2010-02-14 Pluto occultation
From SwRI
Overview
Bruno Sicardy is leading an effort to observe this event from many sites in Europe. Please see his web page here: http://www.lesia.obspm.fr/perso/bruno-sicardy/14_feb_10/
Contents |
Contacts
- List of contacts are here: Contacts
PHOT Observers
Definitely available
- Cathy Olkin (prefers Switzerland)
- Harold Reitsema (prefers France)
- Eliot Young
- Leslie Young (prefers France)
- Larry Wasserman
Interested, uncommitted
Definitely unavailable
- Marc Buie
- Henry Roe
- Peter Tamblyn
- John Spencer
- Amanda Gulbis
- Dick French
- Jeff Regester
- John Stansberry
Contacted, not yet heard from
- Bob Howell
- Kevin Shoemaker
Not yet contacted
- Bobby Bus
- Bob Millis
Paris-Meudon and European Observers
Definitely available
- Bruno Sicardy (prefers Catania)
- Thomas Widemann (Cagliari or Vienna)
- François Colas
- Jean Lecacheux
- Jean-Eudes Arlot (prefers Castel Gandolfo)
- Françoise Roques
- Olivier Mousis
- Mirel Birlan
Switzerland :
- Raoul Behrend (prefers St Luc)
- Frédéric Malman (St Luc)
- Stefano Sposett
Italy/Vatican :
- P. David Brown S.J.
- Claudio Costa
Germany :
- Wolfgang Beisker
- Claus-Peter Heidmann
Spain :
- Jose-Luis Ortiz (Calar Alto)
- Carles Schnabel (Baleares)
- Ricard Casas (Sabadell)
==
Available Instruments
In the US, we have carnets already for the following cameras:
- Ansel (MicroMax). Can mount into 2"eyepiece holder. Will need to be pumped down.
- Walker (MicroMax).Can mount into 2"eyepiece holder.Will need to be pumped down.
- Eadweard (PhotonMax). Will probably need a mounting plate.
- Doc (PhotonMax).Will probably need a mounting plate.
- Gjon (PhotonMax). Will need work on front-mounting screws.Will probably need a mounting plate.
PhotonMax cameras are mounted with mounting plates. The front faces come off, as seen here: http://www.boulder.swri.edu/~layoung/projects/PHOT/20060130_opticslab/P1010073.JPG. The drawings are here: http://www.boulder.swri.edu/~layoung/projects/PHOT/drawings/. We have plates of different sizes that attach to the front of the camera and have the right holes drilled to match a bolt pattern.
Meudon has 5 EMCCD cameras, 2 IR cameras, and several WATEC 120N+.
IOTA-ES (Germany) up to 5 Iota Occultation Cameras, QHY6 cameras, Watecs etc.
Site Summary
| Vatican | Site | Aperture | Time Allocated | Instrumentation | Observers | Notes | |||||
| Castel Gandolfo | 0.61 | ? | ? | Arlot? Costa? | |||||||
| Italy | Site | Aperture | Time Allocated | Instrumentation | Observers | Notes | |||||
| Catania Obs, Sicily | .91m, .8m (brand new), .61m | Yes | Meudon cams + aperture photometer? | B. Sicardy, F. Roques | - | ||||||
| Teramo | .72m (?) | Not possible, elevation too low. | Meudon cams | Olivier Mousis, Daniel Cordier, Philippe Rousselot | Near l'Aquila's 2009 Earthquake site. Ideally situated in the Appenins range as a base for mobile stations. | ||||||
| Mousis Portable | 0.35 | N/A | Meudon cams | O. Mousis, D. Cordier, Ph. Rousselot | Based in Teramo | ||||||
| Beisker Portable | 0.279 | N/A | QHY6 + IOTA | Wolfgang Beisker | Based somwhere in Italy/Suisse according to weather conditions | ||||||
| Costa Portable | 0.35 | N/A | ? | Claudio Costa in contact/coordination with amateurs in Italy | |||||||
| Loiano, 35 km south of Bologna | 1.52, .6 | Yes | Wasserman | PHOT-Eadweard | Complementary site, distant from others | ||||||
| Arectri, near Firenze | no info on web page | Tozzi contacted by B. Sicardy Jan 17: old 37cm refractor not usable, but 3 C14 available there | ? | ? | ? | ||||||
| Capodimonte, near Naples, Italy | 1.51, 0.6 | Yes | Olkin | PHOT-Gjon | Altitude limits uncertain | ||||||
| Campo Imperatore | 1.08 | ? | SWIRCAM (1.1 - 2.5 μm ), facility instr. | ? | property of Obs. Pulkovo | ||||||
| Cagliari, Sardinia | .42 | Prof. Nicolò D'Amico and Ignazio Porceddu contacted, allocation OK. Marco Massa and amateur group also contacted and will participate. | Meudon camera (e.g. Watec) | Inappropriate light pollution at SE | Facility instrument of INAF's Osservatorio Astronomico di Cagliari (OAC). Oil refinery in SE direction. | ||||||
| Max Valier (Bolzano) | 0.8 | Not possible due to elevation (min. 19 deg) | ? | ||||||||
