The Galactic Mapping Project & Historical Archive of Exploration
Oh aye, Priapus was all about 'vegetables'
https://s14-eu5.ixquick.com/cgi-bin...3/128.jpg&sp=1255ad58ca5be8f6649e2ce0005c3bbd
Oh damn, I didn't check if it has some sexual meaning :/ I can change it if it's an issue !
Croidaea OO-X D2-1 - "Perseus Deep"
"Perseus Deep"
Croidaea OO-X D2-1
Named for the Perseus Fade and the fact that it is at 431.1875 / -1346.125 / -7180.75, Perseus Deep is a difficult but worthwhile visit. Out near the Rim and in an area of stellar scarcity, the low level of illumination from other stars allows a remarkable view of both Megallanic clouds and Andromeda.
The system has all Jumponium components except for Niobium, including a Yttrium +4 and a Polonium +3. Niobium can be found in systems on the way "down".
The system also contains two terraformable planets and an Earth Like World.
FGES Sleipnir, commanded by Chrystoph, discovered the system in 3303. Station X in Crab Sector DL-Y d9 functions as a starting point to this unique find (Jumponium required).
Arsenic - 6A
Cadmium - 2A
Germanium - 2A, 6A
Niobium -
Polonium - 2A
Vanadium - 2A, 5A, 6A
Yttrium - 6A
2A - Polonium +3 (C, G, V)
5 - Terraforming Candidate
6 - Terraforming Candidate
6A - Yttrium +4 (A, C, G, V)
7 - Earth Like World
https://www.edsm.net/en/system/id/13909887/name/Croidaea+OO-X+d2-1
| Source: Crab Sector DL-Y d9 - Station X CommID: Commander Chrystopher Chance Callsign: Chrystoph Priority: Routine Recipients: General Distribution Timestamp: 3303/07/14 | 
|
"Perseus Deep"
Croidaea OO-X D2-1
Named for the Perseus Fade and the fact that it is at 431.1875 / -1346.125 / -7180.75, Perseus Deep is a difficult but worthwhile visit. Out near the Rim and in an area of stellar scarcity, the low level of illumination from other stars allows a remarkable view of both Megallanic clouds and Andromeda.
The system has all Jumponium components except for Niobium, including a Yttrium +4 and a Polonium +3. Niobium can be found in systems on the way "down".
The system also contains two terraformable planets and an Earth Like World.
FGES Sleipnir, commanded by Chrystoph, discovered the system in 3303. Station X in Crab Sector DL-Y d9 functions as a starting point to this unique find (Jumponium required).
Arsenic - 6A
Cadmium - 2A
Germanium - 2A, 6A
Niobium -
Polonium - 2A
Vanadium - 2A, 5A, 6A
Yttrium - 6A
2A - Polonium +3 (C, G, V)
5 - Terraforming Candidate
6 - Terraforming Candidate
6A - Yttrium +4 (A, C, G, V)
7 - Earth Like World
https://www.edsm.net/en/system/id/13909887/name/Croidaea+OO-X+d2-1
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Wouldn't bother me, but I'm not the final arbiter on adding POIs
We won't have any problem with that reference.
Update:
POI Name: Seagull Nebula
Desc update: "The Seagull Nebula (IC 2177), is a region of nebulosity that lies along the border between the constellations Monoceros and Canis Major. It is a roughly circular H II region centered on the star BD-10 1848 (HD 53367). This nebula was discovered by Welsh amateur astronomer Isaac Roberts and was described by him as 'pretty bright, extremely large, irregularly round, very diffuse.' "
Add image:
POI Name: Seagull Nebula
Desc update: "The Seagull Nebula (IC 2177), is a region of nebulosity that lies along the border between the constellations Monoceros and Canis Major. It is a roughly circular H II region centered on the star BD-10 1848 (HD 53367). This nebula was discovered by Welsh amateur astronomer Isaac Roberts and was described by him as 'pretty bright, extremely large, irregularly round, very diffuse.' "
Add image:
New POI
POI Name: HD 53041
Galmap ref: HD 53041
POI Type: Stellar Feature
Description: "At just over 1300 Ly from Sol in the Col 140 Sector, this system is a great destination for new explorers. Two black holes and four bright stars are located here. The primary black hole provides excellent optical effects for Barnard's Loop; and the three A-type stars are in very close orbits, forming a brilliant blue-white dot which resolves into a vivid triangle."
