Erasmus - Revision history

NewZimiaGov at 19:10, 18 October 2026

2026-10-18T19:10:25Z

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	\| align="center" colspan="2" style="background:#FFFFFF;"\|		\| align="center" colspan="2" style="background:#FFFFFF;"\|
	{\| border=0 cellpadding=2 cellspacing=0 style="background:none; text-align:center;"		{\| border=0 cellpadding=2 cellspacing=0 style="background:none; text-align:center;"
	\| [[Image:~~Erasmus12~~.png\|100px]]		\| [[Image:Erasmus1018.png\|100px]]
	\|}		\|}
	\|-		\|-

NewZimiaGov at 02:51, 13 October 2026

2026-10-13T02:51:30Z

← Older revision		Revision as of 02:51, 13 October 2026
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	\| align="center" colspan="2" style="background:#FFFFFF;"\|		\| align="center" colspan="2" style="background:#FFFFFF;"\|
	{\| border=0 cellpadding=2 cellspacing=0 style="background:none; text-align:center;"		{\| border=0 cellpadding=2 cellspacing=0 style="background:none; text-align:center;"
	\| [[Image:~~Erasmus627~~.png\|100px]]		\| [[Image:Erasmus12.png\|100px]]
	\|}		\|}
	\|-		\|-

NewZimiaGov at 01:55, 28 June 2026

2026-06-28T01:55:38Z

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	\| align="center" colspan="2" style="background:#FFFFFF;"\|		\| align="center" colspan="2" style="background:#FFFFFF;"\|
	{\| border=0 cellpadding=2 cellspacing=0 style="background:none; text-align:center;"		{\| border=0 cellpadding=2 cellspacing=0 style="background:none; text-align:center;"
	\| [[Image:~~Erasmus2026~~.png\|100px]]		\| [[Image:Erasmus627.png\|100px]]
	\|}		\|}
	\|-		\|-

NewZimiaGov: /* Southern Polar Regions */

2026-04-19T14:35:06Z

Southern Polar Regions

← Older revision		Revision as of 14:35, 19 April 2026
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	==Southern Polar Regions==		==Southern Polar Regions==
	The Southern Polar Regions of ~~'''~~Erasmus~~'''~~ are brighter and more ~~topographically varied~~ than much of the ~~equatorial surface. Broad frozen plains~~, ~~enclosed icy~~ basins, ~~fractured~~ margins, and ~~rough polar uplands extend across~~ the ~~high southern latitudes~~. ~~The southern cap is irregular~~ and ~~segmented~~, ~~with~~ embedded ~~dark masses~~, ~~broken shelves~~, ~~and uneven frozen cover spread across a rugged underlying surface~~.		The Southern Polar Regions of Erasmus are brighter and more visibly active than much of the north, with wide ice-rich surfaces spreading across the lower hemisphere in smooth sheets, pooled basins, and broken glacial margins. In the southwest, the subdued depression known as Kyra Hollow marks a darker transitional basin between exposed southern ground and the brighter ice systems beyond. Across the south-central lower hemisphere, Bride’s Mirror Shelf occupies one of the moon’s clearest and most reflective ice provinces, where bright frozen material appears gathered across lower terrain and broken by embedded ridges and protrusions. To the southeast, Benevolence Basin stands out as a distinct enclosed southern formation, while Hostward Rift marks one of the clearest disrupted margins descending toward the far southern edge of the map.

	~~Several large basins in~~ the ~~south contain smooth bright ice~~, ~~while nearby ridges~~, ~~exposed rocky masses~~, and ~~cratered uplands project through the surrounding~~ frozen ~~terrain~~. ~~Fractures~~ and ~~collapsed margins are common~~ across ~~the lower edge of the polar zone. In places~~ the ice ~~gathers within low basins and troughs; elsewhere it thins across rougher high ground~~ and broken ~~crater rims~~. ~~This gives the south a segmented structure~~, ~~with strong contrast between white frozen surfaces~~ and ~~darker exposed crust.~~		The southern polar zone appears shaped by the interaction of glacial flow, subglacial activity, and geothermal disturbance. The page’s reference to cycles of melting and refreezing, the Eternal Geyser, and possible subglacial lakes suggests that this lower hemisphere is not simply frozen in place, but repeatedly reworked over time. Bright material appears pooled in hollows and stretched across smoother basins, while darker rocky interruptions rise through the ice in ridges and broken masses. In mapped usage, Kyra Hollow, Bride’s Mirror Shelf, Benevolence Basin, and Hostward Rift help distinguish the principal southern basin, reflective shelf, enclosed depression, and fractured polar margin within this broader glacial environment.

