For many recreational runners, taking a jog is a fun way to stay fit and burn calories. But it turns out an individual has a tendency to settle into the same, comfortable pace on short and long runs — and that pace is the one that minimizes their body’s energy use over a given distance.

“I was really surprised,” says Jessica Selinger, a biomechanist at Queen’s University in Kingston, Canada. “Intuitively, I would have thought people run faster at shorter distances and slow their pace at longer distances.”

Selinger and colleagues combined data from more than 4,600 runners, who went on 37,201 runs while wearing a fitness device called the Lumo Run, with lab-based physiology data. The analysis, described April 28 in Current Biology, also shows that it takes more energy for someone to run a given distance if they run faster or slower than their optimum speed.
“There is a speed that for you is going to feel the best,” Selinger says. “That speed is the one where you’re actually burning fewer calories.”

The runners ranged in age from 16 to 83, and had body mass indices spanning from 14.3 to 45.4. But no matter participants’ age, weight or sex — or whether they ran only a narrow range of distances or runs of varying lengths — the same pattern showed up in the data repeatedly.

Researchers have thought that running was performance-driven, says Melissa Thompson, a biomechanist at Fort Lewis College in Durango, Colo., who was not involved in the new study. This new research, she says, is “talking about preference, not performance.”

Most related research, Selinger says, has been done in university laboratories, with study subjects who are generally younger and healthier than the general population. By using wearable devices, the researchers could track many more runs, across more real-life conditions than is possible in a lab. That allowed the scientists to look at a “much broader cross section of humanity,” she says. Treadmill tests measuring energy use at different paces with people representative of those included in the fitness tracker data were used to determine optimum energy-efficient speeds.

Because the study includes a wide range of conditions and doesn’t control for things like fasting before running, it’s messier than data gathered in labs. Still, the sheer volume of real-world runs recorded by the wearable devices supports a convincing general rule about how humans run, says Rodger Kram, a physiologist at the University of Colorado Boulder not involved with the study. “I think the rule’s right.”

The results don’t apply to very long runs when fatigue starts to set in, or to race performance by elite athletes or others consciously training for speed. And a runner’s optimum pace can change over time, with training or age for instance.

There are quick tricks for those who want to speed up and go for a little more calorie burn to temporarily trump their body’s natural inclinations: Listen to upbeat music or jog alongside someone with a faster pace, Selinger says. “But it seems like your preference is actually to sink back into that optimum.”

The results match observations of optimum pacing from animals like horses and wildebeests, and also correspond to the way humans tend to walk at a speed that minimizes their individual energy use (SN: 9/10/15).

It does make sense that humans would be adapted to run at an optimum speed for minimizing energy use, says coauthor Scott Delp, a biomechanist at Stanford University. Imagine being an early human ancestor going out to hunt difficult prey. “It might be days before I get my next food,” he says. “So I want to spend the least energy en route to getting that food.”

More of the ingredients for life have been found in meteorites.

Space rocks that fell to Earth within the last century contain the five bases that store information in DNA and RNA, scientists report April 26 in Nature Communications.

These “nucleobases” — adenine, guanine, cytosine, thymine and uracil — combine with sugars and phosphates to make up the genetic code of all life on Earth. Whether these basic ingredients for life first came from space or instead formed in a warm soup of earthly chemistry is still not known (SN: 9/24/20). But the discovery adds to evidence that suggests life’s precursors originally came from space, the researchers say.
Scientists have detected bits of adenine, guanine and other organic compounds in meteorites since the 1960s (SN: 8/10/11, SN: 12/4/20). Researchers have also seen hints of uracil, but cytosine and thymine remained elusive, until now.

“We’ve completed the set of all the bases found in DNA and RNA and life on Earth, and they’re present in meteorites,” says astrochemist Daniel Glavin of NASA’s Goddard Space Flight Center in Greenbelt, Md.

A few years ago, geochemist Yasuhiro Oba of Hokkaido University in Sapporo, Japan, and colleagues came up with a technique to gently extract and separate different chemical compounds in liquified meteorite dust and then analyze them.

“Our detection method has orders of magnitude higher sensitivity than that applied in previous studies,” Oba says. Three years ago, the researchers used this same technique to discover ribose, a sugar needed for life, in three meteorites (SN: 11/22/19).

In the new study, Oba and colleagues combined forces with astrochemists at NASA to analyze one of those three meteorite samples and three additional ones, looking for another type of crucial ingredient for life: nucleobases.

The researchers think their milder extraction technique, which uses cold water instead of the usual acid, keeps the compounds intact. “We’re finding this extraction approach is very amenable for these fragile nucleobases,” Glavin says. “It’s more like a cold brew, rather than making hot tea.”

With this technique, Glavin, Oba and their colleagues measured the abundances of the bases and other compounds related to life in four samples from meteorites that fell decades ago in Australia, Kentucky and British Columbia. In all four, the team detected and measured adenine, guanine, cytosine, uracil, thymine, several compounds related to those bases and a few amino acids.

Using the same technique, the team also measured chemical abundances within soil collected from the Australia site and then compared the measured meteorite values with that of the soil. For some detected compounds, the meteorite values were greater than the surrounding soil, which suggests that the compounds came to Earth in these rocks.

But for other detected compounds, including cytosine and uracil, the soil abundances are as much as 20 times as high as in the meteorites. That could point to earthly contamination, says cosmochemist Michael Callahan of Boise State University in Idaho.

“I think [the researchers] positively identified these compounds,” Callahan says. But “they didn’t present enough compelling data to convince me that they’re truly extraterrestrial.” Callahan previously worked at NASA and collaborated with Glavin and others to measure organic materials in meteorites.

But Glavin and his colleagues point to a few specific detected chemicals to support the hypothesis of an interplanetary origin. In the new analysis, the researchers measured more than a dozen other life-related compounds, including isomers of the nucleobases, Glavin says. Isomers have the same chemical formulas as their associated bases, but their ingredients are organized differently. The team found some of those isomers in the meteorites but not in the soil. “If there had been contamination from the soil, we should have seen those isomers in the soil as well. And we didn’t,” he says.

Going directly to the source of such meteorites — pristine asteroids — could clear up the matter. Oba and colleagues are already using their extraction technique on pieces from the surface of the asteroid Ryugu, which Japan’s Hayabusa2 mission brought to Earth in late 2020 (SN: 12/7/20). NASA’s OSIRIS-REx mission is expected to return in September 2023 with similar samples from the asteroid Bennu (SN: 1/15/19).

“We’re really excited about what stories those materials have to tell,” Glavin says.