POI Name: HD 53041
Galmap ref: HD 53041
POI Type: Stellar Feature
Description: "At just over 1300 Ly from Sol in the Col 140 Sector, this system is a great destination for new explorers. Two black holes and four bright stars are located here. The primary black hole provides excellent optical effects for Barnard's Loop; and the three A-type stars are in very close orbits, forming a brilliant blue-white dot which resolves into a vivid triangle."
New POI
POI Name: Vela Pulsar
POI Type: Pulsar
Galmap Ref: Vela Pulsar
Desc: "The Vela Pulsar is a radio, optical, X-ray- and gamma-emitting pulsar associated with the Vela Supernova Remnant in the constellation of Vela. The spin of 11.195 times per second (i.e. a period of 89.33 milliseconds) was the shortest known at the time of discovery.
The pulsar was discovered by astronomers at the University of Sydney in 1968, and was the direct evidence that supernovae form neutron stars. It was also studied in 2015 by a NASA balloon launched from Alice Springs, Australia. Perhaps most unusually, the emissions of Vela and the pulsar PSR B0329+54 were converted into audible sound by French composer Gérard Grisey and used in the piece 'Le noir de l'étoile'.
The Vela Pulsar is in binary pair with a B-class star and also is found with a number of class V gas giants."
POI Name: Vela Pulsar
POI Type: Pulsar
Galmap Ref: Vela Pulsar
Desc: "The Vela Pulsar is a radio, optical, X-ray- and gamma-emitting pulsar associated with the Vela Supernova Remnant in the constellation of Vela. The spin of 11.195 times per second (i.e. a period of 89.33 milliseconds) was the shortest known at the time of discovery.
The pulsar was discovered by astronomers at the University of Sydney in 1968, and was the direct evidence that supernovae form neutron stars. It was also studied in 2015 by a NASA balloon launched from Alice Springs, Australia. Perhaps most unusually, the emissions of Vela and the pulsar PSR B0329+54 were converted into audible sound by French composer Gérard Grisey and used in the piece 'Le noir de l'étoile'.
The Vela Pulsar is in binary pair with a B-class star and also is found with a number of class V gas giants."
A new submit, a Planetary Nebula in a empty zone of GMP (near Zephyrus region).
- POI Name : Trignai blend
- POI Type : β - Planetary Nebula
- GalMap Ref : Trignai MT-Q e5-28 EDSM link
- Description : Beautiful Blue-pink planetary nebula, with a neutron star and G-star core.
- Screenshot reference :
- POI Name : Trignai blend
- POI Type : β - Planetary Nebula
- GalMap Ref : Trignai MT-Q e5-28 EDSM link
- Description : Beautiful Blue-pink planetary nebula, with a neutron star and G-star core.
- Screenshot reference :
New POI
POI Name: Phi Velorum
Galmap Ref: Phi Velorum
POI Type: Planetary Feature
Desc: "At just 1500 light years from Sol on the north edge of the Vela Molecular Ridge, this system is a good stop for the explorer headed out into the north-eastern sections of the galaxy. Phi Velorum is a blue-white supergiant, but the attraction here is the L-class dwarf with enormous rings. The rocky outer rings are a total of 68.5 light-seconds from end to end, and 41.2 light-seconds wide. This system is also a 'green' system containing landable planets with all materials necessary for frame-shift drive injections, including premium."
POI Name: Phi Velorum
Galmap Ref: Phi Velorum
POI Type: Planetary Feature
Desc: "At just 1500 light years from Sol on the north edge of the Vela Molecular Ridge, this system is a good stop for the explorer headed out into the north-eastern sections of the galaxy. Phi Velorum is a blue-white supergiant, but the attraction here is the L-class dwarf with enormous rings. The rocky outer rings are a total of 68.5 light-seconds from end to end, and 41.2 light-seconds wide. This system is also a 'green' system containing landable planets with all materials necessary for frame-shift drive injections, including premium."