	~~Taken as a whole,~~ the southern ~~hemisphere presents Erasmus as a cold, impact-dominated moon with permanent polar ice concentrated over an older cratered landscape. Its southern regions are defined by frozen~~ basin ~~systems~~, ~~fractured polar deposits~~, ~~rugged transition belts~~, and ~~exposed rocky interruptions~~ within ~~the~~ broader ~~ice cover~~.

	==Mythology==		==Mythology==

NewZimiaGov: /* Equatorial Regions */

2026-04-19T14:34:11Z

Equatorial Regions

← Older revision		Revision as of 14:34, 19 April 2026
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	==Equatorial Regions==		==Equatorial Regions==
	The Equatorial Regions of ~~'''~~Erasmus~~''' are dominated by dark~~ plains, ~~broad belts~~ of ~~pale~~ dust ~~or frost-stained material~~, and a ~~dense concentration~~ of ~~impact structures~~. ~~Much~~ of the ~~middle latitudes consist of low~~-~~reflectivity terrain spread between lighter basin fields~~ and ~~cratered plateaus~~. ~~Large~~ dark ~~provinces occupy~~ the ~~central equatorial belt~~, while ~~brighter plains~~ and ~~distinct crater clusters are concentrated across~~ the ~~western and eastern low latitudes~~.		The Equatorial Regions of Erasmus contain the broadest range of terrain on the moon. Dark basalt plains, lighter bands of dust, crater chains, and scattered broken uplands dominate much of the belt, giving the middle latitudes a mixed and heavily reworked appearance. Across the western equatorial zone, the smoother pale tract known as Mercy Planitia occupies one of the broadest open surfaces visible on the map. Just to its east lies Whisper Basin, a prominent circular depression that serves as the clearest mapped counterpart to the moon’s famous whispering crater. At the center of the equatorial belt stretches the Erasmian Expanse, a broad mid-latitude province whose alternating dark and pale surfaces give Erasmus much of its recognizable character from orbit. Cutting across the upper part of this belt is Charis Chasma, a long dark break applied to one of the clearest linear depressions on the moon, while Galen Reach marks the east-central transition from smoother basaltic surfaces into rougher and more cratered terrain. Farther east, the broken escarpment called Sophene Scarp defines one of the sharpest transitions in the equatorial regions.

	~~Several major craters define this region~~. Some ~~are~~ broad ~~basins with darker floors~~ and ~~bright interiors or rim deposits~~, while others are ~~more sharply bounded and surrounded~~ by ~~lighter ejecta or mantling. Pale surface material spreads across wide areas of the equator in irregular swaths~~, ~~especially around major impact features~~ and ~~across open plains~~. ~~This produces a strong contrast between exposed dark crust~~ and ~~lighter mantled~~ terrain.		The combination of basalt plains, fine golden dust, large impacts, and frequent dust-storm reworking gives the equatorial regions a layered and shifting appearance. Some areas remain broad and open, while others are interrupted by old crater walls, collapsed margins, and darker volcanic-looking ground. The named regions reflect that same complexity: Mercy Planitia and the Erasmian Expanse denote the broad open terrain, Whisper Basin preserves the most distinctive enclosed depression in the western equatorial belt, and Charis Chasma, Galen Reach, and Sophene Scarp correspond to some of the clearest cuts, transition zones, and sharper relief boundaries visible on the mapped surface. Taken together, the equatorial regions give Erasmus much of its visual identity: a cold, cratered moon whose central belt preserves both ancient impacts and later geological reshaping beneath drifting dust.

