Rirhath B - Revision history

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2021-01-30T09:45:03Z

12 revisions imported

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newimport>DianeDuane at 13:16, 31 May 2010

2010-05-31T13:16:22Z

Import>DianeDuane at 13:16, 31 May 2010

2010-05-31T13:16:22Z

newimport>DianeDuane at 15:54, 24 January 2010

2010-01-24T15:54:57Z

newimport>DianeDuane at 12:06, 24 January 2010

2010-01-24T12:06:13Z

newimport>DianeDuane at 09:52, 7 May 2008

2008-05-07T09:52:43Z

newimport>DianeDuane at 20:06, 5 May 2008

2008-05-05T20:06:55Z

newimport>DianeDuane at 21:56, 19 May 2005

2005-05-19T21:56:40Z

newimport>DianeDuane at 20:56, 20 March 2005

2005-03-20T20:56:12Z

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 Rirhath B's population is described in [[WAW]] as relatively small: on any given day, its population of transient aliens will far outnumber the world's actual residents.  ([[HW]], [[TBONWM]] ''et al.'')
-*Despite the nomenclature, this is not a secondary body or a planet of a binary star: the "B" refers to a Rirhait naming convention expressing a cultural referent difficult to translate into many  [[language of discourse | languages of discourse]].
+*Despite the nomenclature, this is not a secondary body or a planet of a binary star: the "B" refers to a Rirhait naming convention expressing a cultural referent difficult to translate into many  [[Discourse, language of | languages of discourse]].
 [[Category:Locations]]
 [[Category:Planets]]
 [[Category:Textual oddities]]

← Older revision		Revision as of 15:54, 24 January 2010
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−	(Also "Rirhath B vi") Sixth planet of eight in the [[Rirhath]] system; home planet of the [[Crossings Intercontinual Worldgating Facility]] and origin planet of the [[Rirhait]] species.*	+	[[Image:Rirhath B Close.jpg\|thumb\|right\|300px\|Rirhath B, showing the Khe'tek continent where the [[Crossings Intercontinual Worldgating Facility \| Crossings]] is located]](Also "Rirhath B vi") Sixth planet of eight in the [[Rirhath]] system; home planet of the [[Crossings Intercontinual Worldgating Facility]] and origin planet of the [[Rirhait]] species.*

	In [[HW]], Rirhath B is identified as a planet of [http://www.solstation.com/stars/eps-indi.htm epsilon Indi] by [[Callahan, Dairine \| Dairine's]] newly cloned computer, which gives the right distance to that star in lightyears. However, this identification seems in retrospect to be incorrect, as the space around Rirhath B, later observed by [[Kit]] and [[Nita]] as being full of short-term variable stars, does not match the space observable around ε Indi. The fluorescence of the planet's daytime atmosphere also does not match up with what might be expected in the neighborhood of a [http://www.daviddarling.info/encyclopedia/K/Kstar.html type K star] slightly cooler than Earth's sun. Explanations for what is either an error in target identification or in the computer's interstellar gating routines are difficult to come by at this stage, but there is always the possibility that the cloning procedure that Dairine used on the computer was flawed, producing the equivalent of a crosslinked file or similar disk error. Also, the [[Manual software]] is explicitly stated in [[HW]] to be in a beta release, so it is also possible that the computer's atlas functions were impaired by some deeply buried bug in its ID routines. Yeah, that's the ticket.		In [[HW]], Rirhath B is identified as a planet of [http://www.solstation.com/stars/eps-indi.htm epsilon Indi] by [[Callahan, Dairine \| Dairine's]] newly cloned computer, which gives the right distance to that star in lightyears. However, this identification seems in retrospect to be incorrect, as the space around Rirhath B, later observed by [[Kit]] and [[Nita]] as being full of short-term variable stars, does not match the space observable around ε Indi. The fluorescence of the planet's daytime atmosphere also does not match up with what might be expected in the neighborhood of a [http://www.daviddarling.info/encyclopedia/K/Kstar.html type K star] slightly cooler than Earth's sun. Explanations for what is either an error in target identification or in the computer's interstellar gating routines are difficult to come by at this stage, but there is always the possibility that the cloning procedure that Dairine used on the computer was flawed, producing the equivalent of a crosslinked file or similar disk error. Also, the [[Manual software]] is explicitly stated in [[HW]] to be in a beta release, so it is also possible that the computer's atlas functions were impaired by some deeply buried bug in its ID routines. Yeah, that's the ticket.

