Difference between revisions of "Appleton-Tsu Basin"

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(Created page with "<div id="content_view" class="wiki" style="display: block"> =Appleton-Tsu Basin= ''(unofficial name)''<br /> {| class="wiki_table" | colspan="2" | Lat: 149.0°, Long: 27....")
 
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[[Image:ATB-small.jpg|ATB-small.jpg]]<br />
 
[[Image:ATB-small.jpg|ATB-small.jpg]]<br />
 
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''Visualization of farside Kaguya altimetry data by Michael Zeiler; from LPOD, Nov 23, 2009'' On the small image [/Appleton Appleton] and [/Tsu%20Chung-Chi Tsu Chung-Chi] are indicated by A & T.<br /> <div id="toc">
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''Visualization of farside Kaguya altimetry data by Michael Zeiler; from LPOD, Nov 23, 2009'' On the small image [[Appleton|Appleton]] and [[Tsu%20Chung-Chi|Tsu Chung-Chi]] are indicated by A & T.<br /> <div id="toc">
 
=Table of Contents=
 
=Table of Contents=
 
<div style="margin-left: 1em">[#Appleton-Tsu Basin Appleton-Tsu Basin]</div><div style="margin-left: 2em">[#Appleton-Tsu Basin-Images Images]</div><div style="margin-left: 2em">[#Appleton-Tsu Basin-Maps Maps]</div><div style="margin-left: 2em">[#Appleton-Tsu Basin-Basin Classification Basin Classification]</div><div style="margin-left: 2em">[#Appleton-Tsu Basin-Description Description]</div><div style="margin-left: 2em">[#Appleton-Tsu Basin-Additional Information Additional Information]</div><div style="margin-left: 2em">[#Appleton-Tsu Basin-Nomenclature Nomenclature]</div><div style="margin-left: 2em">[#Appleton-Tsu Basin-LPOD Articles LPOD Articles]</div><div style="margin-left: 2em">[#Appleton-Tsu Basin-Bibliography Bibliography]</div></div>
 
<div style="margin-left: 1em">[#Appleton-Tsu Basin Appleton-Tsu Basin]</div><div style="margin-left: 2em">[#Appleton-Tsu Basin-Images Images]</div><div style="margin-left: 2em">[#Appleton-Tsu Basin-Maps Maps]</div><div style="margin-left: 2em">[#Appleton-Tsu Basin-Basin Classification Basin Classification]</div><div style="margin-left: 2em">[#Appleton-Tsu Basin-Description Description]</div><div style="margin-left: 2em">[#Appleton-Tsu Basin-Additional Information Additional Information]</div><div style="margin-left: 2em">[#Appleton-Tsu Basin-Nomenclature Nomenclature]</div><div style="margin-left: 2em">[#Appleton-Tsu Basin-LPOD Articles LPOD Articles]</div><div style="margin-left: 2em">[#Appleton-Tsu Basin-Bibliography Bibliography]</div></div>
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[http://www.lpod.org/coppermine/thumbnails.php?album=search&type=full&search=Moscoviense LPOD Photo Gallery] [http://www.lpi.usra.edu/resources/lunar_orbiter/bin/srch_nam.shtml?Moscoviense%7C0 Lunar Orbiter Images] [http://www.lpi.usra.edu/resources/apollo/search/feature/?feature=Mare+Moscoviense&sort= Apollo Images of Mare Moscoviense]<br /> <br />  
 
[http://www.lpod.org/coppermine/thumbnails.php?album=search&type=full&search=Moscoviense LPOD Photo Gallery] [http://www.lpi.usra.edu/resources/lunar_orbiter/bin/srch_nam.shtml?Moscoviense%7C0 Lunar Orbiter Images] [http://www.lpi.usra.edu/resources/apollo/search/feature/?feature=Mare+Moscoviense&sort= Apollo Images of Mare Moscoviense]<br /> <br />  
 
==Maps==
 
==Maps==
''([/LAC%20zone LAC zone] 48B3)''<br /> <br />  
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''([[LAC%20zone|LAC zone]] 48B3)''<br /> <br />  
==[/Lunar%20Basins Basin Classification]==
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==[[Lunar%20Basins|Basin Classification]]==
 
  (description of terms and most numeric basin data from Wood, C.A. (2004) [http://www.lpod.org/cwm/DataStuff/Lunar%20Basins.htm Impact Basin Database])<br /> <br />  
 
  (description of terms and most numeric basin data from Wood, C.A. (2004) [http://www.lpod.org/cwm/DataStuff/Lunar%20Basins.htm Impact Basin Database])<br /> <br />  
 
{| class="wiki_table"
 
{| class="wiki_table"
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<br />  
 