	~~The equatorial region contains the broadest uninterrupted exposures of Erasmus’s ancient surface. It~~ preserves the ~~moon’s large-scale impact history~~ in the ~~form~~ of ~~overlapping crater fields~~, ~~degraded rims~~, ~~ejecta blankets~~, ~~and wide regolith-covered plains extending across~~ much of ~~the hemisphere~~.

	==Southern Polar Regions==		==Southern Polar Regions==

NewZimiaGov: /* North Polar Regions */

2026-04-19T14:33:47Z

North Polar Regions

← Older revision		Revision as of 14:33, 19 April 2026
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	'''{{PAGENAME}}''' is the third major moon of the planet [[Nephele]] in the [[Atos System]].		'''{{PAGENAME}}''' is the third major moon of the planet [[Nephele]] in the [[Atos System]].
	==North Polar Regions==		==North Polar Regions==
	[[File:Erasmus2026Skin.jpeg\|200px\|thumb\|left\|The surface of Erasmus.]]		[[File:ErasmusLabelle2026.png\|200px\|thumb\|left\| A labelled map of the surface of Erasmus.]]
	The North Polar Regions of ~~'''~~Erasmus~~'''~~ are ~~dominated~~ by ~~an extensive ice cap~~ broken ~~by broad fractures, enclosed basins, rough frozen~~ uplands, and ~~clustered~~ fields of ~~steep ice formations~~. ~~The highest latitudes are covered in thick~~, ~~continuous ice~~, ~~but~~ the polar ~~surface is heavily disrupted rather than smooth~~. ~~Large cracks~~, ~~broken margins~~, and ~~uneven frozen plateaus divide~~ the ~~cap across much of~~ the ~~hemisphere~~.		[[File:Erasmus2026Skin.jpeg\|200px\|thumb\|left\|The surface of Erasmus, unlabelled.]]
			The North Polar Regions of Erasmus are defined by wide frost-bright expanses, broken uplands, and ancient ice fields that stretch across much of the upper hemisphere. In the far northwest, the subdued northern margin known as Penbellen Verge marks one of the clearest transitions between the moon’s darkest exposed ground and its high frozen polar terrain. Farther east, the pale and haze-softened zone called Lamplit Veil occupies a broad northern tract where bright material appears to gather over rougher ground and soften the sharper relief beneath. At the center of the northern hemisphere rises Koinon Crown, a large ice-dominated prominence that gives Erasmus one of its most recognizable polar forms from orbit. Beyond it, the elevated ground of Philanthros Rise stands out from the surrounding northern surface, while the jagged uplift and clustered heights of Amity Spires define one of the harshest and most broken sectors along the northeastern polar margin.

	~~Along the lower edge~~ of the ~~northern cap, the frozen surface gives way to darker exposed ground~~, ~~crater rims~~, and ~~broad transition zones where older terrain remains visible beneath or between the polar deposits~~. ~~Several dark~~-~~floored basins cut into the polar margin~~, ~~while isolated~~ bright ~~craters~~ and ~~smaller circular depressions~~ remain ~~embedded~~ in the ~~surrounding terrain~~. In ~~places~~, ~~sharp blade-like ice masses~~ and ~~clustered ridges rise above~~ the ~~surrounding frozen plains, giving the north a rugged and deeply broken character.~~		The overall character of the north is cold, reflective, and deeply stratified. Ancient ice, frost-covered mountains, and intermittent geothermal venting appear to have shaped a region where bright material gathers in sheets and overhangs while darker rocky interruptions remain exposed in bands and protrusions. The page’s reference to the mysterious Polar Light Column also reinforces the impression of a north that is not merely frozen, but singularly atmospheric in mood. In mapped usage, Penbellen Verge, Lamplit Veil, Koinon Crown, Philanthros Rise, and Amity Spires help distinguish the principal northern ice margin, frost-softened veil, central polar mass, eastern rise, and broken upland sector within this broader polar environment.

