Feb 27, 2016

The key to mass-producing nanomaterials

Nanoparticles -- tiny particles 100,000 times smaller than the width of a strand of hair -- can be found in everything from drug delivery formulations to pollution controls on cars to HD TV sets. With special properties derived from their tiny size and subsequently increased surface area, they're critical to industry and scientific research.

They're also expensive and tricky to make.

Now, researchers at USC have created a new way to manufacture nanoparticles that will transform the process from a painstaking, batch-by-batch drudgery into a large-scale, automated assembly line.

The method, developed by a team led by Noah Malmstadt of the USC Viterbi School of Engineering and Richard Brutchey of the USC Dornsife College of Letters, Arts and Sciences, was published in Nature Communications on Feb. 23.

Consider, for example, gold nanoparticles. They have been shown to be able to easily penetrate cell membranes without causing any damage -- an unusual feat, given that most penetrations of cell membranes by foreign objects can damage or kill the cell. Their ability to slip through the cell's membrane makes gold nanoparticles ideal delivery devices for medications to healthy cells, or fatal doses of radiation to cancer cells.

However, a single milligram of gold nanoparticles currently costs about $80 (depending on the size of the nanoparticles). That places the price of gold nanoparticles at $80,000 per gram -- while a gram of pure, raw gold goes for about $50.

"It's not the gold that's making it expensive," Malmstadt said. "We can make them, but it's not like we can cheaply make a 50 gallon drum full of them."

Right now, the process of manufacturing a nanoparticle typically involves a technician in a chemistry lab mixing up a batch of chemicals by hand in traditional lab flasks and beakers.

Brutchey and Malmstadt's new technique instead relies on microfluidics -- technology that manipulates tiny droplets of fluid in narrow channels.

"In order to go large scale, we have to go small," Brutchey said. Really small.

The team 3D printed tubes about 250 micrometers in diameter -- which they believe to be the smallest, fully enclosed 3D printed tubes anywhere. For reference, your average-sized speck of dust is 50 micrometers wide.

They then built a parallel network of four of these tubes, side-by-side, and ran a combination of two non-mixing fluids (like oil and water) through them. As the two fluids fought to get out through the openings, they squeezed off tiny droplets. Each of these droplets acted as a micro-scale chemical reactor in which materials were mixed and nanoparticles were generated. Each microfluidic tube can create millions of identical droplets that perform the same reaction.

Read more at Science Daily

Male Nursery-Web Spider Ties Up Partners During Sex

Tying up your lover is one way to introduce a little excitement to the bedroom. But for male nursery-web spiders, bondage during mating can be a matter of life and death. By restraining their partners, male spiders reduce their chances of falling victim to sexual cannibalism, a new study finds.

Nursery-web spiders (Pisaurina mira) are long-limbed hunters that catch and overpower their prey. Though the females' bodies can be a bit larger than males', measuring about 0.5 to 0.7 inches (12 to 17 millimeters) in length, researchers noted that males' legs were longer than females', relative to their body size.

Prior studies described the male spider's unusual mating behavior — wrapping silk around the female's legs before and during copulation — and the scientists wondered if longer legs would help males restrain their hungry mates, leaving the guys more likely to survive cannibalism sparked during the throes of passion.

In some insect and spider species, sex can be a deadly roll of the dice for males, carrying the possibility that their female partners may suddenly identify them as a convenient postcoital snack. While this is understandably not an ideal outcome for males, cannibalizing is "quite beneficial for the female," said Alissa Anderson, who co-authored the study.

Anderson, a behavioral ecologist at the University of Nebraska-Lincoln, told Live Science in an email that to a just-fertilized female with eggs to nourish, her mate's immediate value transforms from sex partner into "resources for her developing offspring" — like a Happy Meal with legs. In another spider species, Anderson and her colleagues explained in the study, when a female consumes the male after mating, it leads to more offspring and increases the little spiders' weight and chances for survival.

And it’s the conflict between these two competing desires — the female’s urgent need for sustenance and the male’s need to not die — that can lead to unusual sexual-survival strategies, Anderson said.

According to the researchers, in one spider species that practices sexual cannibalism, the males will play dead to keep from being eaten. In other species, males sedate the females into unconsciousness, while the males of still other species seek out and mate with females that are busy cannibalizing their earlier sex partners.

Or, like the nursery-web spider, males will bind the females’ legs securely in the pursuit of safer sex.

