Difference between revisions of "Montes Hercynii"

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(Created page with "<div id="content_view" class="wiki" style="display: block"> =Montes Hercynii= ''(discontinued [/IAU IAU] name; formerly '''Hercynian Mts''')''<br /> {| class="wiki_table"...")
 
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=Montes Hercynii=
 
=Montes Hercynii=
''(discontinued [/IAU IAU] name; formerly '''Hercynian Mts''')''<br />  
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''(discontinued [[IAU|IAU]] name; formerly '''Hercynian Mts''')''<br />  
 
{| class="wiki_table"
 
{| class="wiki_table"
 
| Lat: 23.9°N, Long: 79.5°W, Diam: 145 km, Depth: , Rükl: 17<br />
 
| Lat: 23.9°N, Long: 79.5°W, Diam: 145 km, Depth: , Rükl: 17<br />
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<div id="toc">
 
<div id="toc">
 
=Table of Contents=
 
=Table of Contents=
<div style="margin-left: 1em">[#Montes Hercynii Montes Hercynii]</div><div style="margin-left: 2em">[#Montes Hercynii-Images Images]</div><div style="margin-left: 2em">[#Montes Hercynii-Maps Maps]</div><div style="margin-left: 2em">[#Montes Hercynii-Description Description]</div><div style="margin-left: 2em">[#Montes Hercynii-Description: Elger Description: Elger]</div><div style="margin-left: 2em">[#Montes Hercynii-Additional Information Additional Information]</div><div style="margin-left: 2em">[#Montes Hercynii-Nomenclature Nomenclature]</div><div style="margin-left: 2em">[#Montes Hercynii-LPOD Articles LPOD Articles]</div><div style="margin-left: 2em">[#Montes Hercynii-Bibliography Bibliography]</div></div>[http://www.lpod.org/coppermine/albums/userpics/Montes_Hercynii_LO-IV-182H_LTVT.JPG [[Image:normal_Montes_Hercynii_LO-IV-182H_LTVT.JPG|external image normal_Montes_Hercynii_LO-IV-182H_LTVT.JPG]]]<br /> ''[http://lpod.org/coppermine/displayimage.php?pos=-3196 LO-IV-182H]'' This name apparently was applied to the west wall of [/Struve Struve], the 164-km diameter crater that occupies the right half of this image. The smooth-floored crater partially visible along the top edge is 19-km '''[/Russell Russell] B''', and the relatively low arc in the extreme lower left corner is the northeast rim of 62-km '''[/Balboa Balboa] B'''. The name '''Montes Hercynii''' appears to have embraced at least the central part of the "range" extending between these points; but its exact limits are unclear.<br /> <br />  
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<div style="margin-left: 1em">[#Montes Hercynii Montes Hercynii]</div><div style="margin-left: 2em">[#Montes Hercynii-Images Images]</div><div style="margin-left: 2em">[#Montes Hercynii-Maps Maps]</div><div style="margin-left: 2em">[#Montes Hercynii-Description Description]</div><div style="margin-left: 2em">[#Montes Hercynii-Description: Elger Description: Elger]</div><div style="margin-left: 2em">[#Montes Hercynii-Additional Information Additional Information]</div><div style="margin-left: 2em">[#Montes Hercynii-Nomenclature Nomenclature]</div><div style="margin-left: 2em">[#Montes Hercynii-LPOD Articles LPOD Articles]</div><div style="margin-left: 2em">[#Montes Hercynii-Bibliography Bibliography]</div></div>[http://www.lpod.org/coppermine/albums/userpics/Montes_Hercynii_LO-IV-182H_LTVT.JPG [[Image:normal_Montes_Hercynii_LO-IV-182H_LTVT.JPG|external image normal_Montes_Hercynii_LO-IV-182H_LTVT.JPG]]]<br /> ''[http://lpod.org/coppermine/displayimage.php?pos=-3196 LO-IV-182H]'' This name apparently was applied to the west wall of [[Struve|Struve]], the 164-km diameter crater that occupies the right half of this image. The smooth-floored crater partially visible along the top edge is 19-km '''[[Russell|Russell]] B''', and the relatively low arc in the extreme lower left corner is the northeast rim of 62-km '''[[Balboa|Balboa]] B'''. The name '''Montes Hercynii''' appears to have embraced at least the central part of the "range" extending between these points; but its exact limits are unclear.<br /> <br />  
 
