Universal Cartographics Galactic Record Breakers

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LARGETS L-TYPE STAR
IC 1396 SECTOR GP-B C15-0 C WITH A SOLAR RADIUS OF 0.3953

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And some beauty shots, cause patau loves em so much
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And another

SMALLEST ROCKY PLANET
COL 173 SECTOR CI-G C12-4 2 A WITH A RADIUS OF 303 KM - FERRIS

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Added. BTW, do you want your forum nick or your CMDR name in the book? I've just noticed that you have your CMDR name in your sig.
 
today I found something I had never seen so far. A ringed t-tauri star. Well two actually in the same system. Just been unlucky so far. Or are they rather rare?


as well found

T-TAURI STAR WITH THE MOST BODIES
BYUA EUQ BA-A E38 5 WITH 10 BODIES CMDR TRAV ELER

ttauri_10moons.png
 
Added. BTW, do you want your forum nick or your CMDR name in the book? I've just noticed that you have your CMDR name in your sig.

I only just added it to my sig... yeah, why not, could you change my records to my CMDR name pls?.. Thanks for offering:)
 
Now let's see who discovers a rocky ice planet with 0.0001 Earth masses...

LIGHTEST ROCKY ICE PLANET
SMOJAI WW-N C6-10 1 A WITH 0.0002 EARTH MASSES - JACK LUMINOUS

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[edit] Stumbled upon a large, heavy L-type star:

LARGEST L-TYPE STAR
SMOJAI IM-F B11-1 A WITH A SOLAR RADIUS OF 0.3923 - JACK LUMINOUS

HEAVIEST L-TYPE STAR
SMOJAI IM-F B11-1 A WITH 0.2109 SOLAR MASSES - JACK LUMINOUS

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Not sure about this one as i haven't seen a system configuration like this before..

M-TYPE STAR WITH THE DEEPEST NESTING
CD-42 4620 IS A 4TH TIER

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If not the M star, then would the G at the top be 4th tier?
 
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Caps...

HOTTEST Y-TYPE STAR
HD 75258 4 WITH A TEMPERATURE OF 695K

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COLDEST CLASS IV GAS GIANT
HD 75258 6 A WITH A TEMPERATURE OF 807K

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What are they orbiting then, because they all have orbital periods in their stats?
Not arguing with your decision, just wondering...

I believe they are orbiting a centre of mass, the orbital period stats show orbital period around the centre of mass
this category was actually suggested by someone else its a bit complicated. Your looking for a star orbiting a star orbiting a star, etc. but binary's etc don't count.
I need to change the wording for category anyone got any suggestions
I will also try to find my old post on this for you
 
I believe they are orbiting a centre of mass, the orbital period stats show orbital period around the centre of mass
this category was actually suggested by someone else its a bit complicated. Your looking for a star orbiting a star orbiting a star, etc. but binary's etc don't count.
I need to change the wording for category anyone got any suggestions
I will also try to find my old post on this for you

Ahh.. i get it..
So A and B orbit about a single point, then C sits outside that orbit, but is still orbiting around the same central point. Then D would be in an even larger orbit around the same point again... etc. etc.

A difficult one to explain in a 4/5 word category title.
 
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Ahh.. i get it..
So A and B orbit about a single point, then C sits outside that orbit, but is still orbiting around the same central point. Then D would be in an even larger orbit around the same point again... etc. etc.

A difficult one to explain in a 4/5 word category title.

I think the centre of that system is between E and ABCD hang on let me draw a pic
 
  • Ender you asked me this question:

    SMALLEST B-TYPE STAR - R CORONAE AUSTRINI A SOLAR RADIUS OF 0.0132
    I strongly suspect there is an error in this record but I can't find any evidence that would support the record (actually, any post with the name of R CORONAE AUSTRINI in it). Rukmerot, would you, please, redirect me to it because if it's true I will add it to my ticket about errors in body properties (a star so small isn't a giant star).​
Here it is:

2nlh276.jpg

It emits vast amounts of enrgy once in a while so I personally think it is in the midst of collapsing, It has a huge ssolar mass 2 (10. 6211) so i hope i can get a screenshot when it does this again.

And as promised, here's the screenshot you requested (rukmerot still seems to have problems with his forum account).


EDIT: It seems that Rukmerots posts finally got through. He posted several answers for you here.

Thanks, I somehow missed Rukmerot's post.

Rukmerot, you mean its variable energy emissions are already seen in-game? That's great news for me!

Could this lead to stars changing their class?
Many stars are definitely need to change their class at some point because their temperature is consistent with real data (so they won't change it) but it is outside of range of their classification - they are wrongly classified now so they have wrong designations as eg. is in the case of R Coronae Austrini A (B III star should be larger not much smaller than B IV that is R Coronae Austrini B in-game) that don't match real world designations, as eg. Canopus (and it's still wrong in Release 1.1 Beta - A9 instead of F0)

What's really curious that the status of some planets will also change and some of them will even become stars (strong contender is Capella A 6 - but it's still a planet in Release 1.1 Beta).

Edit: the navigation search option looks like it's working properly, now!
 
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I think this is right:
VB6youw.jpg
Your system is actually centre of mass orbiting a centre of mass orbiting etc..


Thanks.. It makes sense.
The only other way I can think of to word the category is 'xxxx with deepest non-barycentric orbital nesting', bit of a mouthful though.
 
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