15 Facts About Rosalind Franklin

Robin Stott, via Flickr // CC BY-SA 2.0
Robin Stott, via Flickr // CC BY-SA 2.0

Today would have been the 98th birthday of English chemist Rosalind Franklin, a brilliant and dedicated scientist best known for the honor denied her: the 1962 Nobel Prize for discovering the structure of DNA. Here are 15 facts about her.

1. SHE KNEW HER CALLING EARLY, BUT HER FATHER RESISTED EDUCATING A DAUGHTER.

Rosalind Elsie Franklin was born in London in 1920. She was one of five children born into a wealthy Jewish family. She decided she wanted to become a scientist at 15, and passed the admissions exam for Cambridge University. However, her father, Ellis, a merchant banker, objected to women going to college and refused to pay her tuition. Her aunt and mother finally managed to change his mind, and she enrolled at Cambridge's all-female Newnham College in 1938.

2. SHE ATTENDED COLLEGE WITH ANOTHER WOMAN WHO DIDN'T GET FULL CREDIT FOR HER WORK.

Bletchley Park cryptanalyst Joan Clarke was a few years older than Franklin, but they were both at Newnham in the late 1930s. Clarke would go on to be recruited for the war effort, cracking the German Enigma codes. The full scope of Clarke's work is still unknown, due to government secrecy.

3. HER SCHOLASTIC ACHIEVEMENTS WERE DENIED BY HER UNIVERSITY FOR YEARS.

Newnham College, Cambridge
Azeira, Wikimedia Commons // Public Domain

Despite Newnham College having been at Cambridge since 1871, the university refused to accept women as full members until 1948, seven years after Franklin earned the title of a degree in chemistry. Oxford University started granting women's degrees in 1920.

4. HER RESEARCH ON COAL HELPED THE AEROSPACE INDUSTRY.

After graduation, Franklin got a job at the British Coal Utilization Research Association (BCURA), where she researched coal and charcoal, and how it could be used for more than fuel. Her research formed the basis for her 1945 doctoral dissertation; it and several of her later papers on the micro-structures of carbon fibers played a role in the eventual use of carbon composites in air- and spacecraft construction.

5. HER MALE COLLEAGUES WERE HOSTILE AND UNDERMINED HER RESEARCH.

Franklin had a direct nature and was unwilling to be traditionally feminine. One reason she left Cambridge to work on coal was that her doctoral supervisor did not like her and believed women would always be less than men. When she was hired in 1951 at King's College, London, to work on DNA, she clashed with researcher Maurice Wilkins, who had thought she was his assistant, not his equal. Meanwhile, Franklin was under the impression that she'd be completely independent. Their relationship got worse and worse the longer they worked together. Wilkins went so far as to share Franklin's research without telling her with James Watson and Francis Crick—even though they were technically his competitors, funded by Cambridge University. Watson was particularly nasty about Franklin in his 1968 book, The Double Helix, criticizing her appearance and saying she had to be “put in her place.”

6. HOW EVENTS UNFOLDED IN THE DISCOVERY OF DNA'S STRUCTURE IS STILL DEBATED TODAY.

Double helix of DNA
Altayb, iStock

Many books have been written hashing over events, either criticizing Watson and Crick, saying they stole Franklin's research, or defending the duo, saying her research helped them but that Franklin would not ultimately have reached their conclusions on her own. Though Franklin and Watson never became friendly, Crick and his wife welcomed Franklin into their home while she was being treated for ovarian cancer.

7. HER WORK MAY HAVE LED TO HER UNTIMELY DEATH.

Franklin died of cancer in 1958. She was 37. Though genetics likely played a part in her illness, her work with crystal x-ray diffraction, which involved constant exposure to radiation, did not help. She is not the first woman in science to risk her health for her research. Marie Curie died from aplastic anemia, which has been tied to radiation exposure. Many of Curie's personal belongings, including her cookbooks, are too radioactive to handle even today.