==Images==
 
==Images==
 
[http://www.lpod.org/coppermine/thumbnails.php?album=search&type=full&search=Struve LPOD Photo Gallery] [http://www.lpi.usra.edu/resources/lunar_orbiter/bin/srch_nam.shtml?Struve%7C0 Lunar Orbiter Images]<br /> <br />  
 
[http://www.lpod.org/coppermine/thumbnails.php?album=search&type=full&search=Struve LPOD Photo Gallery] [http://www.lpi.usra.edu/resources/lunar_orbiter/bin/srch_nam.shtml?Struve%7C0 Lunar Orbiter Images]<br /> <br />  
 
==Maps==
 
==Maps==
''([/LAC%20zone LAC zone] 37C1)'' [http://www.lpi.usra.edu/resources/mapcatalog/LTM/sheet_2/ LTM map] (version 1), [http://www.lpi.usra.edu/resources/mapcatalog/LTM/sheet_2_grad/ LTM Map] (version 2), [http://planetarynames.wr.usgs.gov/images/Lunar/lac_37.pdf USGS Digital Atlas PDF] (see [/Struve Struve])<br /> <br />  
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''([[LAC%20zone|LAC zone]] 37C1)'' [http://www.lpi.usra.edu/resources/mapcatalog/LTM/sheet_2/ LTM map] (version 1), [http://www.lpi.usra.edu/resources/mapcatalog/LTM/sheet_2_grad/ LTM Map] (version 2), [http://planetarynames.wr.usgs.gov/images/Lunar/lac_37.pdf USGS Digital Atlas PDF] (see [[Struve|Struve]])<br /> <br />  
 
==Description==
 
==Description==
 
<br />  
 
<br />  
 
==Description: Elger==
 
==Description: Elger==
''([/IAU%20Directions IAU Directions])'' <u>Hercynian Mountains</u>, on the north-west limb, west of the walled plain [/Struve Otto Struve]. These are too near the edge to be well observed, but, from what can be seen of them, they appear to abound in lofty peaks, and to bear more resemblance to a terrestrial chain than any which have yet been referred to.<br /> <br />  
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''([[IAU%20Directions|IAU Directions]])'' <u>Hercynian Mountains</u>, on the north-west limb, west of the walled plain [[Struve|Otto Struve]]. These are too near the edge to be well observed, but, from what can be seen of them, they appear to abound in lofty peaks, and to bear more resemblance to a terrestrial chain than any which have yet been referred to.<br /> <br />  
 
==Additional Information==
 
==Additional Information==
* The position and "diameter" given in the title line refer to the central part of the "range" shown in the [/Lunar%20Orbiter Lunar Orbiter] image. The original name may well have been intended to include the broad peaks at the top and bottom of the frame, in which case the center would be moved about 1 deg to the east, and the diameter increased to about 185 km.
+
* The position and "diameter" given in the title line refer to the central part of the "range" shown in the [[Lunar%20Orbiter|Lunar Orbiter]] image. The original name may well have been intended to include the broad peaks at the top and bottom of the frame, in which case the center would be moved about 1 deg to the east, and the diameter increased to about 185 km.
 
