July 2012 Observing Targets

by Brian Cuthbertson



Mid-summer evening skies mean, by and large, the summer Milky Way. And certainly one could spend all one's observing time moving up and down that starry path. But surrounding constellations also have targets to offer, like this month's target in Hercules. Wherever you look, its a grand spectacle out there, a regular fireworks show. So get out there and enjoy!


95 Her rating EASY

double star in Hercules

RA 18h 01.5m Dec +21d 35.7' (2000)

Magnitude 4.3


Sitting in SE Hercules above Ophiuchus, 95 Her is a famous little double, notorious among observers for changing estimates of color. It consists of a pair of fifth magnitude giants separated by 6.3 arc seconds, with the combined light of a single 4.3-magnitude star. At their 470 light-year distance the pair has a separation of at least 900 Astronomical Units. Given their masses, it would take at least 11,000 years to complete a full mutual orbit, so its not a surprise that no relative orbital motion has yet been measured.


The odd color history of 95 Her goes back to 1780, when Herschel observed the pair as "bluish-white and reddish". Around 1830, Struve called them greenish yellow and reddish yellow. In 1855, Secchi called them orange and green. Piazzi Smyth observed them from the Peak of Teneriffe in 1856 as both white, but the following year called them "apple green and cherry red". Higgins actually watched Smyth's colors fade and then return in 1862-63. By 1878 Pickering was again reporting Struve's 1830 colors, but by 1905 Agnes Clerke reported "the stars of 95 Herculis are now an identical pale yellow."


95 Her isn't the only double to manifest apparent color changes. Similar changes have been reported for other well-known pairs including Gamma Leo, 70 Oph, Delta Her, Gamma Del and Zeta Cnc. But none of these stars have shown any noticeable spectral changes which would have to accompany any real change in color. Star colors, even for strongly contrasting pairs, are delicate and elusive; disagreements among even experienced observers seem to be the rule rather than the exception.


NGC 6664 rating MEDIUM

open cluster in Scutum

RA 18h 36.7m Dec -08d 13.5' (2000)

Magnitude 7.8


When it comes to open star clusters, the small Milky Way constellation of Scutum is best known for M11. But in fact, there are at least a dozen open clusters in Scutum. One of these, NGC 6664, is an easy find because it sits just 20' east of 4th-magnitude Alpha Scuti.


NGC 6664 is a sparse cluster embedded in a rich part of the Milky Way, and covers an area about one quarter that of the full Moon. It looks like a partially resolved cloud in a 2.4-inch refractor. In a 6-inch you can see about 35 stars in a 25' area, with the brighter ones mostly on the north side.


A 10-inch scope at medium powers will show 60 or more stars, all fainter than 10th magnitude. Overall, the cluster has no central condensation and is highly-elongated north to south.


A study by Halton Arp of reddening of cluster members reveals a cluster distance of 1,450 parsecs, or about 450 light-years. The cluster contains a Cepheid variable star as a member: EV Scuti varies from 9.9 to 10.3 over a 3.09-day period.

 

NGC 6629 rating HARD

planetary nebula in Sagittarius

RA 18h 25.7m Dec -23d 12.3' (2000)

Magnitude 11.3


This challenging little planetary lies in Sagittarius roughly 2 degrees north, and just a bit west, of 3rd-magnitude Lambda Sgr, which marks the top of the Sagittarius teapot. Closer in, you'll find it 7' south of 8th-magnitude SAO 186800. This is a difficult planetary for small scopes, even through an OIII filter, but it can be detected with averted vision.


In larger scopes, such as an 8-inch at 110x, NGC 6629 looks like a very faint round diffuse ball with no discernable edges. In a 10-inch scope at 100x, it looks like a 10th-magnitude star. At 250x its about 15" in diameter, fading abruptly at the edge.


The magnitude of the central star is 12.9


 
 
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