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Controlled Mosaic of Enceladus Hamah Sulci Se 400K 43.5/315 CMN, 2018 GENERAL NOTES 66° 360° West This map sheet is the 5th of a 15-quadrangle series covering the entire surface of Enceladus at a 66° nominal scale of 1: 400 000. This map series is the third version of the Enceladus atlas and 1 270° West supersedes the release from 2010 . The source of map data was the Cassini imaging experiment (Porco et al., 2004)2. Cassini-Huygens is a joint NASA/ESA/ASI mission to explore the Saturnian 350° system. The Cassini spacecraft is the first spacecraft studying the Saturnian system of rings and 280° moons from orbit; it entered Saturnian orbit on July 1st, 2004. The Cassini orbiter has 12 instruments. One of them is the Cassini Imaging Science Subsystem 340° (ISS), consisting of two framing cameras. The narrow angle camera is a reflecting telescope with 290° a focal length of 2000 mm and a field of view of 0.35 degrees. The wide angle camera is a refractor Samad with a focal length of 200 mm and a field of view of 3.5 degrees. Each camera is equipped with a 330° 300° large number of spectral filters which, taken together, span the electromagnetic spectrum from 0.2 60° 320° 310° to 1.1 micrometers. At the heart of each camera is a charged coupled device (CCD) detector 60° consisting of a 1024 square array of pixels, each 12 microns on a side. MAP SHEET DESIGNATION Peri-Banu Se Enceladus (Saturnian satellite) 400K Scale 1 : 400 000 43.5/315 Center point in degrees consisting of latitude/west longitude CMN Controlled Mosaic with Nomenclature Duban 2018 Year of publication IMAGE PROCESSING3 Julnar Ahmad - Radiometric correction of the images - Creation of a dense tie point network 50° - Multiple least-square bundle adjustments 50° - Ortho-image mosaicking Yunan CONTROL For the Cassini mission, spacecraft position and camera pointing data are available in the form of SPICE kernels. SPICE is a data system providing ancillary data such as spacecraft and target Hisham positions, target body size/shape/orientation, spacecraft orientation, and instrument pointing, which is used for planning space science missions and recovering the full value of science instrument data returned from missions (http://naif.jpl.nasa.gov/). A 3-D control network was set up to correct errors in the nominal camera pointing data. The network utilized all images in the Cassini ISS CLR (effective wavelength λe = 651 nm), GRN (λe = 569 nm), IR3 (λe = 928 nm), and UV3 (λe = 343 nm) filters with a pixel scale between 50 and 500 m/pixel and a phase angle less than 120°: a total of 586 images. The control network consisted of 10,362 tie points and 173,704 individual image measures, averaging nearly 17 measures per 40° tie point. Least squares bundle adjustment resulted in a root mean square (rms) residual of 0.45 40° pixels, corresponding to rms ground point uncertainties of 66 m, 51 m, and 46 m in latitude, longitude, and radius, respectively. The bundle solution yielded independently determined shape information, resulting in radii (a, b, c axis) slight smaller than, but within the stated uncertainty of, IAU values, and a 0.769° shift in the prime meridian offset (W0). Using this geodetic control network, Fitnah updated pointing kernels for every image were calculated, substantially improving image locations. Additionally, a new global mosaic of Enceladus using the best available data from the mission was created. The longitude system according to Davies and Katayama (1983)4 and adopted by the IAU/IAG (International Astronomical