341 California

Template:Short description Template:Use dmy dates {{#invoke:infobox|infoboxTemplate | class = vcard | titleclass = fn org | title = 341 California | image = {{#invoke:InfoboxImage|InfoboxImage|image=000341-asteroid shape model (341) California.png|upright={{#if:||1.1}}|alt=}} | caption = Shape model of California | headerstyle = {{#if:#D6D6D6|background-color:#D6D6D6|background-color:#E0CCFF}} | labelstyle = max-width:{{#if:||11em}}; | autoheaders = y

| header1 = Discovery

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

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15 km<ref name="IRAS"/> | label72 = Template:Longitem | data72 = | 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 = ~2.7 g/cm³<ref name="Krasinsky_et_al_2002"/> | label82 = Template:Longitem | data82 = | label83 = Template:Longitem | data83 = | label84 = Template:Longitem | data84 = | label85 = Template:Longitem | data85 = Template:Convert | 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:yes |Template:Longitem |Albedo}} | data93 = Template:Val<ref name="jpldata"/>
0.495<ref name="IRAS"/> | label94 = Temperature | data94 =

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| header110 = Atmosphere

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341 California is an asteroid belonging to the Flora family in the Main Belt. It was discovered by Max Wolf on 25 September 1892 in Heidelberg, and is named for the U.S. state of California.<ref name=Peebles2016/> This object is orbiting the Sun at a distance of Template:Val with a period of Template:Convert and an eccentricity (ovalness) of 0.19. The orbital plane is inclined at an angle of 5.7° to the plane of the ecliptic.<ref name="jpldata"/>

The very slow rotation rate of this asteroid favors collecting photometric data for an extended period in order to measure the period. Data collected from June to December 2016 was used to produce a light curve showing a rotation period of Template:Val with a brightness variation of 0.9 in magnitude. It is tumbling with a period of Template:Val.<ref name=Pilcher_et_al_2017/> It has an unusually high albedo.

ReferencesEdit

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External linksEdit

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