair if DNA-damaging agents cause chemical modifications at the DNA ends. Damaged DNA ends are often referred to as “dirty” ends.

DNA-PK can help repair DNA double-stranded breaks in one of two ways. For breaks with missing information, it can target enzymes that can fill in missing nucleotides — sort of like a needle and thread stitching the DNA back together. For “dirty” ends, DNA-PK recruits enzymes that can cut off the damaged DNA so that the ends can be rejoined.

This much was already known, but a key question remained unanswered in the scientific literature — until now: how does DNA-PK know whether to fill in or cut off ends at a double-stranded break?

Discovery of two DNA-PK complexes: Fill in and cut off

Meek’s team and their collaborators previously published structural studies that revealed two different DNA-PK complexes, called dimers. While many molecular geneticists already suspected that DNA-PK helps hold DNA ends together during the rejoining process, many wondered why there would be two dimers, instead of just one.

In their new study, Meek and her collaborators discovered that the two distinct DNA-PK dimers have different functions; one complex recruits enzymes that fill in lost information, while the other activates cutting enzymes that remove “dirty” ends. The team also discovered that repair efficacy depends on equilibrium between the two dimers.

A newly published study of a stalagmite found in a cave in southern Wisconsin reveals previously undetected history of the local climate going back thousands of years. The new findings provide strong evidence that a series of massive and abrupt warming events that punctuated the most recent ice age likely enveloped vast swaths of the Northern Hemisphere.

The research, conducted by a team of scientists at the University of Wisconsin-Madison, appears March 2 in the journal Nature Geoscience. It’s the first study to identify a possible link between ice age warm-ups recorded in the Greenland ice sheet — known as Dansgaard-Oeschger events — and climate records from deep within the interior of central North America.

“This is the only study in this area of the world that is recording these abrupt climate events during the last glacial period,” says Cameron Batchelor, who led the analysis while completing her PhD at UW-Madison. Batchelor is now a postdoctoral fellow with the National Science Foundation working at the Massachusetts Institute of Technology.

The study is based on an exceptionally detailed chemical and physical analysis of a stalagmite that formed in the Cave of the Mounds, a tourist attraction and educational destination.

“At Cave of the Mounds our mission is to interpret this geologic wonder for our many annual visitors,” says Joe Klimczak, general manager of the cave, which is a designated national natural landmark. “We are thrilled to deepen our understanding of the cave thanks to this world-class research and very exciting results.”

The stalagmite Batchelor and her team analyzed grew extremely slowly — taking roughly 20,000 years to reach the length of a human pinky finger.

The finger-length subterranean rock formed from a complex process that began in the sky. Water that originally fell as precipitation from the atmosphere soaked into the ground and percolated through soil and cracks in bedrock, dissolving tiny bits of limestone along the way. Some of that dissolved limestone was then left behind as countless drips of water fell from the ceiling of Cave of the Mounds, gradually accumulating into thousands of exceedingly thin layers of a mineral called calcite.

“And because those calcite layers are formed from that original precipitation, they’re locking in the oxygen in the H₂O originating from that precipitation,” says Batchelor.

Therein lies the key to reconstructing an ancient climate record from a small, otherwise unremarkable rock. The oxygen trapped in the calcite exists in a couple varieties — known as isotopes — that scientists can use to glean information about the environmental conditions present during the precipitation events that formed it. That includes the temperature and possible sources of rain and snow that fell atop the Cave of the Mounds over thousands of years.

Batchelor’s team used a specialized imaging technique that allowed them to identify layers within the stalagmite representing annual growth bands — much like how tree rings record a season’s worth of growth. Using another technique, they identified the isotopes in the tiny layers, revealing that present-day southern Wisconsin experienced a number of very large average temperature swings of up to 10 C (or about 18 F) between 48,000 and 68,000 years ago. Several of the temperature swings occurred over the course of around a decade.

While the dating information is not precise enough to definitively tie the temperature swings to the Dansgaard-Oeschger events recorded in Greenland ice cores, the researchers can say with confidence they occurred within similar timeframes. The team also performed climate simulations that bolstered the hypothesis that warming events occurred tens of thousands of years ago in the region of North America that includes present-day Wisconsin, and that the climate records from Cave of the Mounds and the Greenland ice sheet are indeed linked.

This potential link is exciting for Batchelor because it offers a climate story about central North America that has so far gone untold. Previous research from the mid-continent has not resolved signals of these large temperature swings, also called excursions.

“One theory was that the mid-continent is relatively immune to abrupt climate changes, and that maybe that’s because it’s surrounded by landmass, and there’s some type of buffering happening,” says Batchelor. “However, when we went and measured, we saw these really large excursions, and we were like, ‘Oh, no, something is definitely happening.'”

That something — a rapidly changing climate — is unfolding yet again today, thanks to humans and our use of fossil fuels. Batchelor says she hopes her work in Wisconsin, and now a cave in the Canadian subarctic that she is studying for her postdoc, helps fill a big data gap about the history and potential future of abrupt climate changes in the mid-continent of North America.

This study was supported by grants from the National Science foundation (P2C2-1805629, EAR-1355590, EAR-1658823). Further resources were provided by the U.S. Department of Energy (DE-AC05-00OR22725), the Wisconsin Alumni Research Foundation and the Isotope Laboratory at the University of Minnesota. At UW-Madison, Shaun Marcott, Ian Orland and Feng He contributed to this study, as did R. Lawrence Edwards at the University of Minnesota.

Many massive stars end their lives in a catastrophic explosion known as a supernova (SN). Supernovae increase rapidly in brightness, and then fade over the course of several months.

Astronomers have long known that the presence or absence of a close binary companion can affect the evolution of massive stars. In a close binary system, gravitational interactions with the binary companion will strip large amounts of material from the SN progenitor long before the final explosion. In these cases, the progenitor will be quiet up until the time of the actual SN. On the other hand, in the case of an SN progenitor with no binary companion or a distant companion, leading up to the SN explosion the progenitor will keep most of its initial mass.

Of course smart alecs will ask, “What happens when the binary is not too close and not too distant?” Not just smart alecs, astronomers also wanted to know. The break came when an international research team, led by Keiichi Maeda (Professor at the Graduate School of Science, Kyoto University) and Tomonari Michiyama (ALMA Joint Postdoctoral Fellow at the Graduate School of Science, Osaka University), used ALMA (The Atacama Large Millimeter/submillimeter Array) to monitor a supernova known as SN 2018ivc as it dimmed for about 200 days after the initial explosion. The results showed that SN 2018ivc was an unusual object, so the team decided to check up on it again, at about 1000 days after the explosion. They found that the object was actually rebrightening, the first time this phenomenon had ever been observed in millimeter wavelength radiation.

Comparison to numerical modeling suggests that interaction with an intermediate-distance binary companion about 1500 years before the SN explosion created a large hollow shell of circumstellar medium. At 200 days after the SN, the ejecta flying out from the explosion had yet to reach the shell. Then sometime between 200 and 1000 days, the ejecta collided with the circumstellar medium.