Pyros - Revision history

NewZimiaGov at 17:37, 18 October 2026

2026-10-18T17:37:00Z

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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:~~Pyros12~~.png\|100px]]		\| [[Image:Pyros1018.png\|100px]]
	\|}		\|}
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NewZimiaGov at 01:53, 13 October 2026

2026-10-13T01:53:25Z

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	{\| 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:~~Pyros1012F~~.png\|100px]]		\| [[Image:Pyros12.png\|100px]]
	\|}		\|}
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NewZimiaGov at 01:24, 13 October 2026

2026-10-13T01:24:00Z

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	{\| 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:~~Pyros628~~.png\|100px]]		\| [[Image:Pyros1012F.png\|100px]]
	\|}		\|}
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NewZimiaGov at 16:57, 28 June 2026

2026-06-28T16:57:26Z

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	{\| 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:~~Pyros627~~.png\|100px]]		\| [[Image:Pyros628.png\|100px]]
	\|}		\|}
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NewZimiaGov at 01:43, 28 June 2026

2026-06-28T01:43:24Z

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	{\| 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:~~Pyros510B~~.png\|100px]]		\| [[Image:Pyros627.png\|100px]]
	\|}		\|}
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NewZimiaGov: /* Ring System */

2026-05-12T18:30:57Z

Ring System

← Older revision		Revision as of 18:30, 12 May 2026
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	==Ring System==		==Ring System==
	[[File:PyrosSurface.jpeg\|200px\|thumb\|left\|The rings of Pyros extend overhead in this photo - taken by a top-secret New Zimian rover - ~~over~~ the Pyrotian surface.]]		[[File:PyrosSurface.jpeg\|200px\|thumb\|left\|The rings of Pyros extend overhead in this photo - taken by a top-secret New Zimian rover - on the Pyrotian surface.]]
	Pyros possesses a faint and comparatively narrow ring system encircling the planet near its equatorial plane. Unlike the broad, highly reflective rings associated with larger gas giants, the Pyrotian rings are composed of sparse particulate material and are generally difficult to observe except under favorable lighting conditions. Survey imagery indicates that the rings are dominated by sand-sized and dust-sized silicate grains, mixed with darker basaltic fragments and lighter mineral particles similar in color to the planet's exposed plains, volcanic fields, and frost-bright deposits.		Pyros possesses a faint and comparatively narrow ring system encircling the planet near its equatorial plane. Unlike the broad, highly reflective rings associated with larger gas giants, the Pyrotian rings are composed of sparse particulate material and are generally difficult to observe except under favorable lighting conditions. Survey imagery indicates that the rings are dominated by sand-sized and dust-sized silicate grains, mixed with darker basaltic fragments and lighter mineral particles similar in color to the planet's exposed plains, volcanic fields, and frost-bright deposits.

NewZimiaGov: /* Ring System */

2026-05-12T16:33:53Z

Ring System

← Older revision		Revision as of 16:33, 12 May 2026
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	==Ring System==		==Ring System==
			[[File:PyrosSurface.jpeg\|200px\|thumb\|left\|The rings of Pyros extend overhead in this photo - taken by a top-secret New Zimian rover - over the Pyrotian surface.]]
	Pyros possesses a faint and comparatively narrow ring system encircling the planet near its equatorial plane. Unlike the broad, highly reflective rings associated with larger gas giants, the Pyrotian rings are composed of sparse particulate material and are generally difficult to observe except under favorable lighting conditions. Survey imagery indicates that the rings are dominated by sand-sized and dust-sized silicate grains, mixed with darker basaltic fragments and lighter mineral particles similar in color to the planet's exposed plains, volcanic fields, and frost-bright deposits.		Pyros possesses a faint and comparatively narrow ring system encircling the planet near its equatorial plane. Unlike the broad, highly reflective rings associated with larger gas giants, the Pyrotian rings are composed of sparse particulate material and are generally difficult to observe except under favorable lighting conditions. Survey imagery indicates that the rings are dominated by sand-sized and dust-sized silicate grains, mixed with darker basaltic fragments and lighter mineral particles similar in color to the planet's exposed plains, volcanic fields, and frost-bright deposits.