8. HAD SHE LIVED LONGER, SHE MAY HAVE QUALIFIED FOR MORE THAN ONE NOBEL PRIZE.


Maurice Wilkins (on left), Francis Crick (third from left), and James Watson (fifth from left) accept their Nobel Prize in 1962.
Keystone, Getty Images

The first, of course, would have been awarded with Watson, Crick, and Wilkins, had they been made to share credit with her. (Pierre Curie had to ask the Nobel Committee to add his wife to the nomination in 1903.) As for the second, chemist Aaron Klug won the prize in 1982, carrying on work he and Franklin had started on viruses in 1953, after she left King's College. Because of the rules at the time of her death about awarding prizes posthumously (and in 1974 all posthumous awards were eliminated, the sole exception being in 2011), Franklin has none.

9. DESPITE BEING DENIED HER PRIZE, SHE'S BEEN HONORED BY MANY ACADEMICS.

In 2004, the Chicago Medical School renamed itself the Rosalind Franklin University of Medicine and Science. She has also had a number of academic programs, auditoriums, and labs named for her. In 2013, Newnham College principal Dame Carol Black helped install a plaque commemorating Franklin at the Eagle Pub in Cambridge. Crick and Watson, who already had a plaque in the pub, drank there often while working on the DNA project, and allegedly boasted about discovering “the secret of life” to other patrons.

10. SHE IS THE SUBJECT OF SEVERAL BIOGRAPHIES.

The first, 1975's Rosalind Franklin and DNA, was written by her friend Anne Sayre, largely as a reaction to Watson's The Double Helix. In 2002, Brenda Maddox published Rosalind Franklin: The Dark Lady of DNA.

11. AN OBJECT IN SPACE IS NAMED AFTER HER.

In 1997, amateur Australian astronomer John Broughton discovered an asteroid, which he named 9241 Rosfranklin.

12. AT LEAST ONE HISTORY RAP BATTLE IS ABOUT HER.

It was produced by seventh graders in Oakland, California (with some help from teacher Tom McFadden). And it is delightful.

13. SHE HAS BEEN IMMORTALIZED ON THE SMALL SCREEN AND THE BIG STAGE.

In 1987, BBC's Horizon series aired The Race for the Double Helix, starring Juliet Stevenson as Franklin. Jeff Goldblum played Watson. In 2011, playwright Anna Ziegler premiered a one-act about Franklin called Photograph 51. It opened on the West End in 2015, starring Nicole Kidman as Franklin.

14. THE 2015 RUN OF PHOTOGRAPH 51 RE-IGNITED THE OLD CONTROVERSY.

While Kidman got much praise from critics for her turn as Franklin in Photograph 51, Maurice Wilkins' friends and former colleagues have taken exception to a scene where Wilkins takes a photograph—the titular Photo 51, which showed evidence of DNA's structure—from Franklin's desk when she isn't there, saying he would never have done something so dishonorable.

15. THE PLAY MAY COME TO THE BIG SCREEN IN THE NEXT FEW YEARS.

In 2016, the West End production's director, Michael Grandage, told The Hollywood Reporter that he hopes to turn the play into a film—with Kidman reprising the role.

Arrokoth, the Farthest, Oldest Solar System Object Ever Studied, Could Reveal the Origins of Planets

NASA/Johns Hopkins University Applied Physics Laboratory/Southwest Research Institute/Roman Tkachenko
NASA/Johns Hopkins University Applied Physics Laboratory/Southwest Research Institute/Roman Tkachenko

A trip to the most remote part of our solar system has revealed some surprising insights into the formation of our own planet. Three new studies based on data gathered on NASA's flyby of Arrokoth—the farthest object in the solar system from Earth and the oldest body ever studied—is giving researchers a better idea of how the building blocks of planets were formed, what Arrokoth's surface is made of, and why it looks like a giant circus peanut.

Arrokoth is a 21-mile-wide space object that formed roughly 4 billion years ago. Located past Pluto in the Kuiper Belt, it's received much less abuse than other primordial bodies that sit in asteroid belts or closer to the sun. "[The objects] that form there have basically been unperturbed since the beginning of the solar system," William McKinnon, lead author of one of the studies, said at a news briefing.

That means, despite its age, Arrokoth doesn't look much different today than when it first came into being billions of years ago, making it the perfect tool for studying the origins of planets.