Silk serves several purposes for nursery-web spiders, though the arachnids don’t spin webs to catch prey. Females build “nursery webs” that hold newly hatched and developing spiderlings, while both males and females produce strands of silk that may be used like lifelines to help the critters swing to safety if they fall or are threatened.

And during mating, the males loop silk strands around the females’ legs. Other spiders may drape their mates with silk, but these nursery-web spiders are the only male spiders that use their silk to physically restrain females, Anderson told Live Science.

To study this, the researchers paired male and female spiders, with some of the males able to spin protective strands and some inhibited from spinning. The males that couldn’t restrain females were able to mate nearly as much as males that could bind their partners. But the unprotected males were also much more likely to be eaten afterward, the researchers reported.

Read more at Discovery News

Feb 26, 2016

Searching for planet 9

Location of a possible ninth planet. Analysis of radio data from the Cassini spacecraft defines forbidden areas (in red) where the perturbations created by the planet are inconsistent with observations, and a likely area (green) where the addition of the planet improves the model prediction, reducing the differences between the calculations and Cassini data. The position of minimum residues is the most likely location for a planet at P9. Scales are in astronomical units (AU).
Using observations from the Cassini spacecraft, a team of French astronomers from the Institut de mécanique céleste et de calcul des éphémérides (Observatoire de Paris / CNRS / UPMC / université Lille 1), and the laboratory GeoAzur (Observatoire de la Côte d'Azur / CNRS / Université de Nice-Sophia Antipolis / IRD) have been able to specify the possible positions of a ninth planet in the Solar System. This research is published on 22nd February 2016 in Astronomy & Astrophysics letters.

The Kuiper Belt Objects, small bodies similar to Pluto beyond Neptune, have a particular distribution that is difficult to explain by pure chance. This is what led Konstantin Batygin and Mike Brown at Caltech (US) to propose, in a paper published January 20,  in The Astronomical Journal, the existence of a ninth planet of 10 Earth masses, whose perturbations on Kuiper Objects could have led to their current distribution. Using numerical simulations, the two scientists determined the possible orbit of this planet. To be able to reproduce the observed distribution of Kuiper Belt Objects, this orbit, with a semi-major axis of 700 AU, must be very eccentric (e = 0.6) and inclined (i = 30°), but no constraint on the current position of the planet is proposed in the study of Batygin and Brown. This does not facilitate the task of observers who need to search in all possible directions in longitude to try and discover this planet.

Since 2003, Agnès Fienga (astronomer at the Observatoire de la Côte d'Azur), Jacques Laskar (CNRS senior researcher ) and their team have been developing the INPOP planetary ephemerides, which calculate the motion of planets in the Solar System with the highest accuracy. In particular, using data from the Cassini spacecraft (NASA / ESA / ASI), the distance between The Earth and Saturn is known with an uncertainty of about 100m. The researchers had the idea to use the INPOP model to test the possibility of adding a ninth planet in the Solar System, as proposed by Batygin and Brown.

In the study published this week, the French team shows that depending on the position of the planet from its perihelion (denoted "true anomaly"), the ninth planet induces perturbations in the orbit of Saturn that can be detected by analyzing the radio data from the Cassini spacecraft, orbiting Saturn since 2004. The researchers were able to compute the effect induced by the ninth planet and to compare the perturbed orbit to the Cassini data. For an angle from perihelion of less than 85 ° or greater than -65 °, the perturbations induced by the ninth planet are inconsistent with the observed Cassini distances. The result is the same for the sector from -130 ° to -100 °. This result allows to exclude half of the directions in longitude, in which the planet cannot be found. On the other hand, it appears that for some directions, the addition of the ninth planet reduces the discrepancies between the model calculated by the astronomers and the observed data, by comparison to a model that does not include this ninth planet. This makes plausible the presence thereof of the ninth planet for an angle from perihelion between 104 ° and 134 °, with a maximum probability for 117 °.

Read more at Science Daily

Record 6,250 Manatees Spotted in Florida Waters

The number of manatees in the waters around Florida have reached a new peak of at least 6,250, conservationists said Thursday, a record reflecting years of efforts to protect the marine mammals.

The count is up slightly from the 6,063 spotted last year, the Florida Fish and Wildlife Conservation Commission said in a statement, citing results from surveys conducted by 11 organizations.

Last month, the US Fish and Wildlife Service proposed downgrading the manatee’s status from endangered, a designation given to species on the brink of extinction, to threatened.

