Chrislyannenar

(Yes, Stars are now planets, shut up.)
==Chrislyannenar's Stelliet==
===Condensed Summary===
Standard blue star, a small planetary system, and an asteroid belt that may or may not turn into a future dwarf planet. 
===Trivia===
*I am using this article to develop a format for a format for stars.
*Somehow the planet box is better then the star box.
*This was originally going to be a Wolf-Rayet star, but they take too long to find.
===Featurals===
There are not that many key features of a star besides that it has a bright blue color in its corona, its whitish in stellar appearance, and its bright. It is also smooth and circular texture. The flares do not go that far as well, and are few and far between.
===Planetary system summary===
Just a few hot small worlds and a thin debris ring which acts like an asteroid belt.
==Chrislyannenar's Physicals==
This star has an equatorial diameter of 3404157.22 miles, with the man diameter being 3404157.22 miles, and the polar diameter is 3404157.22 miles. The oblateness of this star is 0, with the mass being 19.772 M⨀, and the density is 0.45666 grams per cubic centimeter. The insolation is nothing, with the effective temperature being 38250 kelvin, and the Earth similarity index is nothing as well. The solar day is nothing, with the axial tilt of it being 100*17’2.69”. The gravity on the equator is 349.96 meters per second, with the gravity on average being 349.22 meters per second,  and the gravity on the poles is 349.22 meters per second. The circular velocity is 2187839.61 miles per hour, with the escape velocity being 3094072.28 miles per hour, and the age of the star is 2.2 million years, additionally, the lifetime is around the same, though is estimated to be a few more million years (4 - 5), plus the tidal heating of the thing is nothing.
==Chrislyannenar's Gallery==
File:Chrislyannenar-001.png
File:Chrislyannenar-007.png
File:Chrislyannenar-002.png
File:Chrislyannenar-010.png
File:Chrislyannenar-005.png
File:Chrislyannenar-003.png
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File:Chrislyannenar-009.png
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File:Chrislyannenar-008.png
== Chrislyannenar's Entras ==
=== Planetary System ===
This star has a small planetary system around it. Nothing really to note here, all of them are of a small size for their class  all of the planets around this star, asteroids included, are scorching hot, and all of the planets orbit relatively close to the star. This whole system is smaller than 6.75 AU, and is rather simplistic with its assets, only 3 planets and a debris disc which is masquerading as an asteroid belt. No oort cloud can be found in this system. The system’s asteroid belt goes from the 1st and 2nd positions, more specifically, it takes up the space directly behind the 1st orbit and goes halfway to the 2nd orbit, in which the density dramatically decreases. 
This asteroid belt may form into a future dwarf planet given enough time, and it will have a similar mass to Ceres, though considerably smaller. This system, excluding the central star, has a combined mass of ~13 Earths. This system is believed to have just exited the primordial formation phase of the stellar life cycle, which explains the formative fragments remaining in a position which would form an object of some kind. That future dwarf planet will also have a lot of gold considering the composition of the asteroid belt. The planets in this planetary system are also evenly spaced out from each other, follow circular orbits, and all roughly follow a stellar plane. 
Stats 	Broda'huy'rusta 	Koliunorridae 	Te'vas'anne
Image 	
File:Chrislyannenar-011.png	
File:Chrislyannenar-012.png	
File:Chrislyannenar-013.png
Class 	Torrid arid subterra	Torrid neptune	Torrid arid terra
Mass 	0.12531 M⨁ 	12.115 M⨁ 	0.52948 M⨁
Diameter	4271.66 Miles 	20372.68 Miles	6513.56 Miles
Orbital 	140.290d 	1.523y 	3.267y
=== Local system ===
This star is on the fringes of a star cluster, orbiting it at a fair distance from the core, though not far enough that the star can see stars not part of the cluster when looking away from the said star cluster’s center. Because of the star cluster parentage, the star’s local area is dense, not core dense, but dense enough that there is already star within 0.70 light years of it, that being a small red dwarf system. Add to that that there is a planemo near the system which is 0.35 light years away. It however is most likely an ejected planet from this star’s system, which would explain an oddity with the 3rd planet’s orbit. The star is the brightest in its local area and can be seen by every star provided that this one is not covered up by other stars. This star’s local area is dense and average for a star cluster. 
File:Chrislyannenar-014.png|"Local area" if it is defined as a ~10 ly diameter.
== Chrislyannenar's Axternalities ==
=== Representation ===
This star is not represented by any part of common culture. Since it is in a far away galaxy in a random star cluster, and since it is not host to any real unique qualities, it is seen as another “blue star”, if it is even noted in any way. The most representation it got was in a “Survey Review” podcast episode which mentioned this star in a long list of “Average O class stars.”. 
=== Sorting ===
This star is sorted as SC441-13 in the survey it was original found in, and it was later named and sorted into its current name a year later. It is also sorted as being part of the “CENTRALREG” area of the NGC 6872 galaxy, so just raw searching the thing in the survey’s database won't turn up any results. 
=== Studies ===
There are no studies specific to this star, though there is one which mentions this star as a data point (3*). A 2023 study on star formation in the NGC 6872 galaxy used this star as a small data point, as previously mentioned, in reference to the commonality of Blue supergiants in star clusters. It was also named in a “total list” of all the stars used, and was also used as a data point when describing the star formation patterns of O class stars outside of the main spirals. 
== Sources ==
# NGC6872GENSURVEY.catalog/Centralreg/Clusters/SC441/SC441-13/Ascriptions
# NGC6872GENSURVEY.catalog/Centralreg/Clusters/SC441/SC441-13/Exoplanets
# Vemal, L. M., Christian S. C., Gordon F. D., Ramel Q.N. (2023). Look On Star Formation, Presence Of Star Types, Placement, And Outlook In NGC 6872 Galaxy. The Astrophysical Journal, 399(10), 406(5), 100(1).
# IAU/Namingof/Chrislyannenar
Category:Procedural objects
Category:Objects
Category:Stars