Union/International Association of Geodesy) Working Group on Cartographic Coordinates and Rotational Elements as standard (Archinal et al., 2018)5 is defined A by crater Salih at 5° west. Ghanim S MAP PROJECTION S Lambert conic conformal projection with two standard parallels at 58°N and 30°N 30° O HARRAN Scale is true at 58°N and 30°N SULCI 30° F Adopted figure: sphere Mean radius: 252.1 km Ayyub Grid system: planetographic latitude, west longitude R Ja‘afar I Marjanah NOMENCLATURE N Names are suggested by the ISS-Camera-Team and approved by the International Astronomical A Union (IAU). For a complete list of IAU-approved names on Enceladus, see the Gazetter of Planetary Nomenclature at http://planetarynames.wr.usgs.gov/. B Al-Fakik S REFERENCES I 1 Roatsch, Th., Kersten, E., Hoffmeister, A., Wählisch, M., Matz, K.-D., Porco, C.C., 2013, Recent 21° improvements of the Saturnian satellites atlases: Mimas, Enceladus, and Dione, Planetary and H 21° Space Science, 77, 118-125. 360° West A 2 I Porco, C.C., West, R.A., Squyres, S., McEwen, A., Thomas, P.C., Murray, C.D., DelGenio, J.A., M C 270° West Ingersoll, A.P., Johnson, T.V., Neukum, G., Veverka, J., Dones, L., Brahic, A., Burns, J.A., Haemmerle, L V., Knowles, B., Dawson, D., Roatsch, Th., Beurle, K., Owen, W., 2004, Cassini Imaging Science: A U Instrument Characteristics and Anticipated Scientific Investigations at Saturn, Space Science Review, 115, 363-497. S H 3 Bland, M.T., Becker, T.L., Edmundson, K.L., Patterson, G.W., Roatsch, Th., Takir, D., Collins, G.C., Pappalardo, R.T., Schenk, P.M., Hare, T.M., A new Enceladus global control network, image mosaic, and updated pointing kernels from Cassini’s thirteen-year mission, submitted to Earth and 350° 280° Space Science. 4 Davies, M.E. and Katayama, F.Y., 1983, The Control Networks of Mimas and Enceladus, Icarus, 53, 332-340. 5 Archinal, B.A., Acton, C.H., A’Hearn, M.F., Conrad, A., Consolmagno, G.J., Duxbury, T., Hestroffer, D., Hilton, J.L., Kirk, R.L., Klioner, S.A., McCarthy, D., Meech, K., Oberst, J., Ping, J., Seidelmann, 340° P.K., Tholen, D.J., Thomas, P.C., Williams, I.P., 2018, Report of the IAU Working Group on Cartogra- 290° SAMARKAND SULCI phic Coordinates and Rotational Elements: 2015, Celestial Mechanics and Dynamical Astronomy, 130, 3, 22. SARANDIB PLANITIA Image processing (USGS): Becker, T.L., Bland, M.T. 330° 300° Scale 1:400 000 Cartographic production and design (DLR): Kersten, E., Wählisch, M. 320° 310° 0 10 20 30 40 km EDITOR German Aerospace Center (DLR), Institute of Planetary Research, Roatsch, Th. Please send comments, suggestions, and questions to [email protected]. Index map Se-1 Index of Cassini images Resolution of the images Sindbad Se-5 Se-4 Se-3 Se-2 60° Hamah Sulci Shahrazad Kasim Ali Baba 66° 66° 60° 60° m/px 44 95 20 1 N1487299402 30° 400 - 500 2 N1487299578 50° 108 106 4 N1487300285 50° Se-10 Se-9 Se-8 Se-7 Se-6 1 5 N1487300482 300 - 400 Aziz Ebony Dorsum Khusrau Bulak Sulcus Salih 15 N1489048550 44 21 40° 20 N1489049580 40° 200 - 300 21 N1489049756 83 5 360° 330° 300° 270° 240° 210° 180° 150° 120° 90° 60° 30° 0° 44 N1584039815 15 150 - 200 0° 45 N1584039961 30° 66 N1637469285 30° 107 1 82 N1660436067 100 - 150 82 2 83 N1660436242 21° 95 N1696175570 21° 50 - 100 106 N1858920340 1 360° W 66 45 107 N1858921090 Se-14 Se-13 Se-12 Se-11 108 N1858923093 est 270° West <50 -30° Kamar Cashmere Sulci Hassan Otbah 350° 4 280° 340° 290° Phase angle 120° 330° 300° 320° 310° Incidence angle 87° Emission angle 80° -60° Se-15 Damascus Sulcus Se 400K 43.5/315 CMN, 2018 Se-5.
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