<br />  
 
==Description==
 
==Description==
  Originally considered to be an outer ring of the [/Mare%20Moscoviense Moscoviense Basin], but the [/Kaguya Kaguya] topography suggests that more likely it is an older basin that Moscoviense formed in. Kaguya scientists found that the thinnest crust on the Moon was at Moscoviense - perhaps that is because '''Appleton-Tsu''' previously thinned in it. This also explains why mare lava occurs in Moscoviense, far from any other on the farside.<br /> <br />  
+
  Originally considered to be an outer ring of the [[Mare%20Moscoviense|Moscoviense Basin]], but the [[Kaguya|Kaguya]] topography suggests that more likely it is an older basin that Moscoviense formed in. Kaguya scientists found that the thinnest crust on the Moon was at Moscoviense - perhaps that is because '''Appleton-Tsu''' previously thinned in it. This also explains why mare lava occurs in Moscoviense, far from any other on the farside.<br /> <br />  
 
==Additional Information==
 
==Additional Information==
 
* The depth given in the title line is based on the difference between typical heights on the rim in the north and southwest (1741.6 km) and on the floor (1734.1 km).
 
* The depth given in the title line is based on the difference between typical heights on the rim in the north and southwest (1741.6 km) and on the floor (1734.1 km).
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==Nomenclature==
 
==Nomenclature==
  
* Basins located between craters are given the names of the two opposite craters with a hyphen in between, in this case [/Appleton Appleton] and [/Tsu%20Chung-Chi Tsu Chung-Chi].
+
* Basins located between craters are given the names of the two opposite craters with a hyphen in between, in this case [[Appleton|Appleton]] and [[Tsu%20Chung-Chi|Tsu Chung-Chi]].
* None of the hyphenated basin names are assigned or officially recognized by the [/IAU IAU].
+
* None of the hyphenated basin names are assigned or officially recognized by the [[IAU|IAU]].
 
* This probable basin was named in the [http://lpod.wikispaces.com/November%2023%2C%202009 LPOD] cited below.
 
* This probable basin was named in the [http://lpod.wikispaces.com/November%2023%2C%202009 LPOD] cited below.
 
<br />  
 
<br />  

Revision as of 15:39, 15 April 2018

Appleton-Tsu Basin

(unofficial name)

Lat: 149.0°, Long: 27.0°, Main ring diam: 640 km, Depth: 7.4 km, Rukl: (farside)

ATB.jpg

ATB-small.jpg

Visualization of farside Kaguya altimetry data by Michael Zeiler; from LPOD, Nov 23, 2009 On the small image Appleton and Tsu Chung-Chi are indicated by A & T.

Table of Contents

[#Appleton-Tsu Basin Appleton-Tsu Basin]
[#Appleton-Tsu Basin-Images Images]
[#Appleton-Tsu Basin-Maps Maps]
[#Appleton-Tsu Basin-Basin Classification Basin Classification]
[#Appleton-Tsu Basin-Description Description]
[#Appleton-Tsu Basin-Additional Information Additional Information]
[#Appleton-Tsu Basin-Nomenclature Nomenclature]
[#Appleton-Tsu Basin-LPOD Articles LPOD Articles]
[#Appleton-Tsu Basin-Bibliography Bibliography]

Images

LPOD Photo Gallery Lunar Orbiter Images Apollo Images of Mare Moscoviense

Maps

(LAC zone 48B3)

Basin Classification

(description of terms and most numeric basin data from Wood, C.A. (2004) Impact Basin Database)

Certainty of Existence
USGS Age
Wilhelms Age Group
Ring Diameters
Mare Thickness
Mascon
Probable


640 km
km
mG gravity anomaly


Description

Originally considered to be an outer ring of the Moscoviense Basin, but the Kaguya topography suggests that more likely it is an older basin that Moscoviense formed in. Kaguya scientists found that the thinnest crust on the Moon was at Moscoviense - perhaps that is because Appleton-Tsu previously thinned in it. This also explains why mare lava occurs in Moscoviense, far from any other on the farside.

Additional Information

  • The depth given in the title line is based on the difference between typical heights on the rim in the north and southwest (1741.6 km) and on the floor (1734.1 km).


Nomenclature

  • Basins located between craters are given the names of the two opposite craters with a hyphen in between, in this case Appleton and Tsu Chung-Chi.
  • None of the hyphenated basin names are assigned or officially recognized by the IAU.
  • This probable basin was named in the LPOD cited below.


LPOD Articles

Appleton-Tsu Basin?

Bibliography




This page has been edited 1 times. The last modification was made by - tychocrater tychocrater on Jun 13, 2009 3:24 pm - mfx3