Planetary Imaging Campaign 2016

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1 Planetary Imaging Campaign 2016 Contributing to MissionJUNO and other online databases PACA_Mars, PACA_Jupiter, PACA_SaturnSolstice, hstjupiter, ALPO Trevor Barry Phil Miles Anthony Wesley

2 Planetary Imaging Campaign 2016 Objectives - Tracking long and short lived spatial features on Jupiter, Mars and Saturn using modern hardware and high resolution imaging techniques. - Detecting seasonal changes in colouration and visible features on Jupiter / Mars / Saturn. - Detecting transient events Jovian bolides Mars high altitude cloud Saturn ring features (spokes etc) New things...!

3 Equipment Trevor Barry Custom design newtonian telescopes Fast cooling / unpainted Aluminium tube for optimal thermal performance Peltier cooling / thin mirror design optimised for planetary imaging

4 Composite construction fast cooling 508mm primary mirror (Phil Miles)

5 Camera The GS3-U3-32S4M from Canadian manufacturer Point Grey Research Sensor: Sony CMOS IMX252 (Q4 2015) High QE in visible and NIR, good response up to 900nm. Very low noise when using optimised imaging mode 7 Video Mode 0 Video Mode 7 Pixel Clock (MHz) ADC (Bits) 10-bit 12-bit Quantum Efficiency (% at 525 nm) Temporal Dark Noise (Read Noise) (e-) Signal to Noise Ratio Maximum (db) Signal to Noise Ratio Maximum (Bits) Absolute Sensitivity Threshold (γ) Saturation Capacity (Well Depth) (e-) Dynamic Range (db) Dynamic Range (Bits) Gain (e-/adu)

6 Jupiter, Mars and Saturn are all southern hemisphere targets for the next 5 years at least. MARS has southerly oppositions in 2016, 2018 and 2020 with angular sizes exceeding 20 arc seconds. JUPITER will be in the southern sky until 2021 SATURN will be in the southern sky until 2027 This is the best opportunity for a southern-hemisphere focused campaign covering all three planets, a grouping that will not be repeated in our lifetime for observers based in Australia. In particular this has implications for high resolution imagery of Jupiter during the JUNO mission timescale. Given reasonable seeing conditions, there will be a steady stream of good, high resolution images of Jupiter from observers in the southern hemisphere.

7 Resolution is high enough to see detail on Jupiters moons, Even Callisto which is the darkest and most difficult to see.

8 Contributing to MissionJUNO - In 2014 there was a meeting between Glenn Orton (Pro/Am coordinator for JUNO) and Anthony Wesley where a preliminary outline was created for extending the WinJupos software to create standardised datasets from amateur data in a form suitable for integrating into the MissionJUNO website. - Thanks to the WinJupos team (Grischa Hahn et.al) this functionality is now available and being used to package amateur images and metadata in a standardised format that is usable to the JUNO team. - It can be hoped that this is a way forward for better integration between amateurs and professionals for future missions, WinJupos is a natural place for this integration to happen.

9 Contributing to MissionJUNO Amateur observers measure their image in WinJupos to determine metadata such as size and orientation etc. The Create Transmission Package option is used to create a ZIP file containing the image and metadata in a generic XML format that can be used programmatically. This ZIP file can then be uploaded to the MissionJUNO website.

10 Recent images: March 2016 White Spot Z in the NTrZ The GRS and complex wake

11 Recent Images: March 2016 Oval BA and associated disturbance

12 Recent Images: April 2016 Methane band (889/18) image showing the GRS wake and Oval BA Modern cameras have more sensitivity in the IR band 750nm 900nm in addition to lower noise

13 Recent Images: April 2016 Oval BA setting, followed by complex chain of dark spots and storms

14 Recent Images: Feb 2016 Animation showing relative rotation interior to the GRS over nearly 2 hours Images are from GRS rising and GRS setting. Also visible are relative movements in the jet streams at various latitudes.

15 Recent Images: April arc seconds Phil Miles using his 508mm Fullum Air Tech mirror (fast cooling)

16 Recent Images: April arc seconds Anthony Wesley, 406mm fast-cooling composite mirror

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