NewZimiaGov at 03:09, 11 May 2026

2026-05-11T03:09:18Z

← Older revision		Revision as of 03:09, 11 May 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:~~Pyros510~~.png\|100px]]		\| [[Image:Pyros510B.png\|100px]]
	\|}		\|}
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NewZimiaGov at 20:05, 10 May 2026

2026-05-10T20:05:00Z

← Older revision		Revision as of 20:05, 10 May 2026
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	\|'''Orbital Speed (Km/s)''' \|\| 28.4		\|'''Orbital Speed (Km/s)''' \|\| 28.4
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	\|~~'''~~Satellites~~''' \|\|~~ None		\|Satellites = None; faint silicate dust rings
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	\| align=center colspan=2 style="background: #c0c0ff; text-align:center;"\| '''Atmospheric Characteristics'''		\| align=center colspan=2 style="background: #c0c0ff; text-align:center;"\| '''Atmospheric Characteristics'''
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	\|}		\|}

	~~'''~~Pyros~~''' is the~~ is the planet third closest to the star [[Atos]].		Pyros is the planet third closest to the star [[Atos]]. Although long regarded as a satellite-less terrestrial world, later survey observations confirmed the presence of a faint equatorial ring system composed primarily of fine silicate dust, basaltic grains, and pale mineral-rich particulate matter. The rings are extremely diffuse compared to the prominent ring systems of the outer planets, appearing only as a narrow, sandy-grey band under favorable illumination. Their coloration broadly corresponds to the surface of Pyros itself, with muted tones of ash-grey, tan, beige, charcoal, and frost-pale mineral dust.

			==Ring System==
			Pyros possesses a faint and comparatively narrow ring system encircling the planet near its equatorial plane. Unlike the broad, highly reflective rings associated with larger gas giants, the Pyrotian rings are composed of sparse particulate material and are generally difficult to observe except under favorable lighting conditions. Survey imagery indicates that the rings are dominated by sand-sized and dust-sized silicate grains, mixed with darker basaltic fragments and lighter mineral particles similar in color to the planet's exposed plains, volcanic fields, and frost-bright deposits.

			The prevailing interpretation among researchers is that the ring system represents the remains of an ancient minor satellite or captured asteroid which was disrupted by tidal stress, collision, or gradual fragmentation. Larger fragments appear either to have fallen into Pyros, escaped stable orbit, or been reduced over time into the present diffuse band of debris. Because no large surviving natural satellites are known, the ring system is regarded as the principal circumplanetary structure of Pyros rather than as part of a wider moon system.

			Visually, the rings display a muted palette of pale beige, taupe, ashen grey, charcoal, and off-white material. This coloration closely corresponds to the observed surface of Pyros, particularly its mixture of light dusty plains, dark volcanic or basaltic terrain, and frost-washed polar deposits. The correspondence has led some researchers to suggest that a portion of the ring material may have originated from ancient impact ejecta launched from the Pyrotian surface, although this remains less widely accepted than the disrupted-moonlet hypothesis.

			The rings are not believed to be especially massive or permanent on geological timescales. Their fine particulate composition makes them vulnerable to gradual orbital decay, solar radiation effects, and collisional grinding. Nevertheless, the continued presence of the ring system suggests either that the disruption event was relatively recent in astronomical terms, or that the rings are intermittently replenished by micrometeorite impacts on small embedded fragments too minor to be classified as true satellites.

	==North Polar Regions==		==North Polar Regions==

NewZimiaGov at 20:02, 10 May 2026

2026-05-10T20:02:30Z

← Older revision		Revision as of 20:02, 10 May 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:~~Pyros2026B~~.png\|100px]]		\| [[Image:Pyros510.png\|100px]]
	\|}		\|}
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