New POI
POI Name: Radioactive Green
POI Type: Planetary Feature
Galmap Ref: Col 285 Sector VU-M C8-1
Desc: "The fourth and last gas giant of this system has an unusual feature - it glows a vivid green. The cause of the glow is unknown, but scientists believe the ammonia-based life in this star may be exhibiting a form of bioluminescence. Regardless of the source the planet is a popular tourist attraction and easy to reach at only 300 light-years from Sol. A tourist beacon is set up here in close orbit of the gas giant."
POI Name: Radioactive Green
POI Type: Planetary Feature
Galmap Ref: Col 285 Sector VU-M C8-1
Desc: "The fourth and last gas giant of this system has an unusual feature - it glows a vivid green. The cause of the glow is unknown, but scientists believe the ammonia-based life in this star may be exhibiting a form of bioluminescence. Regardless of the source the planet is a popular tourist attraction and easy to reach at only 300 light-years from Sol. A tourist beacon is set up here in close orbit of the gas giant."
Re submit of this planetary Nebula
Name: "Pilou"
Type: β - Planetary Nebula
Map Reference: Dryi Free ZK-P e5-4565 EDSM Link
First-Discoverer: "Phoenix452_74" 3303-07-23
Description: This planetary Nebula system have a neutron star, and 2 stars ( L star in orbit around a K star). 2 landables planet with a beautiful point of view of the 2 stars.
Screenshot Reference: http://imgur.com/a/762Y2
New Sumbit of this another planetary Nebula
Name: "Héphaïstos's rest"
Type: β - Planetary Nebula
Map Reference: Kyloalks EH-U e3-210 EDSM Link
First-Discoverer: "Phoenix452_74" 3303-07-24
Description: This planetary Nebula system have a black hole and an A stars. There is a lot of landable planet with volcanism activity of difference sort (magma, geysers).
Screenshot Reference: http://imgur.com/a/a6xQB
Name: "Pilou"
Type: β - Planetary Nebula
Map Reference: Dryi Free ZK-P e5-4565 EDSM Link
First-Discoverer: "Phoenix452_74" 3303-07-23
Description: This planetary Nebula system have a neutron star, and 2 stars ( L star in orbit around a K star). 2 landables planet with a beautiful point of view of the 2 stars.
Screenshot Reference: http://imgur.com/a/762Y2
New Sumbit of this another planetary Nebula
Name: "Héphaïstos's rest"
Type: β - Planetary Nebula
Map Reference: Kyloalks EH-U e3-210 EDSM Link
First-Discoverer: "Phoenix452_74" 3303-07-24
Description: This planetary Nebula system have a black hole and an A stars. There is a lot of landable planet with volcanism activity of difference sort (magma, geysers).
Screenshot Reference: http://imgur.com/a/a6xQB
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Is this feature visible, it glows a vivid green, on the system map ? Even with so little presence of a vivid green ?
Just remembered I scanned a system with a lot of moons near Jacques a while back and checked if it was green. It is! Thinking about it, it might be gold since there are so many landable bodies. Not on EDSM sadly since I wasn't using it back then... Oh well here it is anyway, 59 landable bodies:
☢☢ EOL PROU TB-O B35-50 ☢☢
Name: Sapporo's Gold Break
Holy crap this took a while to type. Since it's not on EDSM, need screenshots? If so, please tell me not all the planets please ;-;
-Sappy
Edit: I'm 99% sure this is a gold system. It contains all of the materials found on inara.cz under "surface prospecting".
