Template:Short description Template:For multi Template:Use dmy dates {{#invoke:infobox|infoboxTemplate | class = vcard | titleclass = fn org | title = Pan | image = {{#invoke:InfoboxImage|InfoboxImage|image=Pan color PIA21449.png|upright={{#if:||1.1}}|alt=}} | caption = Color photo of Pan by Cassini in March 2017Template:Efn | headerstyle = {{#if:|background-color:|background-color:#E0CCFF}} | labelstyle = max-width:{{#if:||11em}}; | autoheaders = y

| header1 = Discovery

| label2 = Discovered by | data2 = M. R. Showalter | label3 = Discovery site | data3 = | label4 = Discovery date | data4 = July 16, 1990 | label5 = Template:Longitem | data5 =

| header10 = {{#if:|Designations|Designations}}

| label11 = Template:Longitem | data11 = Saturn XVIII | label12 = Pronunciation | data12 = Template:IPAc-en | label13 = Template:Longitem | data13 = Πάν Pān | label14 = Template:Longitem | data14 = S/1981 S 13 | label15 = Template:Longitem | data15 = | label16 = Adjectives | data16 = Pandean Template:IPAc-en<ref>Template:OED</ref> | label17 = Symbol | data17 =

| header20 = Orbital characteristics{{#ifeq:|yes| (barycentric)}}<ref name="Jacobson2008">Template:Cite journal</ref>

| data21 = | data22 = {{#if: |Epoch {{{epoch}}}}} | data23 = {{#if: | Uncertainty parameter {{{uncertainty}}}}} | label24 = Observation arc | data24 = | label25 = Earliest precovery date | data25 = | label26 = {{#switch:{{{apsis}}} |apsis|gee|barion|center|centre|(apsis)=Apo{{{apsis}}} |Ap{{#if:|{{{apsis}}}|helion}}}} | data26 = | label27 = Peri{{#if:|{{{apsis}}}|helion}} | data27 = | label28 = Peri{{#if:|{{{apsis}}}|apsis}} | data28 = | label29 = {{#switch:{{{apsis}}} |helion|astron=Ap{{{apsis}}} |Apo{{#if:|{{{apsis}}}|apsis}}}} | data29 = | label30 = Periastron | data30 = | label31 = Apoastron | data31 = | label32 = Template:Longitem | data32 = Template:Val | label33 = Template:Longitem | data33 = | label34 = Eccentricity | data34 = Template:Val | label35 = Template:Longitem | data35 = Template:Val (Template:Val) | label36 = Template:Longitem | data36 = | label37 = Template:Longitem | data37 = | label38 = Template:Longitem | data38 = | label39 = Template:Longitem | data39 = | label40 = Inclination | data40 = Template:Val | label41 = Template:Longitem | data41 = | label42 = Template:Longitem | data42 = | label43 = Template:Longitem | data43 = | label44 = Template:Longitem | data44 = | label45 = Template:Longitem | data45 = | label46 = Template:Nowrap | data46 = | label47 = Satellite of | data47 = Saturn | label48 = Group | data48 = Shepherd moon of the Encke Gap | label49 = {{#switch: |yes|true=Satellites |Known satellites}} | data49 = | label50 = Star | data50 = | label51 = Earth MOID | data51 = | label52 = Mercury MOID | data52 = | label53 = Venus MOID | data53 = | label54 = Mars MOID | data54 = | label55 = Jupiter MOID | data55 = | label56 = Saturn MOID | data56 = | label57 = Uranus MOID | data57 = | label58 = Neptune MOID | data58 = | label59 = TJupiter | data59 =

| header60 = Proper orbital elements

| label61 = Template:Longitem | data61 = {{#if: |{{{p_semimajor}}} AU}} | label62 = Template:Longitem | data62 = | label63 = Template:Longitem | data63 = | label64 = Template:Longitem | data64 = {{#if: |{{{p_mean_motion}}} degTemplate:\yr}} | label65 = Template:Longitem | data65 = {{#if:|{{#expr:360/1 round 5}} yr
({{#expr:365.25*360/1 round 3}} d) }} | label66 = Template:Longitem | data66 = {{#if:|{{{perihelion_rate}}} arcsecTemplate:\yr }} | label67 = Template:Longitem | data67 = {{#if:|{{{node_rate}}} arcsecTemplate:\yr}}

| header70 = Template:Anchor{{#if:| Physical characteristics|Physical characteristics}}

| label71 = Dimensions | data71 = Template:Val km
(± Template:Val km)<ref name="Thomas2020"/>Template:Rp | label72 = Template:Longitem | data72 = Template:Val<ref name="Thomas2020"/>Template:Rp | label73 = Template:Longitem | data73 = | label74 = Template:Longitem | data74 = | label75 = Template:Longitem | data75 = | label76 = Flattening | data76 = | label77 = Circumference | data77 = | label78 = Template:Longitem | data78 = | label79 = Volume | data79 = Template:Val<ref name="Thomas2020"/>Template:Rp | label80 = Mass | data80 = Template:Val<ref name="Thomas2020"/>Template:Rp | label81 = Template:Longitem | data81 = Template:Val<ref name="Thomas2020"/>Template:Rp | label82 = Template:Longitem | data82 = Template:Val<ref name="Thomas2020"/>Template:Rp | label83 = Template:Longitem | data83 = | label84 = Template:Longitem | data84 = Template:V2 km/s at longest axis
to Template:V2 km/s at poles | label85 = Template:Longitem | data85 = synchronous | label86 = Template:Longitem | data86 = | label87 = Template:Longitem | data87 = | label88 = Template:Longitem | data88 = zero | label89 = Template:Longitem | data89 = | label90 = Template:Longitem | data90 = | label91 = Template:Longitem | data91 = | label92 = Template:Longitem | data92 = | label93 = {{#if: |Template:Longitem |Albedo}} | data93 = 0.5 | label94 = Temperature | data94 = ≈ 78 K

| data100 = {{#if:|

{{#if:|}}{{#if:|}}{{#if:|}}{{#if:|}}
Surface temp. min mean max
{{{temp_name1}}}
{{{temp_name2}}}
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{{{temp_name4}}}

