RA: 06h 33m 45s, Dec: +4°59’54”
The Rosette Nebula is a large H II region located in the constellation of Monoceros, just to the left of Orion. The nebula is a large star forming region with a cluster at the centre that , through the action of the stellar winds, has blown a large cavity out of the nebula from which it formed. The nebula itself is often referred to simply as NGC 2237 (though NGC 2238, NGC 2239 and NGC 2246 are all parts of the same nebula). The cluster is designated NGC 2244.
Continue reading NGC2244 – The Rosette Nebula
The lunar eclipse of the 3rd March 2007 brought clear skies and good conditions across much of the UK, with only some thin high cloud arriving in Oxfordshire towards the end of the eclipse. Maximum eclipse occured at 23:20:56 – ideally timed for the UK.
More recently, on the 21st February, 2008, another lunar eclipse was visible from the UK and Europe early in the morning. However, the weather for this event was not as favourable with cloudy conditions across much of the UK (despite having a long period of clear weather in the preceding week!).
Continue reading Lunar Eclipse of March 3rd 2007
UPDATE: Since writing this article, BT have moved off the Yahoo platform (see: www.bt.com/newemail) – I’m unsure if the same issue is apparent for BT users, but the same issue exists for Yahoo as far as I know.
If you are a BT or Yahoo email user, then you may notice occasionally that your email takes an age to arrive. Sometimes you may even discover that an email someone sent you you has never arrived. If you experience this, here’s a bit of an explanation as to why this may be happening…
Continue reading BT/Yahoo? Slow Email?
Continuing in the migration of my old site, here’s a post with a round up of my best h-alpha solar images. For a while, I owned a Coronado Solarmax 60 with BF15 blocking filter which I used to use on my Takahashi FC60NZ – I traded this more recently for the FLT110 – I found that I really wasn’t getting to use the h-alpha equipment for most of the year (work gets in the way when the sun is up!).
The h-alpha filter works by using an etalon to restrict the wavelengths of light as viewed through the telescope down to only a small region of the spectrum around 656.3nm (typically with a bandwidth of <0.7Å), which is a principal emission wavelength of excited hydrogen atoms (for the transition n=3 to n=2 in the Balmer series). This allows features such as prominences, flares, filaments and active regions to be observed, whereas in white light these are often not as noticable or are invisible.
Continue reading Solar H-Alpha Imaging Round Up
So the weekend just gone has had fabulous weather here in the UK – sunny, warm (for February!) days, and cold clear nights – and so I thought I’d try to setup my imaging kit to have a go at some astronomy for the first time since April 2007, and also as a bit of a dry run before the Kelling Heath star party in April. I even managed an image of the moon – 30 images using the ST2000XM on the FLT110, processed in Registax – click the image above to view it!
Of course, nothing goes smoothly:
Continue reading Equipment Woes and a Crescent Moon