Journey to the known unbeknownst records of the galaxy

The Dumbae SY-I d9-2339 system is a bit special … and it was not far away from my actual next destination. Hence, I visited it even though it doesn't fall under the above stated "rules" … I know, I know …

Anyway, of all known systems houses this system the largest number of F-type stars. Five of them formed here and on this picture you can see all of them:
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The fifth member of the "family" was a bit shy and is hiding more than 30 kls away. But it is in the photo.

Since five is such a low number I've checked once more and indeed it is indeed a unique record. All other systems contain four or less F type stars.
 
This M (Red giant) Star, …
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… with the designation Hypoe Flya IC-V e2-272 B, has the largest semi major axis (107,538,346,955,365.39 m or ca. 718.85 au) and also the largest orbital circumference (670,406,233,174,275.2 m) of them all. In this case this leads also to a long distance to arrival and finally: let the hoovering begin … well … while writing this, it was already finished.
 
Dryao Ausms DA-A f2925 B is a Neutron Star and it has, with a value of 862,479,686,218,385.4 m, the largest orbital circumference of all of them. And that's it. One would expect also the record for the largest semi major axis … but nope, not this time. In an earlier post I've explained why how this can be the case and this find confirms that it is correct, that I separate those even though such records most often belong to one and the same body.

To celebrate this, I did something daring:
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Operation WHITE DWARF is progressing in huge jumps (pun intended).

Name: Stranoa VZ-G d10-235 A
Subcategory: DB
Record: absolute magnitude (brightest)
Value: 7.469925
Picture: row 1, column

Name: Eor Aug IY-Q d5-159 A
Subcategory: DB
Record: orbital period (longest)
Value: 1,409,943,994,368.0 s or almost 44.71 Millenia
Picture: row 1, column 2

Name: Wepiae AA-A h170 A 2
Subcategory: DB
Record: rotational period (longest)
Value: 31.096166087962963 days
Picture: row 1, column 3

Name: Dryaa Pruae AA-A h613 2
Subcategory: DCV
Record: axial tilt (largest)
Value: 84.95955696070119 degrees
Picture: row 2, column 1

Name: Dryoi Proo JM-W f1-85 B
Subcategory: DAV
Record: velocity in periapsis (fastest)
Value: 501,341.8379449012 m/s or ca. 1.80 Gm/s
Picture: row 2, column 2

Name: Mylaifa AA-A h669 1
Subcategory: DBV
Record: axial tilt (highest)
Value: 65.90590277940643 degrees
Picture: row 2, column 3

Name: Dryaa Pruae AA-A h862 AB 2
Subcategory: DB
Record: axial tilt (largest)
Value: 85.17674541300428 degrees
Picture: row 3, column 1

Name: Screakao AB-W e2-445 B
Subcategory:
Record: DBC
Value: velocity in periapsis (fastest)
Picture: row 3, column 2
Notes:419,231.789939375 m/s or ca. 1.51 Gm/s

Name: Dryau Ausms NX-U e2-907 B
Subcategory: DAV
Record: distance to arrival (longest)
Value: 643,301 ls
Picture: row 3, column 3

143017
 
Also far away from the point of entry into its system is Eord Blue AA-A h115 C:
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And it is also a Wolf-Rayet star but this time of the sobcategory < O >.

It's so far away because it holds the record for the largest semi major axis (102,303,125,778,962.08 or ca. 683.85 au) and with it also for the largest orbital circumference (642,767,120,686,377.1 m) … and it is not what the FSD latches onto when jumping into this system.
 
More white dwarf data

Name: Eos Ausms PS-U f2-2875 B
Subcategory: DAB
Record: velocity in periapsis (fastest)
Value: 774,697.4658412489 m/s or almost 2.79 Gm/s
Picture: row 1, column

Name: Aunair KD-K d8-2168 A
Subcategory: DA
Record: orbital period (longest)
Value: 1,504,022,364,160.0 s or ca. 47.69 Millenia
Picture: row 1, column 2

Name: Egnaiwn BA-A f3729 B
Subcategory: DAV
Record: distance to arrival (shortest)
Value: 3 ls
Picture: row 1, column 3
Notes: The one in the background.

Name: Zunuae DM-C d2296 A
Subcategory: DAV
Record: age (youngest)
Value: 4,698 Million years
Picture: row 2, column 1

Name: Oudaitt TK-C d14-1697
Subcategory: DAB
Record: age (youngest)
Value: 4,684 Million years
Picture: row 2, column 2

Name: Huemeae MO-Q d5-207
Subcategory: DB
Record: age (youngest)
Value: 4,730 Million years
Picture: row 2, column 3
Notes: Yes, that are three youngest white dwarfs in a row. Pun intended but it actually is a weird coincidence :).

