Move mouse over sketch to see labels. Click image for larger version.
The observing highlight of the evening atop Haleakala was gazing through my binoculars at the rich starscape in the vicinity of Eta Carinae. I had not done any homework on the area beforehand, so I approached it with unexpecting eyes. The mottled depths of the surrounding Milky Way, the smattering of intensely bright foreground stars, the abundance of open clusters of all shapes, sizes and intensities, and the stunning patches of glowing nebulosity made the whole region a delicious feast for the eyes. One incredible open cluster to the northeast, nearly took my breath away, but I did not have time to even attempt a sketch of it. Instead, I chose to render the region bracketed by the Eta Carinae complex and a much more manageable cluster, NGC 3293.
Eta Carinae was a brilliant orange star that surrounded itself in a plush comfort of nebulosity. This misty region ended abruptly to the south and then emerged again to surround a trio of bright stars. The observation and sketch were done more hastily than I would have liked and I know there was more detail to be extracted from this bright nebula, but I took what I could get. The northwest side of the view was punctuated by the small, bright open cluster, NGC 3293. Four bright stars announced themselves within its glowing boundary of unresolved starlight.
This section of the sky is still beckoning me, and I know I will have to return to it again with more time to spare. Even if I only have binoculars again the next time, it will still offer more than I can possibly absorb.
Eta Carinae is one of the most massive stars in the universe and is likely greater than 100 solar masses. It is about 4 million times more luminous than the sun, but radiates 99% of this energy in the infrared. Due to its extreme mass, it is expected to go supernova within the next few hundred thousand years. In the meantime, as it rapidly sheds matter, it goes through sporadic, violent outbursts. The most recent outburst peaked in 1843 when Eta Carinae became a magnitude -1 star, second only to Sirius. This eruption generated a rapidly expanding plume of gas that now forms a fascinating dumbell shape (see Hubble image below).
Image courtesy of NASA and STScI.
NGC 3372 is also catalogued and known as ESO 128-EN013, h 3295, GC 2197, Eta Carina Nebula, Keyhole Nebula. Discovered by Nicolas-Louis de Lacaille in 1751.
NGC 3293 is also catalogued and known as Cr 224, MEL 100, ESO 128-SC005, Lund 551, OCL 816, h 3276, GC 2144, Gem Cluster. Discovered by Nicolas-Louis de Lacaille in 1751.
|Subject||Eta Carinae, NGC 3372 and NGC 3293|
Eta Carinae: Peculiar Supermassive Star
NGC 3372: Emission Nebula
NGC 3293: Open Cluster (I 3 r)
Eta Carinae: RA: 10:45:03.6 / Dec: -59:41:04
NGC 3372: RA: 10:45:08.5 / Dec: -59:52:04
NGC 3293: RA: 10:35:53.8 / Dec: -58:14:10
NGC 3372: 120′ x 120′
NGC 3293: 5′
Eta Carinae: -0.8 to 7.9 variable (currently ~5)
NGC 3372: 3.0 bMag
NGC 3293: 4.7 vMag
|Date/Time||June 3, 2007 – 9:15 HADT
(June 4, 2007 – 7:15 UT)
|Observing Loc.||Haleakala Summit, Maui, HI (10,000 ft)|
|Instrument||Oberwerk 15 x 70 Binoculars|
|Conditions||Clear, Cool, Breezy|
|Transparency||~ Mag 6.5 NELM|
|*Sources||NGC/IC Project; AAVSO|
*Based on published data.