| Val d'Aosta | 0.8, 0.4, 0.25, 0.25, 0.12 | contact: A. Carbognani. Telescopes can be pointed to 7.5 deg. elev.. We are welcome to use that site | ? | ||||||||
| Switzerland | Site | Aperture | Time Allocated | Instrumentation | Observers | Notes | |||||
| Jungfraujoch | .76 | LIDAR at the Cass focus, but Valentin Simeonov might agree to help us put a camera at the Cass focus. Pluto's azimuth at 135-deg appears to miss the Monch and Jungfrau. We'll need the adapter plate pattern from Marcel Bartlome | ? | ? | Lidar may prevent other instruments | ||||||
| Gornergrat | 1.5 | No chance. S. dome has a submm scope, and the 1.5-m in the N. dome no longer there. | Facility? | ||||||||
| St Luc | 0.6m | Yes | PHOT-Walker | Reitsema, Behrend, Malman | Snout | ||||||
| Bellinzona | 0.4m | Sposetti contacted | Sposetti | ||||||||
| Falera | 0.9m | Yes | Cathy, Larry? | ||||||||
| Jura | 0.61 | ||||||||||
| Monte Generoso | 0.61 | No | - | - | Closed until March 19 | ||||||
| Zimmerwald | 1.0 | ||||||||||
| Geneva | 0.7 | ||||||||||
| Austria | Site | Aperture | Time Allocated | Instrumentation | Observers | Notes | |||||
| Vienna | .51, .68, .80 | ||||||||||
| Leopold Figl | 0.6, 1.5 | Werner W. Zeilinger contacted. Time allocated including Feb.12-13. | PHOT-Ansel | EYoung | Was Widemann w/ possibly Watec | ||||||
| France | Site | Aperture | Time Allocated | Instrumentation | Observers | Notes | |||||
| Haute Provence | .80 (1.93?) | yes for .80 | PHOT-Doc | LYoung | Mount TBD | ||||||
| Puimichel | 1.0 | not yet contacted | ? | ? | 1 hour from OHP, amateur. | ||||||
| Pic du Midi | .55,.6,1.06,2 | ? | ? | ||||||||
| Nice | |||||||||||
| Saint Veran (AstroQueyra) | .62 | Difficult, no set-up | a team is going at St Veran on Saturday night (Feb. 13) for another run | ||||||||
| Czech Republic | Site | Aperture | Time Allocated | Instrumentation | Observers | Notes | |||||
| Ondřejov | 0.65, 2 | ? | ? | ||||||||
| Bulgaria | Site | Aperture | Time Allocated | Instrumentation | Observers | Notes | |||||
| Rozhen | 2, 0.6 | 2m available with aperture photometer, 0.6m available for Meudon IR camera | |||||||||
| Belogradchik | 0.6 | available, with aperture photometer | |||||||||
| Croatia | Site | Aperture | Time Allocated | Instrumentation | Observers | Notes | |||||
| Hvar | 1.0 | ||||||||||
| Slovenia | Site | Aperture | Time Allocated | Instrumentation | Observers | Notes | |||||
| Crni Vrh | 0.6 | EU member, Schengen | |||||||||
| Greece | Site | Aperture | Time Allocated | Instrumentation | Observers | Notes | |||||
| Skinakas, Crete | 1.1 | No | n/a | n/a | 1.3m out of service (rewiring) | ||||||
| Skinakas, Crete | 0.6 | Capella Obs. contacted by Bruno Jan 21 | n/a | 0.6m out of service (snow) | |||||||
| Chelmos, Greece | 2.3 | Access issues (snow) | Facility SITe 1K x 1K CCD with UBVRI, 1 Hz | Facility | Use if only Greece looks clear? | ||||||
| Kryoneri, Greece | 1.2 | n/a | n/a | n/a | Drive problems - don't use | ||||||
| Spain | Site | Aperture | Time Allocated | Instrumentation | Observers | Notes | |||||
| Calar Alto | ??? | JL Ortiz | |||||||||
| Baleares | ??? | Carles Schnabel | |||||||||
| Sabadell | ??? | Ricard Casas | |||||||||
| Pico Veleta | No | ??? | Too low | ||||||||
| Germany | Site | Aperture | Time Allocated | Instrumentation | Observers | Notes | |||||
| VSW Munich | 0.8m | YES | IOC or QHY6 tbd | CPHeidmann | |||||||
| Hoher List | 0.6m 0.35 | YES | WATEC Cameras, GPS time | Geffert, Brednet | |||||||
| Finland | Site | Aperture | Time Allocated | Instrumentation | Observers | Notes | |||||
| Nyrölä Observatory | 0.4m Meade | To be contacted | ST-8XE CCD | Sirius ry | |||||||
| Tunisia | Site | Aperture | Time Allocated | Instrumentation | Observers | Notes | |||||
| Observatoire Astronomique Néapolis du Club Jeunes Sciences de Nabeul | ? | Thomas emailed, Jan 31 | No telescope beyond suburban Tunis. A C14 and C11 owned by the weather service in Tunis would require heavy paperwork to be made available | ||||||||
Photometry and SNR
Predictions
Star Prediction Summary
With no proper motions applied to the catalog stars, the dec offsets are all similar.