☢☢ EOL PROU TB-O B35-50 ☢☢
Name: Sapporo's Gold Break
AB 1 A
Vanadium 2.7%
Cadmium 0.9%
AB 1 C
Arsenic 1.4%
AB 1 D
Arsenic 1.4%
AB 2 A
Arsenic 1.6%
Niobium 0.8%
Yttrium 0.7%
AB 2 B
Arsenic 1.6%
AB 2 C
Niobium 0.8%
AB 2 D
Germanium 3.5%
Polonium 0.3%
AB 3 A
Cadmium 0.9%
Niobium 0.8%
AB 3 B
Vanadium 3.0%
Niobium 0.8%
AB 4 A
Germanium 3.5%
Cadmium 0.9%
AB 6 G
Vanadium 3.0%
AB 6 H
Germanium 3.5%
Niobium 0.8%
Yttrium 0.7%
AB 6 I
Germanium 3.1%
AB 7 A
Germanium 3.5%
Vanadium 3.0%
Cadmium 1.0%
AB 7 B
Germanium 3.4%
AB 7 C
Arsenic 1.6%
Cadmium 1.0%
AB 7 D
Cadmium 1.0%
Niobium 0.8%
AB 7 E
Cadmium 1.0%
Yttrium 0.7%
AB 7 F
Vanadium 3.0%
Cadmium 0.9%
AB 8 A
Vanadium 3.0%
Cadmium 1.0%
AB 8 B
Cadmium 1.0%
AB 8 C
Vanadium 3.0%
Cadmium 1.0%
Niobium 0.8%
Yttrium 0.7%
AB 8 D
Vanadium 3.1%
AB 9 A
Vanadium 3.0%
Cadmium 0.9%
Polonium 0.3%
AB 9 B
Germanium 3.6%
Vanadium 3.1%
Polonium 0.3%
AB 9 C
Vanadium 3.0%
Cadmium 1.0%
Niobium 0.8%
AB 9 D
Niobium 0.8%
AB 9 E
Cadmium 0.9%
Yttrium 0.7%
AB 9 F
Vanadium 3.0%
Cadmium 0.9%
Niobium 0.8%
______________________________________________________________________
B 1
Arsenic 2.1%
Cadmium 1.8%
B 2
Yttrium 1.3%
B 3
Arsenic 2.0%
______________________________________________________________________
C 2
Germanium 3.3%
Cadmium 1.2%
C 3
Vanadium 4.0%
Germanium 3.3%
Cadmium 1.3%
C 6 A
Vanadium 3.0%
C 6 B
Vanadium 3.1%
Arsenic 1.6%
Cadmium 1.0%
C 7 A
Germanium 3.6%
Arsenic 1.6%
Niobium 0.9%
C 7 B
Germanium 3.5%
Cadmium 0.9%
Yttrium 0.7%
C 7 C
Arsenic 1.6%
Cadmium 1.0%
C 7 D
Germanium 3.5%
Vanadium 3.0%
Cadmium 0.9%
Niobium 0.8%
C 7 E
Vanadium 3.0%
Cadmium 1.0%
C 7 F
Germanium 3.5%
Cadmium 0.9%
C 7 G
Vanadium 3.0%
Cadmium 0.9%
Niobium 0.8%
C 8 A
Vanadium 3.0%
Cadmium 0.9%
C 8 B
Cadmium 1.0%
C 8 C
Cadmium 0.9%
Yttrium 0.7%
C 8 D
Germanium 3.4%
C 8 E
Germanium 3.5%
Polonium 0.3%
C 8 F
Vanadium 3.0%
Cadmium 1.0%
C 8 G
Germanium 3.5%
Cadmium 1.0%
C 8 H
Germanium 3.5%
Cadmium 0.9%
C 9 A
Germanium 3.6%
Cadmium 1.0%
Polonium 0.3%
C 9 B
Germanium 3.6%
Arsenic 1.6%
Cadmium 1.0%
Niobium 0.9%
C 9 D
Niobium 0.9%
C 9 E
Vanadium 3.0%
Cadmium 1.0%
Yttrium 0.7%
Vanadium 2.7%
Cadmium 0.9%
AB 1 C
Arsenic 1.4%
AB 1 D
Arsenic 1.4%
AB 2 A
Arsenic 1.6%
Niobium 0.8%
Yttrium 0.7%
AB 2 B
Arsenic 1.6%
AB 2 C
Niobium 0.8%
AB 2 D
Germanium 3.5%
Polonium 0.3%
AB 3 A
Cadmium 0.9%
Niobium 0.8%
AB 3 B
Vanadium 3.0%
Niobium 0.8%
AB 4 A
Germanium 3.5%
Cadmium 0.9%
AB 6 G
Vanadium 3.0%
AB 6 H
Germanium 3.5%
Niobium 0.8%
Yttrium 0.7%
AB 6 I
Germanium 3.1%
AB 7 A
Germanium 3.5%
Vanadium 3.0%
Cadmium 1.0%
AB 7 B
Germanium 3.4%
