Smorgasbord of potential pleasure targets for Brandt 3/4/06 training session
Observing session time frame: 3/04/2006 7:00PM LT to 03/04/2006 9:00PM Local time - same as - 03/05/2006 2:00UTC to 03/05/2006 4:00UTC - subject as always to cloudy weather in March: Total Days 31 Mean Clear Days 7 Mean Partly Cldy Days 8 Mean Cldy Days 16 This will be a Moon and bright star night because the Moon is up; it will not be a DSO night. Although the focus of the session is training on physical use of the dome and scope during cold weather, a smorgasbord list of potential pleasure targets, from which a couple can be selected for the March 4 Brandt session include the following. Az and Altitude coordinates for stellar objects listed below are for 3/04/2006 7:00PM. Lunar targets are for the terminator position at 40.3 East longitude at 8:00pm local time. Calculated characteristics for the Brandt scope are listed in Part II. - Enjoy Canopus56(Kurt) I. Smorgasboard of targets I(A). Lunar At 3:00 UTC (8:00pm local time), Rukl's lunar terminator estimator tables (p.218-219 Rukl's Atlas of the Moon) puts the lunar terminator at 40.3 East lunar longitude. The favorable libration on March 4 per the RASC Handbook is at the equator on the east limb. Potential showcase objects for the evening are: Crater Hercules Crater Gutenberg Montes Pyrenaues Crater Janessen - and possibly - Rupes Cauchy North to South, some interesting features at 8:00pm might be: 1) 80 N region - Crater deSitter (65km) 80.1 N, 39.6 E, Rukl Map 5 2) 80 N region - Crater Billard (90km flooded creater) 74.6 N, 37.5 E, Rukl Map 5 3) 50 N region - Mare Firgoris 52 N, 40 E (surface albedio effects), Rukl Map 6 4) 50 N region - Crater Hercules (69 km dark material on floor) 46.7 N, 39.6 E, Rukl Map 14 5) 40 N region - Crater Maury (17.6 km) 37.1 N, 39.6 E, Rukl Map 15 6) 20 N region - Crater Fray (20 km, corroded, flooded crater) 16.6 N, 40.2 E, Rukl Map 25 7) 10 N region - Rima Cauchy (240 km - east 20km only visible) 9 N, 37 E, Rukl Map 36-37 8) 10 N region - Rupes Cauchy (120km fault similar to the Rupes Recta - the Straight Wall - east 20km only visible), Rukl Map 36-37 9) 10 S region - Crater Gutenberg (74km - complex crater floor) 8.6 S, 41.2 E, Rukl Map 48-47 10) 20 S region - Crater Bohnengerger (33km) 16.2 S, 40 E, Rukl Map 58-59 11) 20 S region - Montes Pyrenaues (250km mountain range) 14 S 41 E, Rukl Map 58-59 12) 40 S region - Craters Matius (88km), Fabricus (78km) and Janessen (190km - old degraded crater with wide rilles and ridges), approx. 42.9 S, 42 E, Rukl Map 68 13) 60 S region - Crater Vlacq (89km), Rukl Map 75 14) 60 S region - Crater Nearoh (76km) 58.5 S, 39.1 E, Rukl Map 75 15) 80 S region - Crater Boaguslausky (97 km) 72.9 S, 43.2 E, Rukl Map 74 16) 80 S region - Crater Scott (108km) 81.9 S, 45.3 E, Rukl Map 74 (P.S. Some of the crater names may be misspelled. I typed them up quickly and from handwritten notes.) I(C). Bright, Colorful Multiple Stars in the zenith hole from the Belmont Colorful Double List, by Azimuth Id Con J2000 AzAlt SpecPri V V2 Sep Notes 1) psi05 Aur Aur J064643.20+433448.0 Az072.75 Alt+74.32 G0V 5.4 8.4 36.2 Belmont note: yellow/blue; CCDM06467+4335, R Aur 2) pi. Gem Gem J074731.20+332512.0 Az092.73 Alt+60.53 M0III 5.15 5.3 11.4 Belmont note: orange/bluish triple with 3rd at 92"; CCDM07475+3325 3) HD046296 Aur J063419.20+380448.0 Az095.32 Alt+76.04 K0 6.6 10 43.2 Belmont note: yellow/blue/blue quad; CCDM06343+3805, STF 1103 4) HD035295 Aur J052512.00+345136.0 Az176.15 Alt+84.08 K1pvar+ 6.5 8.6 31.2 Belmont note: yellowish/orange; CCDM05252+3451, HJ 2268 5) HD033203 Aur J051019.20+371800.0 Az216.98 Alt+85.71 B2II 6.8 7.1 1.6 Mullaney: gold & bluish-red; CCDM05103+3719, STF0644 6) 56 Per Per J042438.40+335736.0 Az244.32 Alt+76.53 F4V 5.9 8.7 4.5 Belmont note: gold/yellow; CCDM04246+3358 I(C) Position of Planets above horizon at 2:00 UTC, 7:00pm (from Your Sky) by Azimuth Body RA_Dec Az_Alt Saturn 8h 31m 11s +19° 39.7' / 103.734 44.930 Mars 4h 22m 40s +23° 21.9' / 220.527 68.236 Moon 3h 17m 50s +22° 19.1' / 244.382 57.662 Mercury 23h 42m 2s +1° 39.6' / 268.217 4.580 Setting I(D). Separation resolution testing stars by Azimuth Argyle has published a set of matched resolution test stars. Here are some stars spread across the scope's Dawes and Rayleigh limits. None are well-placed near the zenith hole: Id Con J2000 AzAlt SpecPri V V2 Sep PA PA Epoch Other names 1) HD050700 Mon J065408.52-055108.6 Az150.40 Alt+38.93 A6Vn 6.39 6.6 1.3 170 2002 CCDM06541-0551, WDS06541-0551, STF 987, HIP033154 2) HD015328 Cet J022759.88+015739.2 Az237.25 Alt+34.64 K0III 6.45 6.7 0.52 29 2002 CCDM02280+0158, WDS02280+0158, KUI 8, HIP011474 3) HD006886 Psc J010939.12+234739.8 Az272.66 Alt+35.00 F0 6.65 6.8 0.62 290 2002 CCDM01097+2348, WDS01096+2348, BU 303, HIP005444 4) HD208132J Cep J215137.32+654510.1 Az334.55 Alt+28.31 A1m 6.37 6.7 1.4 145 2002 CCDM21516+6545, WDS21516+6545, STF2843, HIP107893 Argyle, R. (ed). 