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-Home planet of the [[Crossings Intercontinual Worldgating Facility]], and origin planet of the [[Rirhait]] species.
+(Also "Rirhath B vi") Sixth planet of eight in the [[Rirhath]] system; home planet of the [[Crossings Intercontinual Worldgating Facility]] and origin planet of the [[Rirhait]] species.*
 In [[HW]], Rirhath B is identified as a planet of [http://www.solstation.com/stars/eps-indi.htm epsilon Indi] by [[Callahan, Dairine | Dairine's]] newly cloned computer, which gives the right distance to that star in lightyears. However, this identification seems in retrospect to be incorrect, as the space around Rirhath B, later observed by [[Kit]] and [[Nita]] as being full of short-term variable stars, does not match the space observable around &#949; Indi.  The fluorescence of the planet's daytime atmosphere also does not match up with what might be expected in the neighborhood of a [http://www.daviddarling.info/encyclopedia/K/Kstar.html type K star] slightly cooler than Earth's sun. Explanations for what is either an error in target identification or in the computer's interstellar gating routines are difficult to come by at this stage, but there is always the possibility that the cloning procedure that Dairine used on the computer was flawed, producing the equivalent of a crosslinked file or similar disk error. Also, the [[Manual software]] is explicitly stated in [[HW]] to be in a beta release, so it is also possible that the computer's atlas functions were impaired by some deeply buried bug in its ID routines. Yeah, that's the ticket.
-...In [[TBONWM]], Rirhath B is identified as the sixth planet out from its primary.  The planet's population is described in [[WAW]] as relatively small: on any given day, its population of transient aliens will far outnumber the world's actual residents.  ([[HW]] ''et al.'')
+Rirhath B's population is described in [[WAW]] as relatively small: on any given day, its population of transient aliens will far outnumber the world's actual residents.  ([[HW]], [[TBONWM]] ''et al.'')
 [[Category:Locations]]
 [[Category:Planets]]
 [[Category:Textual oddities]]

← Older revision		Revision as of 09:52, 7 May 2008
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	[[Category:Locations]]		[[Category:Locations]]
	[[Category:Planets]]		[[Category:Planets]]
		+	[[Category:Textual oddities]]

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 Home planet of the [[Crossings Intercontinual Worldgating Facility]], and origin planet of the [[Rirhait]] species.
 In [[HW]], Rirhath B is identified as a planet of [http://www.solstation.com/stars/eps-indi.htm epsilon Indi] by [[Callahan, Dairine | Dairine's]] newly cloned computer, which gives the right distance to that star in lightyears. However, this identification seems in retrospect to be incorrect, as the space around Rirhath B, later observed by [[Kit]] and [[Nita]] as being full of short-term variable stars, does not match the space observable around &#949; Indi.  The fluorescence of the planet's daytime atmosphere also does not match up with what might be expected in the neighborhood of a [http://www.daviddarling.info/encyclopedia/K/Kstar.html type K star] slightly cooler than Earth's sun. Explanations for what is either an error in target identification or in the computer's interstellar gating routines are difficult to come by at this stage, but there is always the possibility that the cloning procedure that Dairine used on the computer was flawed, producing the equivalent of a crosslinked file or similar disk error. Also, the [[Manual software]] is explicitly stated in [[HW]] to be in a beta release, so it is also possible that the computer's atlas functions were impaired by some deeply buried bug in its ID routines. Yeah, that's the ticket.
 ...In [[TBONWM]], Rirhath B is identified as the sixth planet out from its primary.  The planet's population is described in [[WAW]] as relatively small: on any given day, its population of transient aliens will far outnumber the world's actual residents.  ([[HW]] ''et al.'')

← Older revision	Revision as of 09:45, 30 January 2021
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← Older revision	Revision as of 09:21, 30 January 2021
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← Older revision	Revision as of 13:16, 31 May 2010
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← Older revision		Revision as of 21:56, 19 May 2005
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	In [[HW]], Rirhath B is identified as a planet of [http://www.solstation.com/stars/eps-indi.htm epsilon Indi] by [[Callahan, Dairine \| Dairine's]] newly cloned computer, which gives the right distance to that star in lightyears. However, this identification seems in retrospect to be incorrect, as the space around Rirhath B, later observed by [[Kit]] and [[Nita]] as being full of short-term variable stars, does not match the space observable around ε Indi. The fluorescence of the planet's daytime atmosphere also does not match up with what might be expected in the neighborhood of a [http://www.daviddarling.info/encyclopedia/K/Kstar.html type K star] slightly cooler than Earth's sun. Explanations for what is either an error in target identification or in the computer's interstellar gating routines are difficult to come by at this stage, but there is always the possibility that the cloning procedure that Dairine used on the computer was flawed, producing the equivalent of a crosslinked file or similar disk error. Also, the [[Manual software]] is explicitly stated in [[HW]] to be in a beta release, so it is also possible that the computer's atlas functions were impaired by some deeply buried bug in its ID routines. Yeah, that's the ticket.		In [[HW]], Rirhath B is identified as a planet of [http://www.solstation.com/stars/eps-indi.htm epsilon Indi] by [[Callahan, Dairine \| Dairine's]] newly cloned computer, which gives the right distance to that star in lightyears. However, this identification seems in retrospect to be incorrect, as the space around Rirhath B, later observed by [[Kit]] and [[Nita]] as being full of short-term variable stars, does not match the space observable around ε Indi. The fluorescence of the planet's daytime atmosphere also does not match up with what might be expected in the neighborhood of a [http://www.daviddarling.info/encyclopedia/K/Kstar.html type K star] slightly cooler than Earth's sun. Explanations for what is either an error in target identification or in the computer's interstellar gating routines are difficult to come by at this stage, but there is always the possibility that the cloning procedure that Dairine used on the computer was flawed, producing the equivalent of a crosslinked file or similar disk error. Also, the [[Manual software]] is explicitly stated in [[HW]] to be in a beta release, so it is also possible that the computer's atlas functions were impaired by some deeply buried bug in its ID routines. Yeah, that's the ticket.

−	~~{{stub}}~~	+	...In [[TBONWM]], Rirhath B is identified as the sixth planet out from its primary. The planet's population is described in [[WAW]] as relatively small: on any given day, its population of transient aliens will far outnumber the world's actual residents. ([[HW]] ''et al.'')