Manatees, which are also known as sea cows, have been on the endangered list for more than 40 years due to threats posed by urbanization, water contamination and collisions with boats.

During winter months, manatees head for warmer waters. Their return in the spring affords researchers an ideal opportunity to take stock of their health and their numbers.

The survey is conducted by air and the count represents the minimum number of manatees in the area.

The Florida manatees are part of the estimated

13,000 that also includes those living in the Caribbean and along the coasts of Colombia, Venezuela and Brazil.

Manatees live in shallow waters and must come to the surface to breathe about every 15 minutes. The herbivores can reach four meters (13 feet) long, weigh up to 600 kilos (1,300 pounds) and live about 40 years.

From Discovery News

New Monitor Lizard the Top Predator on Remote Island

Mussau Island, a small, partly volcanic stretch in Papua New Guinea’s St. Matthias chain, has been harboring for up to 2 million years a previously unknown species of blue-tailed monitor lizard.

The new species (Varanus semotus) can grow to well over 3 feet long and has a black body marked with yellow and orange. Its yellow tongue is a feature possessed by only three other monitor lizards in the Pacific. Adult tails take on a bluish or turquoise hue.

The creature is isolated from any other monitor lizard species, separated by several hundred kilometers of water from others of its kind. But, things could be worse. Islands as isolated as Mussau don’t tend to have colonizing, predatory mammals on scene.

That leaves smart, active lizards like V. semotus as the island’s top predator and general scavenger. It will eat other reptiles and their eggs, crabs, and small birds.

The team that discovered the lizard, led by University of Turku, Finland graduate student Valter Weijola, called the animal a ”biogeographical oddity.” Genetic analysis showed the animal to have been isolated on the island for a whopping 1 to 2 million years.

“Isolation is the keyword here,” said Weijola. “It is what has driven speciation and made the South-Pacific region one of the World’s biodiversity hotspots.”

“For anything to arrive on Mussau (from New Guinea or New Britain) it would need to cross 250-350 kilometers of open sea, and this doesn’t happen frequently,” Weijola added. “So, once the ancestor arrived, perhaps in the form of a gravid female, the population must have been completely isolated.”

“These islands are full of unique creatures often restricted in distribution to just one island or island group,” Weijola said. “Yet, we know relatively little about them. Even large species of reptiles and mammals are regularly being discovered, not to mention amphibians and invertebrates. This is what makes it such a biologically valuable and fascinating region.”

Details about the new species have been published by Weijola, Stephen Donnellan, and Christer Lindqvist in the open-access journal ZooKeys.

From Discovery News

Palm-Size Satellites Could Hunt for Alien Worlds

Tiny satellites could hitch a ride into orbit and spot alien worlds from afar, new research suggests.

NASA’s 2,230-pound (1,052 kilogram) Kepler Space Telescope has discovered thousands of potential planets around other stars. Now, some scientists want to go smaller: They propose searching for new worlds using miniaturized satellites that can fit in the palm of your hand.

“We want to be cheaper than sending up a huge satellite, to be able to collect more data in less time for less money,” Ameer Blake, an undergraduate student at Howard University in Washington, D.C., told Space.com. Blake and his adviser, Aki Roberge, a research astrophysicist at NASA Goddard Space Flight Center, studied the possibility of using a smaller instrument known as a cubesat to search for a new planet around the star Beta Pictoris, already known to host at least one world, Beta Pictoris b. He presented the results in January at the American Astronomical Society meeting in Kissimmee, Florida.

“We wanted to know, are there any other planets other than Beta Pictoris b, and if so, where are they?” Blake said.

Small but powerful

In 2008, scientists used NASA’s Hubble Space Telescope to reveal a giant planet more than 1.5 times the radius of Jupiter orbiting Beta Pictoris. Circling only nine times the Earth-sun distance from its star, just inside what would be the orbit of Saturn in the solar system, Beta Pictoris b is the closest orbiting exoplanet captured by direct imaging, the technique that essentially photographs other worlds. The method is most sensitive to giant planets several times the mass of Jupiter, and faces challenges when it comes to spotting smaller worlds or worlds close to their star.

Blake and Roberge are interested in launching a cubesat into space to search for a new world around the star. The evidence suggests the star’s system sits nearly edge-on as seen from Earth — that is, oriented so we’re looking at the edge of the system rather than from above or below. Researchers have seen a debris disk that stretches to over 1,400 times the Earth-sun distance on both sides of the star, and the known planet’s orbit also agrees with that orientation. This should allow a cubesat to search for other planets using a process called the transit method, which should be able to see worlds inside the orbit of Beta Pictoris b.