2004. Tables 2.1-2.7, Test Stars for Binocular through 600mm Telescopes. In Observing and Measuring Visual Double Stars. Springer. ISBN 1-85233-558-0 http://www.springer.com/ II. Some Brandt telescope characteristics: II(A). Resolution criteria: Airy disk radius 0.692 arcsecs Dawes limit 0.579 arcsecs Rayleigh limit 0.692 arcsecs Airy disk diameter 1.384 arcsecs Airy disk diameter linear size 22.546 microns Linear resolving power - theoretical 108 line pairs/mm Linear resolving power - practical film 60 line pairs/mm FWHM angular size 0.579 arcsecs FWHM linear size 9.425 microns II(B). Eyepiece fl/TFOV data at sky brightness ZLM 5.5 mags, 20.0 MPSAS: Note: These limiting magnitudes will not apply to near quarter-phase Moonlight sky on March 4. The telescopic limiting magnitude may be substantially lower due to Moon light. TFOV estimates and useful magnifications apply. Eyepiece focal length 9 mm Eyepiece AFOV 52 degrees Telescopic magnification 373.3 power Magnification per inch: 46.7 useful for: Double stars Telescope TFOV 0.1 degrees Telescope TFOV 8 arcmins Telescope TFOV 501 arcsecs Limiting telescopic magnitude - stellar, color index 0: 14.4 mags Eyepiece focal length 15 mm Eyepiece AFOV 52 degrees Telescopic magnification 224.0 power Magnification per inch: 28 useful for: Specific planetary lunar detail Telescope TFOV 0.2 degrees Telescope TFOV 14 arcmins Telescope TFOV 836 arcsecs Limiting telescopic magnitude - stellar, color index 0: 14.4 mags Eyepiece focal length 20 mm Eyepiece AFOV 52 degrees Magnification per inch: 20.6 useful for: Planetary and lunar details Telescopic magnification 168.0 power Telescope TFOV 0.3 degrees Telescope TFOV 19 arcmins Telescope TFOV 1114 arcsecs Limiting telescopic magnitude - stellar, color index 0: 14.2 mags Eyepiece focal length 52 mm Eyepiece AFOV 48 degrees Telescopic magnification 64.6 power Magnification per inch: 8 useful for: Small clusters and galaxies Telescope TFOV 0.7 degrees Telescope TFOV 45 arcmins Telescope TFOV 2675 arcsecs Limiting telescopic magnitude - stellar, color index 0: 13.3 mags III. Telescopic limiting magnitude test areas There are no good pre-mapped Clark TLM fields in bright open clusters near the zenith on March 4. Possible bright but lower altitude TLM fields pre-mapped by Clark and in the RASC 2006 Handbook are: Id Con J2000 Alt-Az coord Notes M67 Cnc J085006.00-115300.0 Az107.35Alt+36.42 Northwest quadrant of M67; mag range: 10.6-21.3; In the RASC 2006 Handbook NGC225 Cas J004342.00+614648.0 Az321.64Alt+44.30 Clark note: 20 stars mag 9+ Transiting off-zenith Landolt standard star fields are: Area Con J2000 Alt-Az coord Notes SA97 Ori J055725.92+000140.8 Az167.04Alt+48.52 Centered on 60 Ori, HD040210, mag range 7-14, N=37 stars SA98 Mon J065209.60-001742.0 Az148.13Alt+44.24 Centered on HD050209, mag range 8-13, N=30 with 46 supps to mag 18 Clark, R.N., 1990. Star Clusters for Finding Your Limiting Magnitude. Appendix C in Visual Astronomy of the Deep Sky, Cambridge University Press and Sky Publishing http://www.clarkvision.com/visastro/ RASC. 2006. RASC Observer's Handbook. Annual. http://www.rasc.ca/publications.htm Landolt1973: Landolt, A. 1973. UBV photoelectric sequences in the celestial equator selected areas 92-115. 1973AJ.....78..959L; CDS Cat. VI/19 1996yCat.6019....0L http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?1973AJ.....78..959L Landolt1992: Landolt, A. Jul. 1992. UBVRI photometric standard stars in the magnitude range 11.5-16.0 around the celestial equator. 1992AJ....104..340L ; CDS Cat. II/183A/ http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=1992AJ....104..340L __________________________________________________ Do You Yahoo!? Tired of spam? Yahoo! Mail has the best spam protection around http://mail.yahoo.com
Quoting Canopus56 <canopus56@yahoo.com>:
Although the focus of the session is training on physical use of the dome and scope during cold weather, a smorgasbord list of potential pleasure targets, from which a couple can be selected for the March 4 Brandt session include the following.
