This month I started teaching myself how to do some basic python, using the dumps from Spansh (thanks Spansh!).
I've been investigating the makeup of the galaxy, probably just rediscovering all this stuff you guys already knew. Anyway, here's some of it for your amusement.
I started with learning some basic charts - here's the average makeup of discovered systems
Here's the average value of a system assuming you only DSS the metal-rich and above bodies
or here's where Helium rich gas giants were found:
Then I taught myself heat maps, and started counting up interesting information up in 100ly * 100ly areas.
So for instance, here's the proportion of discovered bodies that are high metal content
And here's the proportion of discovered stars that are Neutron Stars
Here's the O types
And here's where the Helium Rich gas giants were found
And here was the averaged value of each region - scanned systems were most valuable on average in the core and on the rim, though some of that is player behaviour driven I guess:
Then I taught myself some animations.
Here's the age of the stars
Here's the last 4 years exploration
And here's the number of systems discovered in each 100ly * 100ly area.
Here's a similar animated heatmap, showing the number of discovered systems but scanning the galaxy from top to bottom in 100ly thick slices.
Note (which I'm sure lots of you already knew) there are some stars in that dump which have no scanned bodies that were imported from the real world catalogues, I only discovered that while doing that heatmap slicing the galaxy. Here's their distribution (x axis is 100s of ly above or below the plane of the galaxy). The spike of 13 stars 11,200 ly below the plane contains pulsars like PSR J0024-7204I from globular cluster 47 Tuc. Someone else actually spotted these a few years ago and posted on Inara about them here.
Anyway, then day before yesterday I discovered this thing called a pointcloud. So I've been visualising stuff like
The three layers of neutron stars, with the obvious gap just below +1000 and above -1000ly from the plane.
Here's a closeup of that lesser known stellar forge gap (at least to me) separate from the main cross
Or spotting that there are paths taken that are clearly a few hundred ly away from the bulk of the discovered galaxy, leading me to suspect there's still profitable routes on the rim just a bit further coreward than that
And I started playing around with transparency, highlighting the areas with lots of systems discovered
Or just showing the same but just masking off stuff you're not interested in instead of using transparency
So now instead of a heatmap of where the helium rich gas giants are, I can show an animation
Or do similar for black holes
or Wolf-Rayets
I was also playing around with relative density plots, this following data isn't from the entire galaxy, just a 2200 system jaunt I took last year before I discovered teh public exploration dumps, so it's maybe not very representative. I'll redo it sometime with a large sample size.
Here's stellar magnitudes:
Surface temperatures
Terrestrial surface temperatures
The ages of the few stars I discovered
And here's stellar masses
Star sizes
Planet sizes
Terrestrial planet sizes
Large body masses
Terrestrial body masses
Surface Gravity
Terrestrial surface gravity
Planets per system type
Planets per star or barycenter type within the systems
Oh, I quite like this visualization I did of the travel route I took
I could go on, but you get the idea. I'll probably redo the relative density plots at some point with galaxy wide data, and make a few more 3d rotating galaxy visualizations of stuff.
Before you give out to me about the length of this post, my excuse is CMDR Marx made me do it!
I've been investigating the makeup of the galaxy, probably just rediscovering all this stuff you guys already knew. Anyway, here's some of it for your amusement.
I started with learning some basic charts - here's the average makeup of discovered systems

Here's the average value of a system assuming you only DSS the metal-rich and above bodies

or here's where Helium rich gas giants were found:

Then I taught myself heat maps, and started counting up interesting information up in 100ly * 100ly areas.
So for instance, here's the proportion of discovered bodies that are high metal content

And here's the proportion of discovered stars that are Neutron Stars

Here's the O types

And here's where the Helium Rich gas giants were found

And here was the averaged value of each region - scanned systems were most valuable on average in the core and on the rim, though some of that is player behaviour driven I guess:

Then I taught myself some animations.
Here's the age of the stars
Here's the last 4 years exploration
And here's the number of systems discovered in each 100ly * 100ly area.
Here's a similar animated heatmap, showing the number of discovered systems but scanning the galaxy from top to bottom in 100ly thick slices.
Note (which I'm sure lots of you already knew) there are some stars in that dump which have no scanned bodies that were imported from the real world catalogues, I only discovered that while doing that heatmap slicing the galaxy. Here's their distribution (x axis is 100s of ly above or below the plane of the galaxy). The spike of 13 stars 11,200 ly below the plane contains pulsars like PSR J0024-7204I from globular cluster 47 Tuc. Someone else actually spotted these a few years ago and posted on Inara about them here.

Anyway, then day before yesterday I discovered this thing called a pointcloud. So I've been visualising stuff like
The three layers of neutron stars, with the obvious gap just below +1000 and above -1000ly from the plane.
Here's a closeup of that lesser known stellar forge gap (at least to me) separate from the main cross
Or spotting that there are paths taken that are clearly a few hundred ly away from the bulk of the discovered galaxy, leading me to suspect there's still profitable routes on the rim just a bit further coreward than that
And I started playing around with transparency, highlighting the areas with lots of systems discovered
Or just showing the same but just masking off stuff you're not interested in instead of using transparency
So now instead of a heatmap of where the helium rich gas giants are, I can show an animation
Or do similar for black holes
or Wolf-Rayets
I was also playing around with relative density plots, this following data isn't from the entire galaxy, just a 2200 system jaunt I took last year before I discovered teh public exploration dumps, so it's maybe not very representative. I'll redo it sometime with a large sample size.
Here's stellar magnitudes:

Surface temperatures

Terrestrial surface temperatures

The ages of the few stars I discovered

And here's stellar masses

Star sizes

Planet sizes

Terrestrial planet sizes

Large body masses

Terrestrial body masses

Surface Gravity

Terrestrial surface gravity

Planets per system type

Planets per star or barycenter type within the systems

Oh, I quite like this visualization I did of the travel route I took

I could go on, but you get the idea. I'll probably redo the relative density plots at some point with galaxy wide data, and make a few more 3d rotating galaxy visualizations of stuff.
Before you give out to me about the length of this post, my excuse is CMDR Marx made me do it!