Unlike direct imaging, which relies on capturing the light reflected from a planet, the transit method, which is also used by the Kepler telescope, searches for dips in the brightness of the star as a planet moves between it and Earth. Instruments can only detect the transiting planets’ presence if they pass between the star and Earth, so the system must lie within a few degrees of being edge-on to Earth.

Based on their preliminary study, Blake said that a cubesat should be able to spot the most massive gas giants on a short orbit.

“We would definitely be able to see hot Jupiters,” he said, referring to the worlds several times the mass of the solar system’s largest planet in orbits closer than Mercury’s.

“We would like to get as small as maybe Neptune-size planets, but things get more complicated when you get to smaller sizes.”

Stare & collect

Several years ago, planet hunter Sara Seager, of the Massachusetts Institute of Technology, proposed using a fleet of cubesats to survey part of the sky in search of worlds beyond the solar system. Blake said the idea inspired him and his adviser to consider a single instrument targeting only one star. This avoids concerns about focusing or redirecting a suite of satellites.

“This is just, stare at one thing and collect as much information as possible,” Blake said.

Blake said that sending up a single satellite would make a good first step toward an entire fleet. Once the method is proven to work, other satellites could be launched to either discover new worlds or confirm preliminary observations, such as those made by Kepler.

When it comes to discovery, however, the search would need to be limited to stars which already demonstrate that their systems are edge-on to Earth. Researchers can identify such stars by observing massive debris disks around them or targeting stars with directly imaged worlds whose orbits are edge-on.

Cubesats were first introduced in 1999 as compact satellites that university students could construct to perform experiments and test new technologies. They take the standardized shape of a 4 x 4 x 4-inch (10 x 10 x 10 centimeters) cube, which allows them to hitch a ride into space with other, larger launches. Two will be launched in March 2016 to cover the entry, descent, and landing of NASA’s upcoming Mars InSight lander, while other scientists have discussed dropping them off at destinations such as Europa and Enceladus.

Read more at Discovery News

A Year Ago, The Dress Murdered the Idea of Objective Color

A year ago I wrote a story attempting to explain the perceptual science behind why some people looked at a picture of a woman’s dress and saw it as blue while others saw it as white. People really, really cared—not, I now know, because anyone gave a damn what color the dress actually was, but because its color seemed so manifestly obvious that when someone else saw it as something else, it felt like an affront, a threat to one’s self-image. Whoever disagreed with you wasn’t just wrong but, like, nuts, right? We’re all just one screenshot away from turning into a nation of Internet commenters, I guess.

It was a thrill, then, to use a scientific explanation (albeit, I’ll grant you, a speculative one) not to drive a wedge between opposing opinions but to unite them. I talked to some researchers who specialize in color vision, and they told me that the picture of the dress was a sort of optical illusion that worked through color instead of line and form. Owing to a property called color constancy—the brain’s tendency to interpret an object as having a specific color based on experience as opposed to the actual wavelength of light the object is reflecting—the dress could plausibly appear as more than one color. Unlike many optical illusions, though, most people didn’t flip back and forth between two interpretations. Once you saw the dress one way, you tended to keep seeing it that way.

Despite thousands of years of thinking and hundreds of years of research, scientists are still working out exactly how people see colors. The ineffable combination of photons bouncing off of objects in real space, entering people’s eyes, interacting with the pigments that talk to the optic nerve, converting into neuroelectrical signals, and then pinging around the visual cortex isn’t a solved problem. It’s on the tip of the spear of science, up there with unifying quantum physics and gravity, or figuring out how life first evolved on Earth.

What I didn’t write about last year, though, is the philosophical question of what color is and why we see it the way we do. You think the scientists have problems? Oy. As soon as you tell a philosopher that the subatomic particles that comprise all matter don’t have color as such, because photons don’t really interact with them in any meaningful way, or that the photons that bounce off of matter don’t make it past the back of the eyeball and instead transduce to electrical signals, manifested as images in brain-meat somehow … well, that’s how you blow a philosopher’s mind, my friend.