	~~The~~ northern ~~hemisphere combines permanent frozen cover with a heavily cratered and fractured underlying crust. Its high latitudes are defined by thick~~ ice, ~~disrupted margins~~, ~~embedded basins~~, and ~~scattered exposed terrain extending into the middle latitudes~~.

	==Equatorial Regions==		==Equatorial Regions==

NewZimiaGov: /* Southern Polar Regions */

2026-04-13T17:52:31Z

Southern Polar Regions

← Older revision		Revision as of 17:52, 13 April 2026
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	==Southern Polar Regions==		==Southern Polar Regions==
	The ~~South~~ Polar ~~region~~ of Erasmus ~~is characterized by its active glacial~~ and ~~geothermal phenomena~~. ~~This area experiences cycles of melting~~ and ~~refreezing due to geothermal heat from~~ the ~~moon's interior~~, ~~resulting in~~ a ~~landscape of shifting ice and dynamic geological activity~~. ~~The terrain features~~ smooth, ~~reflective ice fields interspersed with jagged~~ rocky ~~outcrops~~. ~~One of~~ the ~~most notable features~~ of the ~~South Pole is~~ the ~~"Eternal Geyser," a powerful geothermal vent that continuously erupts, sending jets of water vapor~~ and ~~ice particles~~ high ~~into the atmosphere~~. ~~These eruptions create temporary ice halos around~~ the ~~moon~~, ~~visible~~ as ~~faint rings when backlit by Nephele. Beneath~~ the ~~surface~~, ~~subglacial lakes~~, ~~heated by geothermal activity~~, ~~are believed to harbor unique microbial ecosystems~~, ~~making~~ the ~~South Pole a key area of interest for astrobiological research~~.		The Southern Polar Regions of '''Erasmus''' are brighter and more topographically varied than much of the equatorial surface. Broad frozen plains, enclosed icy basins, fractured margins, and rough polar uplands extend across the high southern latitudes. The southern cap is irregular and segmented, with embedded dark masses, broken shelves, and uneven frozen cover spread across a rugged underlying surface.

			Several large basins in the south contain smooth bright ice, while nearby ridges, exposed rocky masses, and cratered uplands project through the surrounding frozen terrain. Fractures and collapsed margins are common across the lower edge of the polar zone. In places the ice gathers within low basins and troughs; elsewhere it thins across rougher high ground and broken crater rims. This gives the south a segmented structure, with strong contrast between white frozen surfaces and darker exposed crust.

			Taken as a whole, the southern hemisphere presents Erasmus as a cold, impact-dominated moon with permanent polar ice concentrated over an older cratered landscape. Its southern regions are defined by frozen basin systems, fractured polar deposits, rugged transition belts, and exposed rocky interruptions within the broader ice cover.

	==Mythology==		==Mythology==

NewZimiaGov: /* Equatorial Regions */

2026-04-13T17:51:55Z

Equatorial Regions

← Older revision		Revision as of 17:51, 13 April 2026
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	==Equatorial Regions==		==Equatorial Regions==
	The Equatorial ~~region~~ of Erasmus is the ~~moon's most geologically dynamic~~ and ~~diverse area~~. ~~Receiving~~ the ~~most direct sunlight~~, this region ~~has relatively milder temperatures~~, ~~allowing for a variety of geological formations~~. ~~The landscape includes extensive basalt plains, remnants~~ of ~~ancient volcanic activity~~, and ~~patches of fine, golden dust~~. The ~~equator is home to~~ the ~~"Crater~~ of ~~Whispers," a massive impact crater that emits low-frequency sounds resembling whispers when the wind blows across its~~ surface. ~~This phenomenon is due to~~ the ~~unique acoustic properties~~ of ~~the~~ crater~~'s rocky walls and has fascinated researchers and explorers alike. Frequent dust storms~~, ~~driven by temperature fluctuations~~, ~~sweep across the plains~~, ~~revealing new geological features~~ and ~~contributing to~~ the ~~region's ever-changing appearance~~.		The Equatorial Regions of '''Erasmus''' are dominated by dark plains, broad belts of pale dust or frost-stained material, and a dense concentration of impact structures. Much of the middle latitudes consist of low-reflectivity terrain spread between lighter basin fields and cratered plateaus. Large dark provinces occupy the central equatorial belt, while brighter plains and distinct crater clusters are concentrated across the western and eastern low latitudes.