<br />  
 
<br />  
 
==Nomenclature==
 
==Nomenclature==
  
* '''Hercynian Mts''' is said to be an ancient name for the [http://en.wikipedia.org/wiki/Thuringian_Forest Thüringer Wald Mountains] (ref: ''[/Who%27s%20Who%20in%20the%20Moon Who's Who in the Moon]'').
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* '''Hercynian Mts''' is said to be an ancient name for the [http://en.wikipedia.org/wiki/Thuringian_Forest Thüringer Wald Mountains] (ref: ''[[Who%27s%20Who%20in%20the%20Moon|Who's Who in the Moon]]'').
* According to ''[/Whitaker Whitaker]'' (p. 220), the name '''Hercynii Montes''' was introduced by [/M%C3%A4dler Mädler].
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* According to ''[[Whitaker|Whitaker]]'' (p. 220), the name '''Hercynii Montes''' was introduced by [[M%C3%A4dler|Mädler]].
* The name '''Hercynian Mts''' was part of the original [/IAU%20nomenclature IAU nomenclature] of [/Blagg%20and%20M%C3%BCller Blagg and Müller] (1935).
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* The name '''Hercynian Mts''' was part of the original [[IAU%20nomenclature|IAU nomenclature]] of [[Blagg%20and%20M%C3%BCller|Blagg and Müller]] (1935).
* The name was Latinized to '''Montes Hercynii''' in [/IAU%20Transactions%20XIIB IAU Transactions XIIB] (1964).
+
* The name was Latinized to '''Montes Hercynii''' in [[IAU%20Transactions%20XIIB|IAU Transactions XIIB]] (1964).
* The name was dropped in [/IAU%20Transactions%20XIVB IAU Transactions XIVB] (1970), where it was declared to be one of five lunar ranges "not clearly identifiable" on images taken from space. Note: ''[/Whitaker Whitaker]'' (p. 220) says the name was not used after 1961, but he appears to be in error.
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* The name was dropped in [[IAU%20Transactions%20XIVB|IAU Transactions XIVB]] (1970), where it was declared to be one of five lunar ranges "not clearly identifiable" on images taken from space. Note: ''[[Whitaker|Whitaker]]'' (p. 220) says the name was not used after 1961, but he appears to be in error.
* Assuming the range has been correctly identified here, on modern maps it would be regarded as the west wall of [/Struve Struve].
+
* Assuming the range has been correctly identified here, on modern maps it would be regarded as the west wall of [[Struve|Struve]].
 
<br />  
 
<br />  
 
==LPOD Articles==
 
==LPOD Articles==

Revision as of 16:04, 15 April 2018

Montes Hercynii

(discontinued IAU name; formerly Hercynian Mts)

Lat: 23.9°N, Long: 79.5°W, Diam: 145 km, Depth: , Rükl: 17

Table of Contents

[#Montes Hercynii Montes Hercynii]
[#Montes Hercynii-Images Images]
[#Montes Hercynii-Maps Maps]
[#Montes Hercynii-Description Description]
[#Montes Hercynii-Description: Elger Description: Elger]
[#Montes Hercynii-Additional Information Additional Information]
[#Montes Hercynii-Nomenclature Nomenclature]
[#Montes Hercynii-LPOD Articles LPOD Articles]
[#Montes Hercynii-Bibliography Bibliography]
external image normal_Montes_Hercynii_LO-IV-182H_LTVT.JPG
LO-IV-182H This name apparently was applied to the west wall of Struve, the 164-km diameter crater that occupies the right half of this image. The smooth-floored crater partially visible along the top edge is 19-km Russell B, and the relatively low arc in the extreme lower left corner is the northeast rim of 62-km Balboa B. The name Montes Hercynii appears to have embraced at least the central part of the "range" extending between these points; but its exact limits are unclear.

Images

LPOD Photo Gallery Lunar Orbiter Images

Maps

(LAC zone 37C1) LTM map (version 1), LTM Map (version 2), USGS Digital Atlas PDF (see Struve)

Description


Description: Elger

(IAU Directions) Hercynian Mountains, on the north-west limb, west of the walled plain Otto Struve. These are too near the edge to be well observed, but, from what can be seen of them, they appear to abound in lofty peaks, and to bear more resemblance to a terrestrial chain than any which have yet been referred to.

Additional Information

  • The position and "diameter" given in the title line refer to the central part of the "range" shown in the Lunar Orbiter image. The original name may well have been intended to include the broad peaks at the top and bottom of the frame, in which case the center would be moved about 1 deg to the east, and the diameter increased to about 185 km.


Nomenclature


LPOD Articles


Bibliography




This page has been edited 1 times. The last modification was made by - tychocrater tychocrater on Jun 13, 2009 3:24 pm - afx4