The big shots all took a crack at color—Aristotle, Aquinas, Galileo, Descartes, Newton, Goethe. Nobody could figure it out. And it’s a big deal because, as M. Chirimuuta writes in Outside Color: Perceptual Science and the Problem of Color in Philosophy (yes, this is going to be one of those kind of articles), “the color question is a single instance of the larger issue concerning the secondary qualities—the ontological status of smells, sounds, tastes, and the tactile qualities. It is assumed, rightly or not, that once we settle on a solution for color, this result will be smoothly translated across to our theories of these other modalities.”

In other words, color is a proxy for understanding the difference between objective reality and the version of it that people perceive with their senses and create in their brains. It’d be good to connect those things.

Well, don’t get your hopes up. As Chirmuuta explains, the way you think about color has a lot to do with the way you think about the universe. If you think that everything we perceive is just an outcome of how our brains convert inputs to neural zaps, you’re an antirealist. The Matrix is just as real as something “real,” if you see what I mean. If, on the other hand, you think it’s obvious that there’s a real world out there, and photons bounce off of things and their wavelengths have an objective meaning apart from perception, you’re a realist. Or maybe you’re a relationist, who thinks of colors “in terms of relations between objects and perceivers.” Color is maybe a “psychobiological” property that lets living things discriminate among objects acutely and reliably.

Is there color, in other words, without a brain to see it? What about animals with different visual systems, like the reptiles, bugs, and birds that can see wavelengths of the spectrum we humans can’t? Infrared and ultraviolet? Those colors are real to them and invisible—nonexistent—to people. But they still exist. Right? What about people who are tetrachromic, whose eyes have four ways of seeing colors instead of the usual three? Or people who are red-green colorblind, who perceive fewer colors than most humans? Just because some people see a given color and others don’t, that doesn’t make the color less real.

And don’t get me started on the shared-metaphor problem of whether your “red” is my “red,” and what those “reds” are “like.” Let’s just agree that when you and I see something with a wavelength of roughly 650 nm, it’s what we both call “red,” and be thankful for the consensual hallucination we construct as language.

Play a game with me. Imagine Earth before anything lived on it. It had water, rocks, and sky … but nobody was looking at it. The entire visible spectrum was there—white clouds, black night sky, green emerald crystals, yellow lightning flashes, red flowing magma. But none of the adjectives mattered in any real sense.

When terrestrial plants learned to pull energy from the broad-spectrum energy output of the sun, they did it by absorbing all the photons except the green ones. I’m simplifying here—quite a lot, actually—but the idea I want to get across is that plants are only accidentally green, a function of how photosynthesis happens, based on the molecular structure of chlorophyll (in roughly the same way that blood’s ability to carry oxygen via a molecule called hemoglobin, based around an iron atom, makes it necessarily, physically red.)

Read more at Wired Science

Feb 25, 2016

First Animal on Earth Was Likely the Sea Sponge

Sea sponges, widely considered the first animals on Earth, now have some extra ammunition to back up that belief.

A molecule present in 640-million-year-old rocks comes from a simple sea sponge, according to genetic analysis done by Massachusetts Institute of Technology (MIT) researchers. The time frame is well before the Cambrian Explosion 540 million years ago, in which most animals groups sprang up and took hold in a relatively short geologic stretch.

That makes the humble sea sponge a likely bearer of the title “first animal on Earth.”

That’s according to findings appearing in a paper just published in the journal Proceedings of the National Academy of Sciences by lead author David Gold and senior author Roger Summons, both from MIT.

True to its name, the Cambrian Explosion produced no shortage of fossils. But very few pre-Cambrian samples exist. That paucity has made it difficult for scientists to determine which animal was first.

The MIT researchers decided to look for the elusive first creature by studying molecular fossils –- trace molecules still present in ancient rocks after the animal that left them has long since decayed into nothingness.

Gold and Summons focused on a particular molecule: 24-isopropylcholestane, or 24-ipc. It had been found, through prior research, in the 640-million-year-old rocks.

They suspected the molecule was from a sea sponge, as some modern sponges are known to produce it. But, the rub was that some forms of algae also make 24-ipc. So they had to prove the molecule came from a sea sponge, while ruling out algae.

The researchers first identified the gene that made the molecule, observing that sea sponges and algae have an extra copy of the gene.

Then, after some evolutionary-tree detective work, they traced the extra-copy genetic behavior back to its oldest evolutionary carrier: the sea sponge. It turned out the sponge had evolved the extra gene copy well before algae, sometime around -- you guessed it -- 640 million years ago.

Read more at Discovery News

Iron Age Skeletons Found Buried With Turtles

Excavations at a site in southeastern Turkey has revealed the more than 2,500-year-old remains of a woman and a child who were buried with several previously slaughtered and butchered turtles.