Name: Oufaish KQ-X d1-62 A
Subcategory: DBV
Record: orbital period
Value: 1,202,729,254,912.0 s or almost 38.14 Millenia
Picture: row 3, column 1

Name: Dryi Phylaa FF-A e520 C
Subcategory: DBV
Record 1: orbital circumference (largest)
Value 1:576,077,644,504,655.8 m
Record 2: semi major axis (longest)
Value 2:91,713,498,084,261.19 m or ca. 613.07 au
Picture: row 3, column 2

Name: Phoi Aurb FB-O e6-1024 C
Subcategory: DCV
Record: absolute magnitude (brightest)
Value: 10.12793
Picture: row 3, column 3

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For today I finish writing with Lyaisoo MQ-B d14-756 B 1 … Yay! I have yellow tracks :)
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You may remember that Sigma Orionis E 1 was the Metal-rich body furthest away from the point of entry into the system. You may also remember, that one can't land on it.
Well, as you can see did I land on the planet shown on the picture because it is the landable (!) Metal-rich body furthest away from the point of arrival. However, the distance is almost ten times smaller with just 799,890 ls.

I wonder about one thing though. Why am I listed as the one who scanned it first for EDSM. If that really would be the case I wouldn't be here. Fascinating.
 
Lasoae II-H d11-1027 E 1 is the Ammonia world, furthest away from when you enter the system. So I jumped into the latter … and started to prepare dinner. Dinner was ready and I was just 35 kls away. Hence, dinner was delayed a couple of minutes so that I could make this photo:
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I pointed downwards to check how close I can get wile eating said dinner. In hindsight that seemed to be a not so good idea but I just hit the body exclusion zone. Could that have been dangerous?

Ah yes, the dinner. I had trout and potatoes and peas and broccoli.
 
Hypuae Briae YO-A d4892 B 1 was far enough away from the point of entry into the system so that I had an incentive to fly there. But it is also the the Class I gas giant with the largest orbital eccentricity with a value of 0.999806. That gives such an elongated orbit that the computer can't display it in a meaningful manner any longer. Hence, I just show the planet itself:
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As the experienced traveler among the stars can deduce from the lack of light: the planet was at the far-away-from-the-star-end of it's orbit.
 
Dryoi Grie AA-A h7 C is just the second O (Blue-White) Star I've deliberately visited on this journey. Another dinner needed to be prepared so it was handy that with the record of the largest semi major axis (124,276,153,196,665.66 m or ca. 830.73 au) and the largest orbital circumference (774,351,931,463,657.6 m) followed a long distance (albeit not a record) from the point of arrival.

And here it is:
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I collected some material. First an update on Operation WHITE DWARF.

Name: Ooh Chruia DA-A f18 B
Subcategory: DB
Record: velocity in periapsis (fastest)
Value: 682,304.8053362529 m/s or almost 2.46 Gm/s
Picture: row 1, column

Name: Baukoa UG-J d10-1573 A
Subcategory: DBV
Record: absolute magnitude (dimmest)
Value: 11.718689
Picture: row 1, column 2

Name: Rhuedgie MI-T e3-1346 C
Subcategory: DB
Record 1: circumference (largest)
Value 1: 820,929,669,485,210.8 m
Record 2: semi major axis (longest)
Value 2: 30,746,135,521,841.23 m or ca. 873.98 au
Picture: row 1, column 3

Name: Smasiae RZ-O e6-427 D
Subcategory: DC
Record: distance to arrival (furthest)
Value: 706,388 ls
Picture: row 2, column 1

Name: Aowroae AR-U d3-188 A
Subcategory: DAB
Record: rotational period (longest)
Value: 5.847898582175926 days
Picture: row 2, column 2

Name: Teqie AA-A h24 2
Subcategory: DAV
Record: axialt tilt (largest)
Value: 51.58583416631271 degrees
Picture: row 2, column 3

Name: Phleedgae AA-A h128 3
Subcategory: DA
Record: axial tilt (largest)
Value: 88.82155913094927 degrees
Picture: row 3, column 1

Name: Dryao Phylio QH-V d2-95 A
Subcategory: DB
Record: orbital eccentricity (largest)
Value: 0.821182
Picture: row 3, column 2

Name: Kylou Pri LN-S e4-42 B
Subcategory: DAB
Record: distance to arrival (longest)
Value: 587,453 ls
Picture: row 3, column 3

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Something different than a white dwarf, namely a Wolf-Rayet NC Star, is Drumbaae AA-A h8 D:
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I visited it because it was far away from the point of entry into the system since it holds the record for the largest semi major axis (108,172,651,546,317.34 or ca. 723.09 au) and also for the largest orbital circumference (678,247,849,816,363.6 m) for all stars in this class.
 
