Remote observatory ISON-NM Survey of Minor Solar System bodies L. Elenin¹, I. Molotov¹, V. Savanevich², A. Kozhukhov³, A. Bryukhovetskiy³, V. Vlasenko³,

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Presentation transcript:

Remote observatory ISON-NM Survey of Minor Solar System bodies L. Elenin¹, I. Molotov¹, V. Savanevich², A. Kozhukhov³, A. Bryukhovetskiy³, V. Vlasenko³, E. Dikov⁴, A. Yudin¹ ¹ Keldysh Institute of Applied Mathematics RAS (Russia) ² Kharkiv National University of Radioelectronics (Ukraine) ³ National Centre of Space Devices Control and Test (Ukraine) ⁴ Recearch and Design Institute of Micrography (Ukraine) Asteroids, Comets, Meteors 2012, Niigata, Japan

Location ISON-NM Observatory (H15) Coordinates: 32° 54′ 11.79″ N 105° 31′ 42.40″ W 2217 above sea level Asteroids, Comets, Meteors 2012, Niigata, Japan NMSkies astrohosting

Location Why NMSkies? Astroclimate - Many clear nights ( per year) - Dark skies (SQM ~ 22.1 mag/arcsec²) First light only in 5 month - Ready infrastructure (fast Internet) - Experienced support for remote observations Asteroids, Comets, Meteors 2012, Niigata, Japan

Telescope Asteroids, Comets, Meteors 2012, Niigata, Japan Centurion-18 Aperture – 455 mm Focus lenght – 1270 mm Focal ratio – f/2.8 CCD – FLI ML FOV – 100’x100’ Image scale – 1.95”/pix No filter wheel

Main tasks on ISON-NM 1. Survey for a new Solar System objects, include near-Earth objects 2. Follow-up observations of NEA and comets 3. NEAs photometry 4. Optical transients observation, include working with VOEvent 4.1 Gamma-ray bursts 4.2 Supernovae 4.3 Novae 4.4 Cataclysmic variables stars and other transients 5. Supernovae survey* 6. Patrol of cataclysmic variables stars* 7. Photometry of variable stars on survey's images* * - as by-product, this plans for the near future Asteroids, Comets, Meteors 2012, Niigata, Japan

ACPACPSVOEvent Observation program MaximDL TheSky 6 FocusMax Clarity II Asteroids, Comets, Meteors 2012, Niigata, Japan Observatory control CCD FLI ML09000 Mount TCS-4000 Focuser Robofocus Cloud sensor Boltwood II Ethernet power controller PC 2

Images processing pipeline - CLT Asteroids, Comets, Meteors 2012, Niigata, Japan CCD Calibration Cosmetic correction Pre- processing Moving object detection Operator (reject false detections) MPC … Clone n

Minor Planet Center statictics Observatory Number of observations Numbered asteroids Unnumbered asteroids 1Mt. Lemmon Survey (G96) Lincoln Laboratory ETS (704) Catalina Sky Survey (703) Pan-STARRS 1 (F51) Steward Observatory (691) Siding Spring Survey (E12) Purple Mountain Observatory (D29) ISON-NM Observatory (H15) Črni Vrh Observatory (106) LPL/Spacewatch II (291) Overall statistics for 2011 year Asteroids, Comets, Meteors 2012, Niigata, Japan

Minor Planet Center statictic Observatory Number of observations Numbered asteroids Unnumbered asteroids 1Pan-STARRS 1 (F51) Catalina Sky Survey (703) Mt. Lemmon Survey (G96) Lincoln Laboratory ETS (704) Steward Observatory (691) ISON-NM Observatory (H15) Črni Vrh Observatory (106) Oukaïmeden Observatory (J43) Les Engarouines Observatory (A14) Siding Spring Survey (E12) Statistics for January - March 2012 Asteroids, Comets, Meteors 2012, Niigata, Japan

Statistics of residuals Observatory R.A. (arcsec) Decl. (arcsec) 1Mt. Lemmon Survey / / Lincoln Laboratory ETS / / Catalina Sky Survey / / Pan-STARRS / / Steward Observatory / / Siding Spring Survey / / Purple Mountain Observatory / / ISON-NM Observatory / / Črni Vrh Observatory / / LPL/Spacewatch II / / Asteroids, Comets, Meteors 2012, Niigata, Japan Data for October 2011

Results of our survey program Obtained more than observations Discovered more than 1000 MBA (provisional designation) Two near-Earth asteroids 2010 RN80 and 2011 QY37 (Amors) Long-period comet C/2010 X1 (Elenin) Short-period near-Earth (q=1.24) comet P/2011 NO1 (Elenin) Several Jovian trojans Asteroids, Comets, Meteors 2012, Niigata, Japan Dust cloud - the debris of the comet C/2010 X1 ©Rolando Ligustri

NEAs photometry Asteroids, Comets, Meteors 2012, Niigata, Japan Rotation period — 17 min 40 sec All data processed in MPO Canopus software. Thanks to Dr. Warner!

Promising survey telescope Asteroids, Comets, Meteors 2012, Niigata, Japan Aperture, mm600 Focal ratiof/2.17 Angular field diameter, degrees4 Linear field diameter, mm52.4 Spectral range, nm Back focal length, mm159 Central obscuration ratio0.33 Relative illum. on the edge of FOV0.83 Distortion, %0.14 Optical system's length, mm1344

Plans for the future Improving CoLiTec pipeline — ability to detection more faint and fast moving objects, decreasing processing time (CUDA) Replacing our C-18 on new survey 0.65-m f/2.0 telescope: more «deeper» survey with larger sky coverage Extracting more by-products from the survey's images Work in progress... Asteroids, Comets, Meteors 2012, Niigata, Japan

Thank you! Leonid Elenin Asteroids, Comets, Meteors 2012, Niigata, Japan