Tonight's Sky
Sun
Sun
Moon
Moon
Mercury
Mercury
Venus
Venus
Mars
Mars
Jupiter
Jupiter
Saturn
Saturn

Tonight's Sky — Change location

OR

Searching...

Tonight's Sky — Select location

Tonight's Sky — Enter coordinates

° '
° '

All around Aries

This autumn constellation is home to all kinds of targets for telescope observers.
RELATED TOPICS: OBSERVING
ChapleGlenn
Aries is typical of the constellations of autumn — rather obscure to the naked eye, but a treasure trove of celestial delights for the telescope owner.” This is the opening sentence to my double star column in the November 1977 issue of Deep Sky Monthly. Back then, I used the star-hop method to locate and observe the five double stars featured. We’ll do the same as we revisit these stellar duos — plus a few bonus targets.

The focus of that column was the area around the naked-eye stars Hamal (Alpha [α] Arietis), Sheratan (Beta [β] Arietis), and Mesarthim (Gamma [γ] Arietis). Mesarthim is one of the loveliest double stars in the entire night sky. It’s a striking twin system, nearly identical in brightness (magnitudes 4.5 and 4.6) and color (both are pure-white stars of spectral classes A1 and B9). Separated by 7.4", the two are easily split with a common 2.4-inch refractor and a magnification around 50x. As we peer into the eyepiece, they seem to stare back like the gleaming eyes of a celestial cat (or car headlights, if you’re a cat-hater).

More of a challenge is 1 Arietis, 3° north of Mesarthim. To open the 2.9" gap separating its magnitude 6.3 and 7.2 components, you’ll need steady skies and a magnification of 100x or more. Just over a degree south (and 1° west-northwest of Sheratan) is the faint pair Σ 175, one of over 3,100 double stars cataloged by the German-Russian astronomer Friedrich Georg Wilhelm von Struve in the 1830s. These magnitude 9.0 and 9.4 stars have widened from 6.0" in 1783 to a current 28.1" and are likely an optical pair (meaning not physically related).

A return to bright, easily resolved double stars brings us to Lambda (λ) Arietis, found 2½° west of Hamal. The same 50x magnification that split Mesarthim will readily bridge the 37" space between Lambda’s magnitude 4.8 and 6.7 components. Back at Hamal, we hop 2½° northward to the final destination in that Deep Sky Monthly article, the wide triple 14 Arietis. The 5th-magnitude primary star has two 8th-magnitude companions, one 93" to the north-northeast and one 105" to the west.
The area around Aries’ three brightest stars contain plenty of fun deep-sky treats.
The area around Aries’ three brightest stars contain plenty of fun deep-sky treats.
Astronomy: Roen Kelly
So that I’m not totally plagiarizing that 1977 article (can you plagiarize your own writing?), let me add the faint Struve pair Σ 196. This magnitude 9.4 and 10.2 duo (21" separation) is conveniently positioned immediately south of a 6th-magnitude star that lies 1½° east of Sheratan.

For you fans of faint fuzzies, I’ll throw in the Fiddlehead Galaxy (NGC 772), which glows at magnitude 10.3. A challenge for small scopes and even larger ones under moderately light-polluted skies, it appears as a faint, slightly elliptical smudge with a bright nucleus. You’ll find it in an area 1½° east and slightly south of Mesarthim.

Finally, something for you variable star observers. Just 5' east of 6th-magnitude 21 Arietis — found by star-hopping from 14 Arietis, past 16 Arietis to 20 Arietis, and then dropping ¾° south — is the Mira-type variable R Arietis. It varies from magnitude 7 or 8 at maximum brightness to 13 or 14 at minimum over an average cycle of six months.

Based on past behavior, the American Association of Variable Star Observers (AAVSO) predicts that, as this issue goes to press, R Arietis should be on the rise to an early December maximum. Should you wish to monitor this activity, you can obtain free printable charts complete with notated magnitudes of nearby comparison stars at the AAVSO website (www.aavso.org).

Under “Observing” on the main page, scroll down to “Variable Star Charts” and across to “Variable Star Plotter” (VSP). At the VSP page, type in “R Ari” in the name/designation box, and select “A” as your chart scale option. Press “Plot Chart” to create a 15°-wide finder chart (north up) that includes Hamal, Sheratan, and Mesarthim. Use the “B” scale option for a 3°-wide chart to help you monitor R Arietis in the months ahead.

Questions, comments, or suggestions? Email me at gchaple@hotmail.com. Next month: We crater-hop to “Mutus X.” Clear skies!
0

JOIN THE DISCUSSION

Read and share your comments on this article
Comment on this article
Want to leave a comment?
Only registered members of Astronomy.com are allowed to comment on this article. Registration is FREE and only takes a couple minutes.

Login or Register now.
0 comments
ADVERTISEMENT

FREE EMAIL NEWSLETTER

Receive news, sky-event information, observing tips, and more from Astronomy's weekly email newsletter. View our Privacy Policy.

ADVERTISEMENT
ADVERTISEMENT
RCLP_ASY_0919_mediumrectangle
NASA's greatest space probes. What Cassini, Juno, and New Horizons discovered on their missions.
Find us on Facebook