			Several major craters define this region. Some are broad basins with darker floors and bright interiors or rim deposits, while others are more sharply bounded and surrounded by lighter ejecta or mantling. Pale surface material spreads across wide areas of the equator in irregular swaths, especially around major impact features and across open plains. This produces a strong contrast between exposed dark crust and lighter mantled terrain.

			The equatorial region contains the broadest uninterrupted exposures of Erasmus’s ancient surface. It preserves the moon’s large-scale impact history in the form of overlapping crater fields, degraded rims, ejecta blankets, and wide regolith-covered plains extending across much of the hemisphere.

	==Southern Polar Regions==		==Southern Polar Regions==
	The South Polar region of Erasmus is characterized by its active glacial and geothermal phenomena. This area experiences cycles of melting and refreezing due to geothermal heat from the moon's interior, resulting in a landscape of shifting ice and dynamic geological activity. The terrain features smooth, reflective ice fields interspersed with jagged rocky outcrops. One of the most notable features of the South Pole is the "Eternal Geyser," a powerful geothermal vent that continuously erupts, sending jets of water vapor and ice particles high into the atmosphere. These eruptions create temporary ice halos around the moon, visible as faint rings when backlit by Nephele. Beneath the surface, subglacial lakes, heated by geothermal activity, are believed to harbor unique microbial ecosystems, making the South Pole a key area of interest for astrobiological research.		The South Polar region of Erasmus is characterized by its active glacial and geothermal phenomena. This area experiences cycles of melting and refreezing due to geothermal heat from the moon's interior, resulting in a landscape of shifting ice and dynamic geological activity. The terrain features smooth, reflective ice fields interspersed with jagged rocky outcrops. One of the most notable features of the South Pole is the "Eternal Geyser," a powerful geothermal vent that continuously erupts, sending jets of water vapor and ice particles high into the atmosphere. These eruptions create temporary ice halos around the moon, visible as faint rings when backlit by Nephele. Beneath the surface, subglacial lakes, heated by geothermal activity, are believed to harbor unique microbial ecosystems, making the South Pole a key area of interest for astrobiological research.

NewZimiaGov: /* North Polar Regions */

2026-04-13T17:51:40Z

North Polar Regions

← Older revision		Revision as of 17:51, 13 April 2026
Line 44:		Line 44:
	==North Polar Regions==		==North Polar Regions==
	[[File:Erasmus2026Skin.jpeg\|200px\|thumb\|left\|The surface of Erasmus.]]		[[File:Erasmus2026Skin.jpeg\|200px\|thumb\|left\|The surface of Erasmus.]]
	The North Polar ~~region~~ of Erasmus ~~is an enigmatic and icy expanse. This area is~~ dominated by ~~vast~~ ice ~~plains and rugged~~, ~~frost-covered mountains~~, ~~creating a landscape~~ of ~~stark beauty~~. The ~~region experiences extended periods of darkness due to the moon's axial tilt~~, ~~leading to bone-chilling temperatures. The~~ ice ~~here~~ is ~~ancient~~, ~~layered with history~~ and ~~occasionally disrupted by geothermal vents that release plumes~~ of ~~steam~~. ~~These vents create spectacular frost formations that catch~~ the ~~faint light from distant stars~~. ~~One of~~ the ~~most intriguing features of~~ the ~~North Pole is~~ the ~~"Polar Light Column~~," a ~~mysterious~~, ~~vertical beam of light that occasionally appears~~, ~~believed to be caused by unique magnetic interactions with Nephele's field~~, ~~though its exact nature remains a subject of intense study~~.		The North Polar Regions of '''Erasmus''' are dominated by an extensive ice cap broken by broad fractures, enclosed basins, rough frozen uplands, and clustered fields of steep ice formations. The highest latitudes are covered in thick, continuous ice, but the polar surface is heavily disrupted rather than smooth. Large cracks, broken margins, and uneven frozen plateaus divide the cap across much of the hemisphere.

