new sights and old favorites – 19 April, 2009

Location: at home in Tomball, TX
Cloud cover: none
Transparency: above average (4/5)
Seeing: average (3/5)
Darkness: no moon, city glow
Wind: none
Humidity: 50%-75%
Temperature: low 60’s
Start Time: 8:20 pm CDT
End Time: 10:30 pm CDT
OTA: 8″ SC

Saturn alternately fuzzy & clear; Iapetus “close” to planet, Titan and Rhea distinct, Dione & Tethys occasionally lost in glare and turbulence.

M35 OC was amazing, brought Amanda outside to see. Many, many stars (guide info said 70+) over a narrow magnitude range within 1/2 degree region.

38 Gem DBL, could not see color difference. Guessed delta mag between 3 and 4; SNP lists them as 4.7 and 7.8.

β Mon TRIPLE, split with 12.5mm Plossl, appeared DBL in 25mm.

NGC 2392 (eskimo nebula) appeared as a fuzzy disk with a distinct central star. No detail visible.

ζ Can DBL/QUAD (tegmen); ζ1 and ζ2 easily split, close binaries beyond ability of 8″ SCT.

ι Can DBL; blue and yellow easy split. estimated yellow about 1.5 mag brighter than blue. SNP actually lists them as 4.0 and 6.6, so more like 2.6…

NGC 3242 PNEB, also called “Ghost of Jupiter”. Appeared as a fuzzy disk with no detail and no central star. Seems smaller than Jupiter (in arcsec).

Open Clusters, Doubles, & Saturn – March 04, 2008

temp: 53F-46F
humidity: 37%-70%
transparency: 4/5 – 5/5
seeing: average 3/5

Attempted M1 (Crab Nebula) with 25mm, 32mm, 10mm, could not discern any nebulosity
using 25mm
M35 – dozens of stars, many bright – bow shape in center
M36 – moderately bright cluster, some linear patterns
M37 – faint cluster, few lines, bright center star
M38 – odd abstract bilateral symmetry of four rays (two short, two long), center star

M41 – behind a tree
M42 – observed to test dark adaptation of my eyes after failing to see M1. region is impressive as a cluster

M46 – wide cluster in 32mm, celestron controller indicated nebula in field of view, but I could not discern any
M47 – several bright stars, prominent lines, one tight pair of similar magnitude
M48 – dozens of similar magnitude stars, no prominent lines, many “wide” pairs
M50 – sparse cluster, wide magnitude range
M67 – dim cluster with pleasing random arrangement

Rigel – companion much fainter, 9.5″ separation
lambda orionis – similar magnitude companion 4″ separation, very close in 10mm but distinct during moments of good seeing
sirius – could not discern companion

Saturn was bright, Titan clear. Dione was dim but distinct. Rhea was very faint, disappearing at times with poorer seeing.