Huggins and Miller, Proc. Roy. Soc. (1863)
Sun
Betelgeuse
Sirius
Aldebaran
The stars were undoubtedly suns after the order of our sun*…
—Huggins (1897)
*What was it that Giordano Bruno had conjectured?
Slide 58
Interpreting nebular spectra
Huggins and Huggins, Proc. Roy. Soc. (1889)
Remember: these are hand-drawn spectragrams
Slide 59
Huggins observed the planetary nebula 37. H IV Draconis
… after a few moments of hesitation, I put my eye to the spectroscope. Was I not about to look into a secret place of creation? . I looked into the spectroscope. No spectrum such as I expected! A single bright line only!
Slide 60
The bright line was something new in the spectrum
Huggins called it nebulium
In a planetary nebula, ionized oxygen and other elements are blasted off a giant star
This is the line ionized oxygen makes, not reproducible in 19th century chemistry labs
Slide 61
Slide 62
Married William when he was around 50
Margaret was an accomplished photographer
She designed photographic equipment for use with the spectroscope
Huggins laboratory notebooks also become much more organized and informative due to Margaret
Slide 63
William Huggins
in the
Tulse Hill Observatory
(ca. 1905)
Slide 64
The data plots don’t necessarily look like rainbows
Infrared, gamma-ray, microwave, x-ray spectra are all valuable data
Slide 65
The discovery of helium
P.J.C. Janssen (Fr) and J. Norman Lockyer (UK) independently determined that the solar atmosphere could be studied spectroscopically
Consequently, the bright orange ‘D’ line that was assumed to be sodium turned out to be an indication of a new element
Helium isolated in the laboratory in 1895 by William Ramsay
Slide 66
VVVVVrrrrroooooommmm
Spectra can also tell Astronomers if a distant object is moving towards or away from us
And also how fast it is spinning
The technique is to use the Doppler Effect to see how the spectral lines are affected