Erriapus
Template:Short description Template:About {{#invoke:infobox|infoboxTemplate | class = vcard | titleclass = fn org | title = Erriapus | image = {{#invoke:InfoboxImage|InfoboxImage|image=Erriapus-discovery-CFHT.gif|upright={{#if:||1.1}}|alt=}} | caption = Discovery images of Erriapus taken by the CFHT in September 2000 | headerstyle = {{#if:|background-color:|background-color:#E0CCFF}} | labelstyle = max-width:{{#if:||11em}}; | autoheaders = y
| header1 = Discovery<ref name="Discoverers_JPL">{{#invoke:citation/CS1|citation |CitationClass=web }}</ref>
| label2 = Discovered by | data2 = John J. Kavelaars et al. | label3 = Discovery site | data3 = | label4 = Discovery date | data4 = 2000 | label5 = Template:Longitem | data5 =
| header10 = {{#if:|Designations|Designations}}
| label11 = Template:Longitem | data11 = Saturn XXVIII | label12 = Pronunciation | data12 = Template:IPAc-en | label13 = Template:Longitem | data13 = Erriap(p)us | label14 = Template:Longitem | data14 = S/2000 S 10 | label15 = Template:Longitem | data15 = | label16 = Adjectives | data16 = | label17 = Symbol | data17 =
| header20 = Orbital characteristics{{#ifeq:|yes| (barycentric)}}<ref name="JPL_mean_elems">{{#invoke:citation/CS1|citation |CitationClass=web }}</ref>
| data21 =
| data22 = {{#if:2000 January 1.5 |Epoch 2000 January 1.5}}
| data23 = {{#if: | Uncertainty parameter {{{uncertainty}}}}}
| label24 = Observation arc
| data24 =
| label25 = Earliest precovery date
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| label26 = {{#switch:{{{apsis}}} |apsis|gee|barion|center|centre|(apsis)=Apo{{{apsis}}} |Ap{{#if:|{{{apsis}}}|helion}}}}
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| label27 = Peri{{#if:|{{{apsis}}}|helion}}
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| label28 = Peri{{#if:|{{{apsis}}}|apsis}}
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| data29 =
| label30 = Periastron
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| label31 = Apoastron
| data31 =
| label32 = Template:Longitem
| data32 = 17 507 200 km
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| label34 = Eccentricity
| data34 = 0.462
| label35 = Template:Longitem
| data35 = 871.1 d
(2.38 yr)
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| label40 = Inclination
| data40 = 38.7
| label41 = Template:Longitem
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| label46 = Template:Nowrap
| data46 =
| label47 = Satellite of
| data47 = Saturn
| label48 = Group
| data48 = Gallic group
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| label50 = Star
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| label51 = Earth MOID
| data51 =
| label52 = Mercury MOID
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| label53 = Venus MOID
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| label54 = Mars MOID
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| label55 = Jupiter MOID
| data55 =
| label56 = Saturn MOID
| data56 =
| label57 = Uranus MOID
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| label58 = Neptune MOID
| data58 =
| label59 = TJupiter
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| header60 = Proper orbital elements
| label61 = Template:Longitem
| data61 = {{#if: |{{{p_semimajor}}} AU}}
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| 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}}<ref name="LPSC2654">Template:Cite conference</ref><ref name="Denk2018"/>
| label71 = Dimensions | data71 = 16.30 × 10 × 6.34 km (modeled)<ref>Template:Cite journal</ref> | label72 = Template:Longitem | data72 = Template:Val | 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 = | label80 = Mass | data80 = | label81 = Template:Longitem | data81 = | label82 = Template:Longitem | data82 = | label83 = Template:Longitem | data83 = | label84 = Template:Longitem | data84 = | label85 = Template:Longitem | data85 = Template:Val h | label86 = Template:Longitem | data86 = | label87 = Template:Longitem | data87 = | label88 = Template:Longitem | data88 = | label89 = Template:Longitem | data89 = | label90 = Template:Longitem | data90 = | label91 = Template:Longitem | data91 = | label92 = Template:Longitem | data92 = | label93 = {{#if: |Template:Longitem |Albedo}} | data93 = 0.06 (assumed) | label94 = Temperature | data94 =
| data100 = {{#if:|
{{#if:|}}{{#if:|}}{{#if:|}}{{#if:|}}Surface temp. | min | mean | max |
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{{{temp_name2}}} | |||
{{{temp_name3}}} | |||
{{{temp_name4}}} |
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| label101 = Surface absorbed dose rate
| data101 =
| label102 = Surface equivalent dose rate
| data102 =
| label103 = Template:Longitem
| data103 = light red
B−V=0.83, R−V=0.49<ref name="Grav2003" />
| label104 = Template:Longitem
| data104 =
| label105 = Template:Longitem
| data105 = 23.0
| label106 = Template:Longitem
| data106 = 13.7
| label107 = Template:Longitem
| data107 =
| header110 = Atmosphere
| label111 = Template:Longitem | data111 = | label112 = Template:Longitem | data112 = | label113 = Composition by volume | data113 =
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Erriapus Template:IPAc-en, or Saturn XXVIII (28), is a prograde irregular satellite of Saturn. It was discovered by Brett Gladman, John J. Kavelaars and colleagues in 2000, and given the temporary designation S/2000 S 10.<ref>{{#invoke:citation/CS1|citation |CitationClass=web }}</ref><ref>{{#invoke:citation/CS1|citation |CitationClass=web }}</ref> It was named Erriapo in August 2003<ref>{{#invoke:citation/CS1|citation |CitationClass=web }}</ref> after Erriapus (also rendered Erriappus), a giant in Gaulish mythology; the name was changed from dative Erriapo to nominative Erriapus per IAU conventions in late 2007.<ref>{{#invoke:citation/CS1|citation |CitationClass=web }}</ref><ref>IAUC 9191: SATURN XXVIII (ERRIAPUS) January 11, 2011</ref>
Erriapus is about 10 kilometres in diameter, and orbits Saturn at an average distance of 17.5 Gm in 871 days.
As a member of the Gallic group of irregular satellites, which share similar orbital characteristics and a light-red colour, Erriapus is hypothesized to have its origin in the break-up of a common progenitor of the group,<ref name="Grav2003">Template:Cite journal</ref><ref name="Gladman2001">Template:Cite journal</ref> or to be a fragment of its largest member, Albiorix.<ref name="Grav20062">Template:Cite journal</ref> It has a rotation period of Template:Val, and is thought to rotate on its side, giving it similar seasons to those of Uranus.<ref>Template:Cite journal</ref><ref>Template:Cite conference</ref> With a fairly elongated shape, it is a candidate for a contact binary or binary moon.<ref name="Denk2018">Template:Cite book</ref>