Source RA Dec dra ddec errx erry ------------------------ -------------- ------------- ----- ------- ---- ---- Brazil 18:19:14.3847 -18:16:42.323 0 0 35 35 Lowell 18:19:14.3779 -18:16:42.320 -97 3 62 34 Tycho-2-noPM 18:19:14.3774 -18:16:42.379 -103 -56 104 146 PPMX-noPM 18:19:14.3848 -18:16:42.331 1 -8 15 19 UCAC3-noPM 18:19:14.3774 -18:16:42.338 -103 -15 16 16 2MASS-noPM 18:19:14.3848 -18:16:42.310 1 13 60 60 ------------------------------------------------
Ephemeris Correction Summary
Globes and Ground Tracks
Finding Charts
There is a good comparison star 1.9464 arcmin (117 arcsec) away (18 19 06.181, -18 16 45.34) is a conparison star with I=10.255, J=8.568, K=7.135. DENIS3 J181906.1-181645
Test Stars and Setup Stars
Wolfgang Beisker
Wolfgang Beisker writes "Dear all, I have selected some test stars with (almost) same altitude, azimuth, magnitude and color as the star to be occulted. This may be useful for testing the event. Because most (or all?) of you do not want to observe at 4h50 in the morning, the stars have been selected, that they can be observed in the first half of the night. Keep in mind to compensate the observation time for the date you observe. Please have a look at http://www.iota-es.de/pluto-test.html"
Leslie Young: I've copied his information here, and added Star Numbers - WB for Wolfgan Beisker'
Test Stars with same altitude, azimuth, magnitude and color In order to test equipment, telescope, positioning etc. A few test stars have been selected. The stars have for certain times the same altitude, azimuth, magnitude and color as the star to be occulted. In the following table the observing time, UCAC number, RA, Dec, spectral type UCAC magnitude, J, H, and K mag are given.
The first 3 stars are easy to find, they are only a little more than 1 degree away from Sirius. For a rough check for these observing time, Sirius may be a good choice, if anybody wants to see, what the horizon is etc.
NUM m/d hh_mm UCAC # RA Dec SpT UCACmag Jmag Hmag Kmag WB1 1/30 18h20 25023103 06:49:39.18 -17:30:10.9 M6 10.60 7.346 6.378 6.085 WB2 1/30 18h20 24775642 06:45:47,49 -18:02:39.0 M2 10.80 7.883 6.948 6.652 WB3 1/30 18h20 24775522 06:45;22.30 -18:05:40.3 M0 10.32 7.720 6.889 6.629 WB4 1/30 20h00 24572423 08:30:38.22 -18:34:07.5 M0 10.23 7.656 6.861 6.580 WB5 1/30 20h00 24819457 08:34:37.87 -18:08:51.6 M0 10.92 7.728 6.835 6.518 WB6 1/30 20h00 24572586 08:31:21.43 -18:49:15.9 M0 10.33 7.305 6.464 6.202 WB7 1/30 23h15 24839049 11:46:15 -18:13:18 M0 10.36 8.059 7.017 7.264
The same altitude and azimuth is valid on the 15th of January 1h later and on the 14th of February 1h earlier.
The times are only approximate times for the same altitude and azimuth, calculate it exact for your circumstances.
The data have been extracted from UCAC2 catalog as well as from 2MASS catalog.
Larry Wasserman
From: "Lawrence H. Wasserman" <lhw@lowell.edu> Date: Fri, 05 Feb 2010 14:00:35 -0700
Leslie --
If you have a computer controlled telescope to work with and you're not sure of its pointing accuracy, here is a list of stars which more-or-less decrease in brightness and get progressively closer to the target and with which you can presumably "walk" to the target.
