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Hi-Resolution Map Sheet Controlled Mosaic of Enceladus Salih Se 400K 0/36 CMN, 2018 GENERAL NOTES This map sheet is the 6th of a 15-quadrangle series covering the entire surface of Enceladus at a nominal scale of 1: 400 000. This map series is the third version of the Enceladus atlas and supersedes the release from 20101. 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 system. The Cassini spacecraft is the first spacecraft studying the Saturnian system of rings and moons from orbit; it entered Saturnian orbit on July 1st, 2004. 72° West 60° 50° 40° 30° 20° 10° 0° West The Cassini orbiter has 12 instruments. One of them is the Cassini Imaging Science Subsystem 22° 22° (ISS), consisting of two framing cameras. The narrow angle camera is a reflecting telescope with a focal length of 2000 mm and a field of view of 0.35 degrees. The wide angle camera is a refractor with a focal length of 200 mm and a field of view of 3.5 degrees. Each camera is equipped with a large number of spectral filters which, taken together, span the electromagnetic spectrum from 0.2 20° 20° to 1.1 micrometers. At the heart of each camera is a charged coupled device (CCD) detector consisting of a 1024 square array of pixels, each 12 microns on a side. MAP SHEET DESIGNATION Se Enceladus (Saturnian satellite) 400K Scale 1 : 400 000 Bahman 0/36 Center point in degrees consisting of latitude/west longitude CMN Controlled Mosaic with Nomenclature 2018 Year of publication IMAGE PROCESSING3 - Radiometric correction of the images - Creation of a dense tie point network - Multiple least-square bundle adjustments - Ortho-image mosaicking A 10° S 10° S CONTROL O F For the Cassini mission, spacecraft position and camera pointing data are available in the form of R SPICE kernels. SPICE is a data system providing ancillary data such as spacecraft and target A positions, target body size/shape/orientation, spacecraft orientation, and instrument pointing, which A B is used for planning space science missions and recovering the full value of science instrument R Y D A 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 tie point. Least squares bundle adjustment resulted in a root mean square (rms) residual of 0.45 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, 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 0° 0° 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 by crater Salih at 5° west. MAP PROJECTION Salih Mercator projection onto a secant cylinder using standard parallels at 13°S and 13°N Scale is true at 13°S / 13°N Adopted figure: sphere ISBANIR FOSSA Mean radius: 252.1 km Grid system: planetographic latitude, west longitude NOMENCLATURE Names are suggested by the ISS-Camera-Team and approved by the International Astronomical -10° -10° Union (IAU). For a complete list of IAU-approved names on Enceladus, see the Gazetter of Planetary Nomenclature at http://planetarynames.wr.usgs.gov/. REFERENCES 1 Roatsch, Th., Kersten, E., Hoffmeister, A., Wählisch, M., Matz, K.-D., Porco, C.C., 2013, Recent improvements of the Saturnian satellites atlases: Mimas, Enceladus, and Dione, Planetary and Space Science, 77, 118-125. 2 Porco, C.C., West, R.A., Squyres, S., McEwen, A., Thomas, P.C., Murray, C.D., DelGenio, J.A., Ingersoll, A.P., Johnson, T.V., Neukum, G., Veverka, J., Dones, L., Brahic, A., Burns, J.A., Haemmerle, V., Knowles, B., Dawson, D., Roatsch, Th., Beurle, K., Owen, W., 2004, Cassini Imaging Science: Instrument Characteristics and Anticipated Scientific Investigations at Saturn, Space Science Review, 115, 363-497. 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 Space Science. 4 Davies, M.E. and Katayama, F.Y., 1983, The Control Networks of Mimas and Enceladus, Icarus, -20° -20° 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, -22° -22° P.K., Tholen, D.J., Thomas, P.C., Williams, I.P., 2018, Report of the IAU Working Group on Cartogra- 72° West 60° 50° 40° 30° 20° 10° 0° West phic Coordinates and Rotational Elements: 2015, Celestial Mechanics and Dynamical Astronomy, 130, 3, 22. Image processing (USGS): Becker, T.L., Bland, M.T. Scale 1:400 000 Cartographic production and design (DLR): Kersten, E., Wählisch, M. 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 6 N1487300648 72° West 60° 40° 20° 0° West 45 N1584039961 22° 49 N1597183387 22° 95 60 N1637465264 m/px 61 N1637465376 30° 62 N1637465488 400 - 500 94 45 78 63 N1637465824 64 N1637465942 84 10° 10° 300 - 400 Se-10 Se-9 Se-8 Se-7 Se-6 66 N1637469285 99 83 Aziz Ebony Dorsum Khusrau Bulak Sulcus Salih 74 N1660434892 75 N1660435041 200 - 300 63 64 79 82 76 N1660435192 360° 330° 300° 270° 240° 210° 180° 150° 120° 90° 60° 30° 0° 66 77 N1660435342 0° 0° 0° 81 150 - 200 78 N1660435474 105 79 N1660435642 62 100 - 150 77 76 80 N1660435791 81 N1660435942 -10° -10° 61 6 82 N1660436067 50 - 100 80 75 83 N1660436242 Se-14 Se-13 Se-12 Se-11 84 N1660436392 <50 -30° Cashmere Sulci Hassan Otbah Kamar 104 94 N1696174830 74 95 N1696175570 60 49 99 N1702360720 -22° -22° 104 N1711571587 Phase angle 120° 72° West 60° 40° 20° 0° West 105 N1711573744 Incidence angle 87° Emission angle 80° -60° Se-15 Damascus Sulcus Se 400K 0/36 CMN, 2018 Se-6.
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