			Along the lower edge of the northern cap, the frozen surface gives way to darker exposed ground, crater rims, and broad transition zones where older terrain remains visible beneath or between the polar deposits. Several dark-floored basins cut into the polar margin, while isolated bright craters and smaller circular depressions remain embedded in the surrounding terrain. In places, sharp blade-like ice masses and clustered ridges rise above the surrounding frozen plains, giving the north a rugged and deeply broken character.

			The northern hemisphere combines permanent frozen cover with a heavily cratered and fractured underlying crust. Its high latitudes are defined by thick ice, disrupted margins, embedded basins, and scattered exposed terrain extending into the middle latitudes.

	==Equatorial Regions==		==Equatorial Regions==

NewZimiaGov: /* North Polar Regions */

2026-04-12T21:21:31Z

North Polar Regions

← Older revision		Revision as of 21:21, 12 April 2026
Line 43:		Line 43:
	'''{{PAGENAME}}''' is the third major moon of the planet [[Nephele]] in the [[Atos System]].		'''{{PAGENAME}}''' is the third major moon of the planet [[Nephele]] in the [[Atos System]].
	==North Polar Regions==		==North Polar Regions==
			[[File:Erasmus2026Skin.jpeg\|200px\|thumb\|left\|The surface of Erasmus.]]
	The North Polar region of Erasmus is an enigmatic and icy expanse. This area is dominated by vast ice plains and rugged, frost-covered mountains, creating a landscape of stark beauty. The region experiences extended periods of darkness due to the moon's axial tilt, leading to bone-chilling temperatures. The ice here is ancient, layered with history and occasionally disrupted by geothermal vents that release plumes of steam. These vents create spectacular frost formations that catch the faint light from distant stars. One of the most intriguing features of the North Pole is the "Polar Light Column," a mysterious, vertical beam of light that occasionally appears, believed to be caused by unique magnetic interactions with Nephele's field, though its exact nature remains a subject of intense study.		The North Polar region of Erasmus is an enigmatic and icy expanse. This area is dominated by vast ice plains and rugged, frost-covered mountains, creating a landscape of stark beauty. The region experiences extended periods of darkness due to the moon's axial tilt, leading to bone-chilling temperatures. The ice here is ancient, layered with history and occasionally disrupted by geothermal vents that release plumes of steam. These vents create spectacular frost formations that catch the faint light from distant stars. One of the most intriguing features of the North Pole is the "Polar Light Column," a mysterious, vertical beam of light that occasionally appears, believed to be caused by unique magnetic interactions with Nephele's field, though its exact nature remains a subject of intense study.

	==Equatorial Regions==		==Equatorial Regions==
	The Equatorial region of Erasmus is the moon's most geologically dynamic and diverse area. Receiving the most direct sunlight, this region has relatively milder temperatures, allowing for a variety of geological formations. The landscape includes extensive basalt plains, remnants of ancient volcanic activity, and patches of fine, golden dust. The equator is home to the "Crater of Whispers," a massive impact crater that emits low-frequency sounds resembling whispers when the wind blows across its surface. This phenomenon is due to the unique acoustic properties of the crater's rocky walls and has fascinated researchers and explorers alike. Frequent dust storms, driven by temperature fluctuations, sweep across the plains, revealing new geological features and contributing to the region's ever-changing appearance.		The Equatorial region of Erasmus is the moon's most geologically dynamic and diverse area. Receiving the most direct sunlight, this region has relatively milder temperatures, allowing for a variety of geological formations. The landscape includes extensive basalt plains, remnants of ancient volcanic activity, and patches of fine, golden dust. The equator is home to the "Crater of Whispers," a massive impact crater that emits low-frequency sounds resembling whispers when the wind blows across its surface. This phenomenon is due to the unique acoustic properties of the crater's rocky walls and has fascinated researchers and explorers alike. Frequent dust storms, driven by temperature fluctuations, sweep across the plains, revealing new geological features and contributing to the region's ever-changing appearance.