Leslie Young: I've copied his information here, and added Star Numbers - LW for Larry Wasserman'
NUM PPM V RA Dec Dist (deg) SAO LW1 168779 0.80 19:50:47.4 +08:52:10 35.32 (Altair) LW2 164476 2.80 17:43:28.3 +04:34:04 24.49 LW3 201263 3.30 17:59:01.6 -09:46:26 9.81 LW4 234600 4.70 18:29:11.9 -14:33:57 4.41 LW5 234421 5.90 18:21:23.0 -18:51:36 0.77 161376 LW6 234323 7.10 18:18:22.7 -18:28:32 0.28 161294 LW7 Occln Star 18:19:14.4 -18:16:42.3
Here are finder charts from Aladin previewer for selected stars
Leslie Young
Here are bright stars roughly every 1/2 hour of RA or closer, and similar declinations to the occulted star, for practicing pointing all night long.
I am adding SAO numbers for selected stars because that is what we need for pointing (Cathy).
NUM RA_J2000 Dec_J2000 HR Vmag LY01 06:45:08.9 -16:42:58 2491 -1.49 LY02 07:22:13.5 -19:01:00 2812 4.96 LY03 07:59:52.0 -18:23:57 3131 4.61 LY04 08:09:01.6 -19:14:42 3192 4.40 LY05 08:21:54.6 -17:35:11 3281 5.75 LY06 08:55:12.4 -18:14:29 3554 5.75 LY07 09:09:04.3 -18:19:43 3638 5.73 LY08 09:54:52.2 -19:00:34 3923 4.94 LY09 10:04:02.9 -18:06:06 3963 5.86 LY10 10:46:52.0 -17:17:48 4214 5.42 LY11 10:59:46.5 -18:17:56 4287 4.08 LY12 11:24:52.9 -17:41:02 4405 4.08 LY13 11:44:45.8 -18:21:03 4514 4.73 LY14 12:15:48.4 -17:32:31 4662 2.59 LY15 12:29:51.9 -16:30:56 4757 2.95 LY16 13:18:24.3 -18:18:41 5019 4.74 LY17 13:49:52.3 -18:08:03 5196 4.97 LY18 14:15:24.1 -18:12:03 5332 5.43 LY19 14:18:38.3 -18:42:58 5355 5.90 158481 LY19a 15:12:13 -19:47:31 5652 4.54 159090 LY20 16:05:26.2 -19:48:20 5984 2.62 159682 LY21 16:27:01.4 -18:27:23 6118 4.42 LY22 16:41:34.4 -17:44:32 6196 4.96 160046 LY23 17:08:14.9 -17:36:33 6365 5.99 160305 LY24 18:17:11.6 -17:22:26 6838 5.75
Here are finder charts from Aladin previewer for selected stars
Maps
- Google map
- Bruno's longitude-latitude map The longitude-latitude map gives the iso-elevation lines for the Sun (limits of gray zones), the iso-elevation lines for Pluto (in green), the path of center line and half-light line (blue solid lines), and the 1% drop stellar line (in blue dotted), marking the practical limit of detection of the occultation. Enlargement
Schedule
PHOT packing list
Pluto2010-02-14 PHOT packing list
Boulder Cameras
Picture of both cameras and the electronics box http://www.boulder.swri.edu/~layoung/projects/PHOT/20060130_opticslab/P1010064.JPG
Manuals http://www.boulder.swri.edu/~layoung/projects/PHOT/manuals/
MicroMax
The MicroMax camera head (rectangular camera head, C-Mount) weighs 7.25 pounds and is 4.63 inches x 4.63 inchesx 7.05 inches. The focal plane 0.690 inches from front face, with the center of mass is 4.24 inches from front face.
The MicroMax electronics box (ST-133A) is 10 pounds, 8.75 inch high by 5.25 inch wide by 13.63 inch long.
The MicroMax acquisition laptop weighs 5 pounds.
The electronics box to camera cable is 125.5 inches long.
Photos of MicroMax or Micromax mounts. The holes on the optics bench are spaced by 1 inch.
dark = dark0 * exp( (T - T0)/S)
Walker Ansel
T0 -45 C -45 C
dark0 1.7 e/s 3.7 e/s
S 4.8 C 5.9 C
PhotonMax
Photos of PhotonMax or PhotonMax mounts. The holes on the optics bench are spaced by 1 inch.
General Guidelines
Links
- Translation of phrases and URLs http://www.google.com/translate_t?sl=it&tl=en&hl=en&text=specola&source=dictionary#
- Clickable weather statistics http://en.allmetsat.com/climate/europe.php
- Weatherforecast for Italy link: http://www.meteoam.it/
