S/2006 S 1

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S/2006 S 1 is ∼4½ kilometers in size and thus one of the small irregular moons of Saturn. It has been discovered in 2006 joint with eight other outer Saturnian moons. Its mean distance to Saturn is ∼19 million kilometers, with one revolution around the planet on a retrograde orbit lasting approximately 2 years, 7 months and 1 week. This moon has not been named yet. Although barely bright enough in summer 2012, fall 2014, or spring 2017, we made no attempt to observe it with Cassini because its position in the sky was not known precisely enough at this time.

Table of contents

(1) Astronomical and physical properties

This page is intended to compile (much of) our knowledge of unnamed moon S/2006 S 1 in compact form, including general information like discovery circumstances and orbital and physical parameters. For further reading on irregular moons of Saturn in general, see the reference list at my outer-Saturnian moons page.

Last update: 05 Nov 2019 — page content is best displayed on a screen at least 1024 pixels wide


(1) Astronomical and physical properties

Moon name Saturn range Orbit period Orbit direction Size Rotation period Discovery year
S/2006 S 1
million km
years
retrograde
km
unknown
2006

Basic information about S/2006 S 1 is offered in tabular form:
(1A) Basic properties
← Table (Basic properties) in text format [ not available yet ]

Most fundamental values are highlighted in red. The notes offer explanations, calculations, accuracies, references, etc. The data were obtained from ground-based observations.

(1A) Basic properties
Moon name(1) Orbit direction(7) retrograde Mean size(11) ∼ 4½ km
Moon abbrev.(2) 6S1 Semi-major axis(8) 18.74 ⋅ 10km Absolute visual magnitude(12) ∼ 15.5 mag
IAU number(3) Orbit eccentricity(8) 0.08 Apparent vis. mag. from Earth(13) 24.5 mag
Provisional desig.(4) S/2006 S 1 Orbit inclination(8) 155.2° First observation date(14) 04 Jan 2006
SPICE ID(5) 65048 Orbital period(8) 954 d Announcement date(14) 30 Jun 2006
Also-used label(6) Group member(9) Norse IAU circ. announcement(14) no. 8727
Dynamical family(10) Hyrrokkin (?) Discoverers(15) S. Sheppard et al.

Table notes:

(1) The object has no proper name yet.

(2) I use this 3-letter abbreviation in the diagrams of my publications simply for practicability reasons. These have no offcial character.

(3) Moon numbers are assigned by the International Astronomical Union (IAU)’s Committee for Planetary System Nomenclature. For satellites, Roman numeral designations are used.

(4) Designation given to the object in the first announcement; the guidelines are explained here.

(5) SPICE is a commonly-used information system of NASA’s Navigation and Ancillary Information Facility (NAIF). It assists engineers in modeling, planning, and executing planetary-exploration missions, and supports observation interpretation for scientists. Each planet and moon obtained a unique SPICE number.

(6) ‘S’ for ‘Saturnian moon’ plus the roman numeral designation in arabic numbers are often-used labels for satellites. Not sure how official that is.

(7) Prograde (counterclockwise as seen from north) or retrograde (clockwise as seen from north).

(8) Orbit semi-major axis a, eccentricity e, inclination i, orbit period P; from S. Sheppard’s website.

(9) Norse, Inuit, or Gallic.

(10) Classification based on the a,e,i space in Fig. 1 and Table 2 in Denk et al. (2018).

(11) Determined from absolute visual magnitude H (see note (12)). The conversion from H to size (diameter of a reference sphere) was calculated through $D=1 \text{ au}\cdot \frac{2}{\sqrt{A}}\cdot 10^{−0.2·(H−M_☉)}$; with solar apparent V magnitude M = −26.71 ± 0.02 mag and Astronomical Unit 1 au = 149 597 870.7 km. For the object’s albedo A, a value of 0.06 is assumed (see discussions in Grav et al. (2015) and Denk et al. (2018) on albedo uncertainties). Due to the uncertain input values, a size determined this way may be uncertain to ∼ −15/+30% (for A ± 0.02 and H ± 0.1).

(12) From MPEC; the number may be uncertain by several tenths of magnitude. The absolute visual magnitude HV is the magnitude (brightness) of an object (in the visible wavelength range) if located 1 au away from the sun and observed at 0° phase angle (i.e., in this definition, the observer virtually sits at the center of the sun). The magnitude scale is logarithmic, with an object of 6th mag being 100x darker than a 1st mag object.

(13) Apparent visual magnitude V; from S. Sheppard’s website.

(14) The date of the photography wherein the object was spotted for the first time is given in the IAU circular released on the announcement date. In 2019, the object was re-discovered in data from Dec 2004, Jan and Mar 2005, and Feb 2006, allowing a refinement of the orbital elements (MPEC 2019-T2xx). (not issued yet)

(15) The discoverer team included: Scott Sheppard, David Jewitt, Jan Kleyna.


© Tilmann Denk (2019)