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APOGEE IMAGING • CANON • CELESTRON • CORONADO • EXPLORE SCIENTIFIC • FARPOINT • FLI • JMI • KENDRICK • MEADE • MOONLITE • ORION • PENTAX • PLANEWAVE<br />

LX800<br />

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Woodland Hills, CA 91364<br />

Mon-Sat: 9am-6pm (PST)<br />

Toll Free: (888) 427-8766<br />

Local:(818) 347-2270<br />

Fax:(818) 992-4486<br />

STi<br />

Rich View SolarMax II<br />

In Stock!<br />

Drive M<strong>as</strong>ter<br />

In Stock!<br />

WWW.TELESCOPES.NET<br />

See us at the:<br />

21 st Annual<br />

NEAF<br />

NORTHEAST<br />

ASTRONOMY<br />

FORUM<br />

Suffern, NY • April 28-29<br />

QSI • SBIG • SKY-WATCHER USA • SOFTWARE BISQUE • STARLIGHT FOCUSER • STARLIGHT XPRESS • TAKAHASHI • TELE VUE • THE IMAGING SOURCE • VIXEN<br />

Letters<br />

in my front yard with a 5- and 8-inch<br />

Schmidt-C<strong>as</strong>s. After retiring from 30<br />

years of social work, I now fi nd myself the<br />

lucky director of a small planetarium in<br />

Ohio, where your magazine continues to<br />

prove invaluable. I just fi nished reading<br />

the March issue, but I fi rst read the online<br />

version l<strong>as</strong>t week. The digital edition looks<br />

For the Record<br />

✹ The March cover story listed Simon Portegies Zwart’s institution <strong>as</strong> the University of<br />

Amsterdam. He works at Leiden University in the Netherlands.<br />

✹ In the timetable on page 69 of the February article “May’s Great Annular Eclipse,” the<br />

times for Arizona were wrongly corrected for Daylight Savings Time. (Arizona does not<br />

observe DST.) All times listed for Arizona should be one hour earlier. You can also go to<br />

the map at eclipse.gsfc.n<strong>as</strong>a.gov to see predictions in Universal Time.<br />

For a list of p<strong>as</strong>t errata, ple<strong>as</strong>e go to SkyandTelescope.com/Errata.<br />

75, 50 & 25 Years Ago Roger W. Sinnott<br />

May–June 1937<br />

Ghost Images “Not long ago the discovery<br />

of a faint southern comet w<strong>as</strong> announced [by<br />

Harvard Observatory, relayed from a Southern<br />

Hemisphere amateur <strong>as</strong>tronomer]. But, al<strong>as</strong>!<br />

there w<strong>as</strong> no new comet. The experienced amateur<br />

w<strong>as</strong> not careful enough about the refl ection<br />

in i his telescope from<br />

the t nearby planet Mars.<br />

He H had observed and<br />

reported r a ghost. . . .<br />

“[Ghost images] are<br />

even e more dangerous<br />

than t the nebulae and<br />

star s clusters that try to<br />

look l like comets, since<br />

the t ghost will appear to<br />

move in i the h course of fan<br />

hour because of [the]<br />

changing relative position of observer’s eye<br />

and telescope . . . and <strong>this</strong> apparent motion of<br />

an apparent comet so excites the observer that<br />

judgment abandons him and he d<strong>as</strong>hes for the<br />

telegraph offi ce.”<br />

Then <strong>as</strong> now, ghost images are usually caught<br />

before the offi cial announcement of a new<br />

discovery.<br />

May 1962<br />

Stellar Giant “One of the largest known stars<br />

— the red supergiant component of the eclipsing<br />

binary VV Cephei — h<strong>as</strong> a diameter 1,620<br />

times the sun’s, according to Indiana University<br />

<strong>as</strong>tronomer Benjamin F. Peery, Jr.<br />

splendid, is well designed, and is e<strong>as</strong>y to<br />

navigate . . . but the paper copy I hold in<br />

my hand is irreplaceable. Of course, that’s<br />

only the opinion of one old guy.<br />

iPhone-, iPad-, and Kindle-less at the<br />

Hoover-Price Planetarium—<br />

David L. Richards<br />

Canton, Ohio<br />

“This fi nding came<br />

from f his spectroscopic<br />

study s of the unusual 20.4year<br />

y binary. . . . [Knowing<br />

the t orbits’ sizes,] the<br />

Indiana I <strong>as</strong>tronomer could<br />

evaluate e the diameter of<br />

the t M star from the orbital<br />

elements e and the known<br />

duration of the eclipses. eclipse This red supergiant, he<br />

fi nds, is so enormous that the orbit of Jupiter<br />

could be fi tted inside it.”<br />

Peery’s result holds up well today. VV Cephei<br />

h<strong>as</strong> just a few contenders for largest known star;<br />

recent studies put it from 1,600 to 1,900 times the<br />

Sun’s diameter, nearly the size of Saturn’s orbit.<br />

May 1987<br />

Neutrinos from Hell “Neutrino <strong>as</strong>tronomy, for<br />

decades the sole concern of theorists, became<br />

a genuine observational science early on February<br />

23rd. That day, a handful of these elusive<br />

particles were detected from Supernova 1987A<br />

in the Large Magellanic Cloud. . . .<br />

“The observations represent<br />

r the fi rst neutrino<br />

detections d from a known<br />

extraterrestrial e<br />

source.”<br />

Technical editor Ronald<br />

A. A Schorn spearheaded<br />

S&T’s S coverage of the nearest<br />

e supernova observed in<br />

modern m times.

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