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The Caldwell Objects

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64<br />

6 4<br />

Tau Canis Majors Cluster;<br />

“Northern” Jewel Box;<br />

Mexican Jumping Star;<br />

Liquid Pyramid<br />

NGC 2362<br />

Type: Open Cluster<br />

Con: Canis Major<br />

RA: 07 h 18.7 m<br />

Dec: -24° 57'<br />

Mag: 4.1<br />

Diam: 6'<br />

Dist: 5,100 light-years<br />

Disc: Giovanni Batista Hodierna,<br />

before 1654<br />

W. H ERSCHEL: [Observed 6 March 1785] A very beautiful cluster of<br />

pretty [bright] stars, very rich, contain [s] the [star] 30 Canis [Majoris].<br />

(ΗVII-17)<br />

I N THE LOWER BACKBONE OF C ANIS M AJOR,<br />

Orion's greatest hunting dog, is one of the most<br />

inconspicuous yet visually stunning open clusters<br />

accessible to observers in both hemispheres.<br />

NGC 2362 is called the Tau (τ) Canis Majoris<br />

Cluster by most, but I call it the "Northern" lewel<br />

Box. I place "Northern" in quotes because the<br />

cluster is north of the original Jewel Box cluster<br />

(<strong>Caldwell</strong> 94) but south of the celestial equator.<br />

<strong>The</strong> two Jewel Boxes have much in common.<br />

Both have Greek-letter designations; the Jewel<br />

Box is also known as Kappa (κ) Crucis. Both<br />

shine at 4th magnitude; both are roughly 5,000<br />

light-years distant; and both are among the<br />

youngest star clusters known, with ages of a few<br />

million years. In his Astronomical <strong>Objects</strong> for<br />

Southern Telescopes, Ernst Hartung writes: "This<br />

most beautiful cluster contains about forty stars<br />

grouped around the very bright white 30 [Canis<br />

Majoris] which is set like a jewel in their midst."<br />

254<br />

GC: Cluster, pretty large, rich.<br />

NGC: Cluster, pretty large, rich (30 Canis Majoris).<br />

Shining at magnitude 3.8, the Tau Canis Majoris<br />

Cluster is about 13° southeast of dazzling Sirius<br />

and nearly 3° northeast of 2nd-magnitude Delta<br />

(δ) Canis Majoris. <strong>The</strong> cluster is only 0.7<br />

magnitude fainter than M44, the famous Beehive<br />

Cluster in Cancer. Yet look at the star called Tau<br />

Canis Majoris with the naked eye and you'd<br />

never know a cluster existed around it. That's<br />

because the stars in NGC 2362 are packed into an<br />

area only 6' across (1/12 the Beehive's angular<br />

diameter).<br />

Contrary to popular belief, William Herschel<br />

did not discover the Tau Canis Majoris Cluster;<br />

he rediscovered it. <strong>The</strong> honor goes to Giovanni<br />

Batista Hodierna (1597-1660), whose observations<br />

appeared in his De Admirandi Coeli Caracteribus —<br />

a catalog, published in 1654, of some 40 deep-sky<br />

objects. <strong>The</strong> catalog somehow escaped Herschel's<br />

notice, and indeed the modern world's, until<br />

Giorgia Fodera Serio, Luigi Indorato, and Pietro<br />

Nastasi<br />

Deep-Sky Companions: <strong>The</strong> <strong>Caldwell</strong> <strong>Objects</strong>

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