Yada, yada, yada... No self respecting maker of any potentially pleasureful target list, would call the list complete without including Venus. Not the one in the sky, but the one who lurks behind the solid hardwood door, in the second story appartment in building 2A across the pond... ;)
Canopus56 wrote:
This will be a Moon and bright star night because the Moon is up; it will not be a DSO night.
Not to be a grinch, but please note that it will not be a star party night either. The evening will be used for training only. And being that the purpose of the training is to get the level 1 out of the way there will be little eyepiece time. If, after all of the training is finished, there may be some eyepiece time but please do not count on it. Patrick
--- Patrick Wiggins <paw@trilobyte.net> wrote:
Not to be a grinch, but please note that it will not be a star party night either. The evening will be used for training only. And being that the purpose of the training is to get the level 1 out of the way there will be little eyepiece time.
No one was suggesting otherwise. But if you are going to drive 80 miles roundtrip, one might as well point the scope at something during training. - Best regards - C __________________________________________________ Do You Yahoo!? Tired of spam? Yahoo! Mail has the best spam protection around http://mail.yahoo.com
Have you signed up for either of the refractor classes? I just checked and did not see "canopus56@yahoo.com" listed. Patrick Canopus56 wrote:
--- Patrick Wiggins <paw@trilobyte.net> wrote:
Not to be a grinch, but please note that it will not be a star party night either. The evening will be used for training only. And being that the purpose of the training is to get the level 1 out of the way there will be little eyepiece time.
No one was suggesting otherwise. But if you are going to drive 80 miles roundtrip, one might as well point the scope at something during training. - Best regards - C
-- Patrick Wiggins <paw@trilobyte.net> wrote:
Have you signed up for either of the refractor classes? I just checked and did not see "canopus56@yahoo.com" listed. Patrick
Yes, under my personal identity. I use the aliased identity canopus56 for public newsgroup communications to reduce the possibility of identity theft. I have sent you an offline confirmation. Canopus56 (Kurt) __________________________________________________ Do You Yahoo!? Tired of spam? Yahoo! Mail has the best spam protection around http://mail.yahoo.com
Quoting *******56 <*******56@yahoo.com>:
I use the aliased identity ******* public newsgroup communications to reduce the possibility of identity theft. I have sent you an offline confirmation. ******56 (****)
You can run, but you can't hide. We know who you are! ;)
--- diveboss@xmission.com wrote:
You can run, but you can't hide. We know who you are! ;)
Alright already, you can have my wallet. -:) Canopus56(Kurt) http://www.utahastronomy.com/view_photo.php?set_albumName=diveboss&id=Cat_bu... __________________________________________________ Do You Yahoo!? Tired of spam? Yahoo! Mail has the best spam protection around http://mail.yahoo.com
--- diveboss@xmission.com wrote:
Quoting *******56 <*******56@yahoo.com>: You can run, but you can't hide. We know who you are! ;)
http://www.utahastronomy.com/view_photo.php?set_albumName=diveboss&id=Cat_bu... P.S. - Just leave the scope, man, just don't take the scope. -:) C __________________________________________________ Do You Yahoo!? Tired of spam? Yahoo! Mail has the best spam protection around http://mail.yahoo.com
--- Patrick Wiggins <paw@trilobyte.net> wrote: <snip all> Patrick, to the extent there has been any miscommunication as to intent behind this thread, I apologize. - Kurt __________________________________________________ Do You Yahoo!? Tired of spam? Yahoo! Mail has the best spam protection around http://mail.yahoo.com
Canopus56 wrote:
Patrick, to the extent there has been any miscommunication as to intent behind this thread, I apologize. - Kurt
Thanks, but no worries and nothing to apologize for. But as long as I have everyone's attention, here's a great picture I just received. Nothing to do with astronomy. More with aerodynamics. And, yes, the picture is real. http://www.trilobyte.net/paw/temp/FALCON.JPG Patrick
participants (3)
-
Canopus56 -
diveboss@xmission.com -
Patrick Wiggins