In 2019, the NASA spacecraft New Horizons performed a flyby of Arrokoth on the edge of the solar system 4 billion miles away from Earth. The probe captured a binary object consisting of two connected lobes that were once separate fragments. In their paper, McKinnon and colleagues explain that Arrokoth "is the product of a gentle, low-speed merger in the early solar system."

Prior to these new findings, there were two competing theories into how the solid building blocks of planets, or planetesimals, form. The first theory is called hierarchical accretion, and it states that planetesimals are created when two separate parts of a nebula—the cloud of gas and space dust born from a dying star—crash into one another.

The latest observations of Arrokoth support the second theory: Instead of a sudden, violent collision, planetesimals form when gases and particles in a nebula gradually amass to the point where they become too dense to withstand their own gravity. Nearby components meld together gradually, and a planetesimal is born. "All these particles are falling toward the center, then whoosh, they make a big planetesimal. Maybe 10, 20, 30, 100 kilometers across," said McKinnon, a professor of Earth and planetary sciences at Washington University. This type of cloud collapse typically results in binary shapes rather than smooth spheroids, hence Arrokoth's peanut-like silhouette.

If this is the origin of Arrokoth, it was likely the origin of other planetesimals, including those that assembled Earth. "This is how planetesimal formation took place across the Kuiper Belt, and quite possibly across the solar system," New Horizons principal investigator Alan Stern said at the briefing.

The package of studies, published in the journal Science, also includes findings on the look and substance of Arrokoth. In their paper, Northern Arizona University planetary scientist Will Grundy and colleagues reveal that the surface of the body is covered in "ultrared" matter so thermodynamically unstable that it can't exist at higher temperatures closer to the sun.

The ultrared color is a sign of the presence of organic substances, namely methanol ice. Grundy and colleagues speculate that the frozen alcohol may be the product of water and methane ice reacting with cosmic rays. New Horizons didn't detect any water on the body, but the researchers say its possible that H2O was present but hidden from view. Other unidentified organic compounds were also found on Arrokoth.

New Horizon's flyby of Pluto and Arrokoth took place over the course of a few days. To gain a further understanding of how the object formed and what it's made of, researchers need to find a way to send a probe to the Kuiper Belt for a longer length of time, perhaps by locking it into the orbit of a larger body. Such a mission could tell us even more about the infancy of the solar system and the composition of our planetary neighborhood's outer limits.

The Moon Will Make Mars Disappear Next Week

Take a break from stargazing to watch the moon swallow Mars on February 18.
Take a break from stargazing to watch the moon swallow Mars on February 18.
Pitris/iStock via Getty Images

On Tuesday, February 18, the moon will float right in front of Mars, completely obscuring it from view.

The moon covers Mars relatively often—according to Sky & Telescope, it will happen five times this year alone—but we don’t always get to see it from Earth. Next week, however, residents of North America can look up to see what’s called a lunar occultation in action. The moon's orbit will bring it between Earth and Mars, allowing the moon to "swallow" the Red Planet over the course of 14 seconds. Mars will stay hidden for just under 90 minutes, and then reemerge from behind the moon.

Depending on where you live, you might have to set your alarm quite a bit earlier than you usually do in order to catch the show. In general, people in eastern parts of the country will see Mars disappear a little later; in Phoenix, for example, it’ll happen at 4:37:27 a.m., Chicagoans can watch it at 6:07:10 a.m., and New Yorkers might even already be awake when the moon swallows Mars at 7:36:37 a.m.

If you can’t help but hit the snooze button, you can skip the disappearing act (also called immersion) and wait for Mars to reappear on the other side of the moon (called emersion). Emersion times vary based on location, too, but they’re around an hour and a half later than immersion times on average. You can check the specific times for hundreds of cities across the country here [PDF].

Since it takes only 14 seconds for Mars to fully vanish (or reemerge), punctuality is a necessity—and so is optical aid. Mars won’t be bright enough for you to see it with your naked eye, so Sky & Telescope recommends looking skyward through binoculars or a telescope.

Thinking of holding an early-morning viewing party on Tuesday? Here are 10 riveting facts about Mars that you can use to impress your guests.

[h/t Sky & Telescope]

SECTIONS

arrow
LIVE SMARTER