What are the advantages of remote observing?
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Transcript of What are the advantages of remote observing?
What are the advantages of remote observing?
•Altitude
•Latitude
•Longitude
•Avoiding light pollution
•Technical support
•Taking on new astronomical challenges
•Wide range of telescopes and filters to chose from
Altitude
Latitude and longitude
The five telescopes in the RAS Observatory are sited an elevation of 2225 metres in the high desert - close to
Apache Point Observatory – and well above most atmospheric pollution.
Location: 31 miles east of the town of Alamogordo, New Mexico USA
Latitude: 32° 54' 14" Longitude: W 105° 31' 44”
Time Zone: GMT -7:00 New Mexico.
Latitude and longitude - continued
HORIZON
RAS Observatory view – 32N My home town – 52N
Just compare the view of the southern sky!
Light pollution
• Alamogordo, the nearest large town to the observatory, has one of the strictest light pollution ordinances in the United States. If you fly over Alamogordo at night, it is almost invisible, so effective is its battle against light pollution. The State of New Mexico takes light pollution seriously too and in 1999 Governor Gary Johnson signed the nation's strictest state anti-light pollution legislation.
Technical Support
New Challenges
• Most observers have little interest or aptitude for “tinkering”
• If something breaks they want/need/would like somebody else to mend it! This is exactly what happen at the RAS Observatory.
• Members wanted the chance to do a far greater variety of astronomical activities than were possible with their current equipment.
Five telescopes to chose from!
4 versions of M20 – each taken through a different telescope in the RAS Observatory
The types of projects members have done
• Using standard (RGB) and exotic (H Alpha, SII and OIII) filters to image both well known and less well known objects.
Rosette Nebula - Monoceros
Veil Nebula - NGC 6992
20 minutes in H Alpha, RED
20 minutes in OIII, GREEN
20 minutes in SII, BLUE
Crescent Nebula – NGC 6888
in Cygnus
Magnitude: 10.0 - Size: 18.0'x13.0'
40 minutes in H Alpha
Hydrogen Alpha S II
O III
M42 and M43
These well known objects looks very different at three different wavelengths. In each case the
exposure was 40 minutes.
Red = Ha, Green = SII, Blue =OIII Red = Ha, Green = OIII, Blue =SII