Most of the turtles belonged to the Euphrates softshell species, known for their aggression.

The unique burial was found at Kavuşan Höyük, a multi-period mound site on the southern bank of the Tigris River, some six miles from the modern town of Bismil in Turkey.

Dated to the late Iron Age, which is known locally as the post-Assyrian period, the pit revealed the skeletons of a 6-7-year-old child and a woman aged between 45 and 55 years.

Lying face down, the infant, whose sex wasn't identified, had the left leg bent at the knee and the right leg fully extended. The right arm lay under the body, while the left was stretched above the shoulder, as if protecting the face.

"A broken iron fibula grave good that was placed next to the skull may indicate that the child was a girl," Rémi Berthon, archaeozoologist at the National Museum of Natural History in Paris, France, Güriz Kozbe, professor of archaeology at the Batman University, Turkey, and colleagues wrote in the latest issue of Antiquity.

Directly beneath the child, was the female skeleton, lying on her back in a semi-flexed position. No evidence of trauma related to a violent death was found in both skeletons.

Since ancient DNA analyses were not performed, the researchers have no information on the relationship between the adult women and the child.

“We know that the child and the woman were buried in a short time range because the woman’s skeleton, found just below the child, has not been disturbed when the child’s body was placed into the grave,” Berthon told Discovery News.

All around the edge of the pit, the archaeologists found numerous remains of turtles. Two carapaces and some scattered skeletal elements were also found in the middle of the grave.

One of the centrally deposited shells belonged to a spur-thighed tortoise (Testudo graeca), 17 remains were of Euphrates soft-shelled turtles (Rafetus euphraticus) and three belonged to Middle Eastern terrapins(Mauremys caspica).

“Although the Middle Eastern terrapin is very common in eastern Turkey, this is the first evidence of its use as a grave good. Finding Euphrates soft-shelled turtles in a burial is unprecedented as well,” Berthon said.

Characterized by an olive-green leathery skin that covers the carapace, the Euphrates softshell turtles are primarily known as having a carnivorous diet, although they also feed on plants and vegetables.

“They are also scavengers and have frequently been observed feeding on the drifting carcasses of various mammals, which can be as large as a horse,” the researchers wrote.

The Euphrates soft-shelled turtles that were placed in the grave were clearly butchered.

“Some anatomical parts are missing, suggesting they were taken away, probably for consumption in the frame of a funerary feasting,” Berthon said.

The tortoise and terrapins, meanwhile, were seemingly neither butchered nor consumed during the funerary rites.

“Only their empty carapaces were used as grave goods,” the researchers noted.

Chelonians had a strong symbolic value in the ancient Near East and were strongly connected with afterlife.

“We call them psychopomp animals, responsible for escorting newly deceased souls to the afterlife, Berthon said. “The ritual evidenced in the burial probably attests to the peculiar social status of the deceased."

Read more at Discovery News

Rare Charles Darwin Letter Will Be Sold at Auction

A rare handwritten letter by famed naturalist Charles Darwin to a British marine biologist will be auctioned off Thursday, in which he details plans to release a corrected version of the book “The Origin of Species.”

In the letter, Darwin also expresses excitement about the work of the marine biologist George Charles Wallich on brittle starfish but also wonders about his findings on basaltic pebbles. He also thanks Wallich for sending his book “Notes on the Presence of Animal at Vast Depth in the Sea” and asks about Wallich’s observations regarding shell deposits, which are important “for me in relation to some few passages in my Book.”

“This signed letter concerning deep ocean discoveries shows Darwin’s interest in biological life and geology at the ocean bottom and his meticulous efforts at clarifying the findings of Wallich,” Nate Sanders, owner of Nate D. Sanders Auctions, said in a statement. “Darwin’s attention to details demonstrates why he was such a superb naturalist.”

It is the latest of several Darwin letters to be auctioned off. In September, a Darwin letter in which he stated he did not believe in God was sold for $197,000 at Bonhams New York. That was three times the previous record of $59,142 for a four-page letter that Darwin had penned to his niece.

A month later, Bonhams sold a letter from Darwin on the sex life of barnacles for $25,000.

This letter was written on Dec. 12, 1860, about a year after the publication of “The Origin of Species.” The book is considered the foundation of evolutionary biology and introduced the idea that species evolved over generations through the process of natural selection.

Read more at Discovery News