I was reading the Etsy blog this morning and enjoying their collection inspired by the reboot of Carl Sagan's Cosmos: A Personal Voyage - Cosmos: A Spacetime Odyssey hosted by Neil Degrasse Tyson, director of the Hayden Planetarium at the American Museum of Natural History. I was busily adding items to my favorites lists (not just my collection of science-themed items, but my collection of things I want myself, for the befuddled gift-buyers in my life), when I scrolled down and saw my own portrait of Jocelyn Bell Burnell! I'm flattered to be in this company. And yes, you should buy me the Mars globe and the screenprinted moon pillowcases with glow-in-the-dark constellations cause they would go perfectly with my own quilt with NASA imagery and glow-in-the-dark stitching. I mean really.
Showing posts with label Jocelyn Bell Burnell. Show all posts
Showing posts with label Jocelyn Bell Burnell. Show all posts
Monday, March 10, 2014
Tuesday, February 11, 2014
Bell Burnell and the Little Green Men
| Jocelyn Bell and the LGM-1 |
This year, I plan to grow my collection of portraits of women in STEM. I thought I'd get an early start on this project, with my first portrait of a scientist who is still working.
This is a linocut portrait of Jocelyn Bell (now Bell Burnell) and the incredible radioastronomy dataset she gathered when only a graduate student in 1967, working with Anthony Hewlish. The block is inked "à la poupeé" in dark blue grey and green on Japanese kozo paper. The first edition is a variable run of 10 prints, each 10" by 12.5" (25.4 cm by 31.8 cm).
In November, 1967, Jocelyn Bell (Burnell) was just a graduate student when she discovered the first radio pulsar (or pulsating star), a highly magnetized, rotating neutron star that emits a beam of electromagnetic radiation. This radiation (light in the radio frequency band) can only be observed when the star is pointed towards us; so, like the light from a distant lighthouse, it appears to pulse at a precise frequency. Jocelyn Bell had been working with her supervisor Antony Hewish and others to construct a radio telescope to study quasars (quasi-stellar objects which emit radio waves). She noted some "scruff" on her chart-recorder, and then that the pulses were incredibly regular, occurring every 1.337 seconds. Hewish was initially scornful and insisted the regular pulses must be noise from a human made source. He first dubbed this object, emitting with such regularity 'LGM 1' for "Little Green Men 1", a playful joke about their uncertainty about what could emit radiation so regularly - obviously it could only be a communication from extraterrestrials hahaha! After she found other such sources, in different places with different frequencies, her colleagues became convinced. These discoveries lead to the development of the pulsar model. LGM-1 is now known PSR B1919+21.
The 1968 paper announcing this discovery in Nature has five authors, lead by Hewish, followed by Jocelyn Bell. In 1974, Hewish won the Nobel Prize for this discovery, (along with fellow radioastronomer Marlin Ryle). Jocelyn Bell was not included as it was assumed that the "senior man" was responsible for the work. This was controversial and has been condemned by many leading astronomers like Fred Hoyle (who with Thomas Gold was first able to explain the signals as due to a rapidly rotating neutron star). Jocelyn Bell Burnell herself has stated she was not upset. Bell Burnell has a great career and won many honours after her impressive start, but her exclusion from the Nobel win, based on her own research strikes me and many others as one of the more blatant and egregious examples of gender bias in the selection of Nobel prize recipients.![]() |
| Cover of Joy Division's 1979 album 'Unknown Pleasures' designed by Peter Saville, using the pulsar data from the Cambridge Encyclopaedia of Astronomy |
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