Finally, I've visited the last of the white dwarfs considered in Operation WHITE DWARF. Here is the last update.

Name: Bloomoa NX-T e3-1044 E
Subcategory: DB
Record: distance to arrival (longest)
Value: 548,468 ls
Picture: row 1, column

Name: Hypiae Aub OT-Q e5-111 B
Subcategory: DAV
Record: age (oldest)
Value: 13.064 billion years
Picture: row 1, column 2

Name: Pyroomee YK-P e5-825 B
Subcategory: DCV
Record 1: orbital circumference (largest)
Value 1: 776,774,229,570,753.8 m
Record 2: semi major axis (longest)
Value 2: 123,760,102,812,130.38 or ca. 827.29 au
Picture: row 1, column 3
Notes:

Name: Hypiae Ausms MT-F d12-16 A
Subcategory: DCV
Record: age (youngest)
Value: 7.564 billion years
Picture: row 2, column 1
Notes: This is really old for being the youngest.

Name: Eol Prou PS-U f2-3613 B
Subcategory: DA
Record 1: orbital circumference (largest)
Value 1: 845,903,906,558,385.4 m
Record 2: semiMajorAxis (longest)
Value 2: 137,354,563,432,809.02 m or ca. 918.16 au
Picture: row 2, column 2

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This concludes Operation WHITE DWARF. It was announced almost three months ago because I wanted to get these dangerous beasts out of the way. In the first map many of them are highlighted. In the last map (shown in the last tile of the picture above) few of them are left (the light aqua dots). These remaining white dwarfs are too far away to justify a "short visit" while other things are waiting.

The Colonia region was the first theater of operations. Afterwards the road to the bubble and than the bubble itself became the regions this operation took place in. Second to last the white dwarf clusters below Sgr A* and lastly the white dwarfs above Sgr A* and on the way back to Colonia were visited.
All in all, it was a nice motivation to get out there … into the void.

An interesting coincidence is, that this operation started and ended in the Eol Prou sector. I didn't do this deliberately, but when this begun the final system (Eol Prou PS-U f2-3613 B), was still unexplored. It just appeared with the latest update of the data on the map.

This shows also that in the future more white dwarfs can appear. A possible white dwarf record which wasn't visited because it wasn't unique may suddenly be broken by a unique entry. And in this case it will appear on the map.

Anyway, the next body I'll visit on this journey is something very special.
 
Since this journey started I was very much looking forward visiting the landable body with the highest gravity. But the record holder until recently was in a region too far away for a short stop. But that changed when this record was broken.

So, here I am on Kyloall CL-Y g1518 D 1
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… that is not just the only planet in its system, but also holds the above mentioned record for all (landable) celestial bodies and for all Metal-rich bodies with a value of 11.009168647951414 g.
It is also the landable Metal-rich body with the largest mass (94.588409 Earth masses) and the largest radius (18,695.032 km).

Now for some additional thoughts.
On EDSM the colid composition is given as: 53.94% Rock, 42.61% Metal, 0.14% Ice.
This is confusing because neither does it say if it is mass or volume composition nor if this is just the surface composition (something I would guess is the only things our probes can measure).

Now the "ice" may point into the direction that this is mass. Why is that?
Well, the surface temperature is far too high to allow any liquid water (and there is also no atmosphere). We know, that a lot of water is trapped in Earth's mantle.

Thus I take it that the word "ice" was chosen to go together with "solid composition". It is also just a different word for "solid water"

In absence of any other information am I assuming that I'm part of a totally average part of the cosmos (that must not be true), thus I assume that this is a rock-ish planet like Earth and that these develop all approximately the same.
The earth is made up of approx. 35 % Iron, 30 % Oxygen, 15 Silicon and 13 percent Magnesium. The only two of these that are metals are Iron and Magnesium. Thus Iron makes up ca. 73 % of the metal content of Earth.
Since this is just an estimation I go with these numbers and thus say that this planet's Iron content is ca. 29 Earth masses.

The vast majority of the Earth's iron is found in the core. NB: when I write "core" I mean the inner and the outer core and don't distinguish between these two (which seems to be OK since this is just an estimation).
According to the Preliminary reference Earth model (looking at fig. 8 on page 310 keeps you from reading the whole article ;) ) is the density of the core relativ constant and approx. 11 tons per cubic meter. Again: there are changes but within this estimation that doesn't really matter.