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| label101 = Surface absorbed dose rate | data101 = | label102 = Surface equivalent dose rate | data102 = | label103 = Template:Longitem | data103 = | label104 = Template:Longitem | data104 = | label105 = Template:Longitem | data105 = | label106 = Template:Longitem | data106 = | label107 = Template:Longitem | data107 =

| header110 = Atmosphere

| label111 = Template:Longitem | data111 = | label112 = Template:Longitem | data112 = | label113 = Composition by volume | data113 =

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Pan is the innermost named moon of Saturn.<ref name="Moons of Saturn">{{#invoke:citation/CS1|citation |CitationClass=web }}</ref> It is approximately 35 kilometres across and 23 km wide and orbits within the Encke Gap in Saturn's A Ring. Pan is a ring shepherd and is responsible for keeping the Encke Gap free of ring particles. It is sometimes described as having the appearance of a walnut, or ravioli.<ref name="Ravioli">{{#invoke:citation/CS1|citation |CitationClass=web }}</ref>

Pan was discovered by Mark R. Showalter in 1990 from analysis of old Voyager 2 probe photos and received the provisional designation Template:Nowrap because the discovery images dated back to 1981.<ref name="iauc5052">IAUC 5052: Saturn July 16, 1990 (discovery)</ref>

Prediction and discoveryEdit

The existence of a moon in the Encke Gap was first predicted by Jeffrey N. Cuzzi and Jeffrey D. Scargle in 1985, based on wavy edges of the gap which indicated a gravitational disturbance.<ref>Cuzzi, J. N.; and Scargle, J. D.; Wavy Edges Suggest Moonlet in Encke's Gap, Astrophysical Journal, Vol. 292 (May 1, 1985), pp. 276–290</ref> In 1986, Showalter et al. inferred its orbit and mass by modeling its gravitational wake. They arrived at a precise prediction of 133,603 ± 10 km for the semi-major axis and a mass of 5–10Template:E Saturn masses, and inferred that there was only a single moon within the Encke gap.<ref name="Showalter1986">Template:Cite journal</ref> The actual semi-major axis differs by 19 km, and the actual mass is 8.6Template:E of Saturn's.

The moon was later found within 1° of the predicted position. The search was undertaken by considering all Voyager 2 images and using a computer calculation to predict whether the moon would be visible under sufficiently favorable conditions in each one. Every qualifying Voyager 2 image with a resolution better than ~50 km/pixel shows Pan clearly. In all, it appears in eleven Voyager 2 images.<ref name="Showalter1990">Template:Cite journal</ref><ref name="Showalter1991">Template:Cite journal</ref>

NameEdit

The moon was named on 16 September 1991<ref>IAUC 5347: Satellites of Saturn and Neptune 1991 September 16 (naming the moon)</ref> after the mythological Greek god named Pan, who was (among other things) the god of shepherds. This is a reference to Pan's role as a shepherd moon. It is also designated Template:Nowrap.<ref name="Gazetteer">{{#invoke:citation/CS1|citation |CitationClass=web }}</ref>

OrbitEdit

The eccentricity of Pan's orbit causes its distance from Saturn to vary by ~4 km. Its inclination, which would cause it to move up and down, is not distinguishable from zero with present data. The Encke Gap, within which Pan orbits, is about 322 km wide.<ref name="SaturnRingStats"/>

GeographyEdit

File:Pan (moon) edge-on.jpg
Pan, photographed by Cassini on March 7, 2017. The thin equatorial ridge is clearly visible.

Cassini scientists have described Pan as "walnut-shaped"<ref>"PIA08320: Cruising with Pan", Planetary Photojournal.</ref> owing to the equatorial ridge, similar to that on Atlas, that is visible in images. The ridge is due to ring material that Pan has swept up from the Encke gap. It has been referred to by journalists as a space empanada, a form of stuffed bread or pastry, as well as a ravioli.<ref>Template:Cite news</ref><ref name="Space empanada">{{#invoke:citation/CS1|citation |CitationClass=web }}</ref> A new study suggests that the bizarre shape of Pan could also be due to collisions between tiny moonlets, thus causing them to merge and form Pan (known as the pyramidal regime formation scenario).<ref>{{#invoke:citation/CS1|citation |CitationClass=web }}</ref>

Pandean ringletEdit

The Encke Gap contains a ringlet that is coincident with Pan's orbit, indicating that Pan maintains the particles in horseshoe orbits.<ref>Template:Cite journal</ref> A second ringlet is periodically disrupted by Pan, similarly to how the F Ring is disturbed by Prometheus.<ref>Template:Cite journal</ref>

GalleryEdit

See alsoEdit

NotesEdit

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ReferencesEdit

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External linksEdit

Template:Sister project Template:Spoken Wikipedia

Template:Moons of Saturn Template:Saturn Template:Portal bar