Are you guys using any tools for logging and collecting data about the star systems you visit ?
My desk is cluttered with pen and papers.
Are you guys using any tools for logging and collecting data about the star systems you visit ?
OLDEST T-TYPE
SYNUEFAI NU-M B12-0 C AT 18,025 MILLION YEARS CMDR NATALIE PORTMAN
Are you guys using any tools for logging and collecting data about the star systems you visit ?
I'm starting to wonder...is it even possible to get ice planets surface temperature lower than 20k?
I say that because I just found this system -
Every single one of these planets is an ice planet orbiting a Class T dwarf of 831K. The furthest planet out is 15.3AU, yet has the same temperature as the closest planet to the sun.
Is 20K rock bottom for icey planets?
A couple more to throw into the mix...
COLDEST METAL RICH PLANET - HIP 60459 2 B - SURFACE TEMPERATURE OF 1,015K
COLDEST CLASS III GAS GIANT - HR 4485 4 - SURFACE TEMPERATURE 248K
It looks like 20K is the lower limit for all non-gas giants, for some reason.I'm starting to wonder...is it even possible to get ice planets surface temperature lower than 20k?
I say that because I just found this system -
View attachment 13581
Every single one of these planets is an ice planet orbiting a Class T dwarf of 831K. The furthest planet out is 15.3AU, yet has the same temperature as the closest planet to the sun.
Is 20K rock bottom for icey planets?
All I say is that such small stars shouldn't be designated as B III (giants of B-type). I don't know where you have found information about R Coronae Austrini A being on the verge of transition to a white dwarf (I couldn't see it in the link you provided) but if it is R Coronae Australis from the real world then it's a very young pre-main sequence star classified as Herbig Ae/Be of spectral and luminosity type B8 II (or B5 III is in-game, depending on source). You could see it here. Thus, if those stars are the same then the size of R Coronae Austrini A is definitely a bug as is probably the size of BD+08 1303 A. Thanks for finding them.Ender I found another b- type that is in transision its a bit bigger, but I a managed to get my raptr recorder going,
BD+08 1303 A
https://www.youtube.com/watch?v=-NuSll3luFM&feature=youtu.be
A couple more to throw into the mix...
COLDEST METAL RICH PLANET - HIP 60459 2 B - SURFACE TEMPERATURE OF 1,015K
COLDEST CLASS III GAS GIANT - HR 4485 4 - SURFACE TEMPERATURE 248K
Sorry, but you shouldn't in the second case - it's a class II gas giant not class III. Fortunately, this issue is already corrected in Release 1.1 Beta. Unfortunately, descriptions of metal-rich and high metal content planets aren't, yet.ADDED TO THE BOOKS
It looks like 20K is the lower limit for all non-gas giants, for some reason.
All I say is that such small stars shouldn't be designated as B III (giants of B-type). I don't know where you have found information about R Coronae Austrini A being on the verge of transition to a white dwarf (I couldn't see it in the link you provided) but if it is R Coronae Australis from the real world then it's a very young pre-main sequence star classified as Herbig Ae/Be of spectral and luminosity type B8 II (or B5 III is in-game, depending on source). You could see it here. Thus, if those stars are the same then the size of R Coronae Austrini A is definitely a bug as is probably the size of BD+08 1303 A. Thanks for finding them.
Sorry, but you shouldn't in the second case - it's a class II gas giant not class III. Fortunately, this issue is already corrected in Release 1.1 Beta. Unfortunately, descriptions of metal-rich and high metal content planets aren't, yet.
Edit: BTW, perhaps some of you would like to join discussion about First Discovered tag, here, as it is going probably to have great impact on our behavior in-game. Unfortunately, the only reason currently to surface-scan objects is the book and with Release 1.1 it looks like we will even have more incentives to NOT surface-scan objects.
that's more like it! not bad 19,000k from sol are you on your way to sag* and beyond?New record (sorry Hozzdutch)
Old record;
FURTHEST TERRAFORMABLE HIGH METAL CONTENT PLANET FROM SOL
HIP 63835 CD 3 AT 275.46LY
New record;
FURTHEST TERRAFORMABLE HIGH METAL CONTENT PLANET FROM SOL
DRYAU SCRAA WD-K D8-677 C1, C2, C3 AND C4 AT 19,027.53LY - CMDR CALBARON
Crazy system has 4 Terraformable HMC planets, 1 Terraformable water world and 1 Earthlike, all orbiting the same sun (and a Neutron star in the system too)
ok, so I've found a 'red giant' star.
There doesn't appear to be a category for this one...is is it named something else?