Sky & Telescope - USA (2019-11)

(Antfer) #1

O. M. Mitchel


34 NOVEMBER 2019 • SKY & TELESCOPE


Neither his projector nor the images for it survives, so we
don’t know exactly how they looked. However, eight months
later, Mitchel launched his monthly journal The Sidereal
Messenger, the fi rst U.S. periodical exclusively dedicated to
astronomy. In print from July 1846 through October 1848,
almost every issue of The Sidereal Messenger featured a dra-
matic frontispiece of an astronomical object, half a dozen of
which were drawn at the eyepiece of the Cincinnati telescope.
It’s likely his projected telescopic views were similar.
From all accounts, the emotional impact made by celestial
objects as seen through the nation’s largest telescope was akin
to that felt by the NASA generation on seeing the fi rst spec-
tacular images returned from the Hubble Space Telescope in
the 1990s. Immediately, the Boston organizers invited him to
repeat the course the next month (January 1846). One audi-
ence member invited him to offer a course in Brooklyn, New
York. Mitchel’s brilliant lecturing career was launched.
Over the next decade and a half, Mitchel lectured almost
every winter, ultimately speaking in at least 21 cities in 10
states to audiences of between 1,000 and 4,000 per night
and returning to several cities year after year for repeat visits.
By 1859, he was in such great demand that he offered three
concurrent lecture series at three separate venues around
New York City!

Although his lectures were not easy material, he had a
supreme gift for clarity and simplicity. He led his audiences
through the nebular hypothesis and discussions of the stabil-
ity of the solar system, detailing such complex concepts as
aberration of starlight and nutation. He excited audiences by
updating them on the latest news regarding the discovery of
the new planet Neptune and controversy over the determina-
tion of its orbit. He swept his listeners far out into space on
vivid imaginary journeys through the solar system to the very
edges of our Milky Way, and far back in time to the discover-
ies of ancient naked-eye astronomers.
Through all his lectures, Mitchel, a devout Protestant,
emphasized the sublime glory of God as creator and lord
of the universe — a message that deeply resonated with his
audiences, and that indeed was what he fi rst spoke when he
beheld the crescent Moon at age three from his brother’s
arms. In later years, he also gave entire courses of lectures on
the astronomy of the Bible.
Not only were Mitchel’s lecturing proceeds each winter
enough to support his family and the Cincinnati Observatory
for the rest of the year, but they also permitted him to raise
funds for other causes, including new astronomical obser-
vatories. One such benefi ciary of his efforts was the Dudley
Observatory in Albany, New York, for which he chose the
site and designed the building in 1851–52. In 1859, Mitchel
became Dudley’s second director, moving to Albany in spring
1860 — while still remaining director at Cincinnati. He was
scarcely at Dudley a year, however, when the Confederacy
fi red on the U.S. garrison at Fort Sumter, opening the Civil
War in April 1861.

“Old Stars”
Ever since his days as a West Point cadet, Mitchel yearned to
command an army. In August 1861, Abraham Lincoln offered
him a commission as Brigadier General of Volunteers. In early
1862, his commanding general tasked Mitchel — dubbed by

pNEXT-DOOR NEIGHBOR Left: This undated lunar image, which
highlights Montes Apenninus (Apennine Mountains) and Archimedes
Crater (below center), shows the eyepiece fi eld of view through the 11-
inch Merz and Mahler refractor at 500×. In his early lectures, Mitchel
projected a few spectacular telescopic views at the end of his lectures.
Sometime after January 1851, however, he stopped including images
and relied exclusively on the power of the spoken word.

pTHE RINGED PLANET Right: Mitchel’s drawing of Saturn, made
the night of October 13, 1846, shows the planet’s orb and rings, as
well as six of the seven then-known satellites. Mitchel compressed
the proportional positions of the satellites at left, possibly because he
wanted to show as much detail as he could on the planet itself.

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