Earth itself has a mass of ca. 5.97 times 10 to the 24 kg. Assuming the core is pure iron and the complete 35 % are in the core (which is not too far from what is assumed) gives a mass of the core of ca. 2 times ten to the 24 kg.
This gives a volume of Earth's core of ca. 1.8 times ten to the 20 cubic meter. Assuming it is a sphere follows from this a radius of ca. 3,500 km. Despite all the assumptions and estimations is this pretty close to the value we assume is correct. Thus we can continue with the planet I'm standing on.

29 Earth masses Iron content are approx. 1.7 times ten to the 26 kg. Assuming the same average density of 11,000 kg per cubic meter (which might not be too far from the truth, since the density of earth's inner core is even less dependent on the depth than the outer core, so more pressure seems not to compress the solid core a lot more) am I arriving at a radius of the core of approx. 15,500 km.

Mhmmm … The radius of earth's core is approx. half of its total radius. Here though the core radius is almost 83 percent of the total radius! That makes the following very very interesting.

With a core radius of 15,500 km and a total radius of ca. 18700 km it means that ca. 1.2 times ten to the 22 cubic meters of material are in the mantle of this planet. The core accounts for ca. 29 Earth masses of the total 94.588409 Earth masses of this planet. Thus we we need to cramp the remaining 65.6 Earth masses into these 1.2 times ten to the 22 cubic meters. Thus follows, that the average density of the mantle-material of this planet is 33,200 kg per cubic meter … … … ! … … … !!! … … … !!!oneoneeleven … o_O

Well, this seems to be an inverted planet with a denser mantle than the core. I would be interested in the physics that can explain how such a planet can form.
It can't be that my assumptions are super wrong. Because I need to increase the density of the core by an order of magnitude to half the radius of the core which would lead to a halved density of the mantle material … this is still three times larger than Earth's mantle material density. BUT a ten times higher density … of Iron! … these physics would be equally interesting compared with an inverted planet.

Is "Metal" than not Iron? Looking at densities of metals under normal conditions doesn't leave me a lot of room to wiggle here. A can maybe get a factor of approx 2.5 but not ten.

Something very different that is stable and behaves like metal? Well, we are back to very interesting physics.

Also: if I increase the core density towards infinity will the mantle density converge towards a value around 14,000 kg per cubic meter. So even with an infinitely dense core something must be very different.

Or Rock is not Rock (a.k.a. mostly silicon dioxide) but behaves like it … interesting physics at all corners … Thinking about it, is this planet truly fascinating :)

I'm open for suggestions to solve this riddle. And even though I've gone through the calculations several times may I have forgotten to divide by a thousand somewhere. So anybody please be my guest and check these numbers.
 
I'm back at Colonia and thinking about what to do next.
Well, I'd like to get Chicken of Doom here and mine. Less to get money but more to get engineering materials. Afterwards I intended to get down to the bubble and do mining for the stations on the way.

BUT … it is so expensive to get the ship here in the first place. That will be approx. 1/10th of my assets. I may get this with double painite mining, but how do I find these spots?
I also don't know if I'll get all the mining equipment here in Colonia. I guess so since I intend to do old style mining but I'm unfamiliar with this region of space

Anyway, I'll do this because I'm in the mood for it and except mining for Explorer's Anchorage I never really did that.

And when I get bored of that I have a new (sub)goal on my Journey to the known unbeknownst records of the galaxy. I'm going to visit all yewllow-ish (orange, yellow, white, but not blue-white) stars … that are record holders. This includes the following:
  • F (White) Star + F (White super giant) Star
  • G (White-Yellow) Star + G (White-Yellow super giant) Star
  • K (Yellow-Orange) Star + K (Yellow-Orange giant) Star
  • M (Red dwarf) Star + M (Red giant) Star + M (Red super giant) Star
  • Herbig Ae/Be Star
  • C Star
  • CN Star
  • CJ Star
  • MS-type Star
  • S-type Star
It does not include T Tauri stars since these are often not yellow.

I will call this OPERATION YELLOW ORB.

I thought it a good idea to stick with the reporting format I had introduced for the white dwarfs.
This is because I'm running out of ideas how to take interesting pictures and describe all these stars that are always kind of the same. This format will also save you from reading (and me from writing) too much boring stuff … pffffff … I knew before that this also will be a journey of endurance … and well, the fun one has instead of reading philosophy ;)

Here is a map with where I need to go:
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Yellow are systems that i need to visit for operation YELLOW ORB. It seems that a large amount of my "targets" is in or around the bubble. Well, I'm fine with that.
 
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