AB 7 C
Arsenic 1.6%
Cadmium 1.0%
AB 7 D
Cadmium 1.0%
Niobium 0.8%
AB 7 E
Cadmium 1.0%
Yttrium 0.7%
AB 7 F
Vanadium 3.0%
Cadmium 0.9%
AB 8 A
Vanadium 3.0%
Cadmium 1.0%
AB 8 B
Cadmium 1.0%
AB 8 C
Vanadium 3.0%
Cadmium 1.0%
Niobium 0.8%
Yttrium 0.7%
AB 8 D
Vanadium 3.1%
AB 9 A
Vanadium 3.0%
Cadmium 0.9%
Polonium 0.3%
AB 9 B
Germanium 3.6%
Vanadium 3.1%
Polonium 0.3%
AB 9 C
Vanadium 3.0%
Cadmium 1.0%
Niobium 0.8%
AB 9 D
Niobium 0.8%
AB 9 E
Cadmium 0.9%
Yttrium 0.7%
AB 9 F
Vanadium 3.0%
Cadmium 0.9%
Niobium 0.8%
______________________________________________________________________
B 1
Arsenic 2.1%
Cadmium 1.8%
B 2
Yttrium 1.3%
B 3
Arsenic 2.0%
______________________________________________________________________
C 2
Germanium 3.3%
Cadmium 1.2%
C 3
Vanadium 4.0%
Germanium 3.3%
Cadmium 1.3%
C 6 A
Vanadium 3.0%
C 6 B
Vanadium 3.1%
Arsenic 1.6%
Cadmium 1.0%
C 7 A
Germanium 3.6%
Arsenic 1.6%
Niobium 0.9%
C 7 B
Germanium 3.5%
Cadmium 0.9%
Yttrium 0.7%
C 7 C
Arsenic 1.6%
Cadmium 1.0%
C 7 D
Germanium 3.5%
Vanadium 3.0%
Cadmium 0.9%
Niobium 0.8%
C 7 E
Vanadium 3.0%
Cadmium 1.0%
C 7 F
Germanium 3.5%
Cadmium 0.9%
C 7 G
Vanadium 3.0%
Cadmium 0.9%
Niobium 0.8%
C 8 A
Vanadium 3.0%
Cadmium 0.9%
C 8 B
Cadmium 1.0%
C 8 C
Cadmium 0.9%
Yttrium 0.7%
C 8 D
Germanium 3.4%
C 8 E
Germanium 3.5%
Polonium 0.3%
C 8 F
Vanadium 3.0%
Cadmium 1.0%
C 8 G
Germanium 3.5%
Cadmium 1.0%
C 8 H
Germanium 3.5%
Cadmium 0.9%
C 9 A
Germanium 3.6%
Cadmium 1.0%
Polonium 0.3%
C 9 B
Germanium 3.6%
Arsenic 1.6%
Cadmium 1.0%
Niobium 0.9%
C 9 D
Niobium 0.9%
C 9 E
Vanadium 3.0%
Cadmium 1.0%
Yttrium 0.7%
Holy crap this took a while to type. Since it's not on EDSM, need screenshots? If so, please tell me not all the planets please ;-;
-Sappy
Edit: I'm 99% sure this is a gold system. It contains all of the materials found on inara.cz under "surface prospecting".
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Hmmmm... An ammonia gas giant exhibiting vivid green colours within its atmosphere? Now where have I seen these themes juxtaposed together before...?
New POI
POI Name: Beehive Cluster
POI Type: Star Cluster
Galmap ref: Praesepe
Desc: "The Beehive Cluster (also known as NGC 2632, M44, or Cr 189) is an open cluster in the constellation Cancer. It is one of the nearest open clusters to Sol, and it contains a larger star population than most other nearby clusters. The Beehive Cluster is one of the best studied open clusters, having been observed as far back as ancient times. It was one of the first objects studied by Galileo.
The cluster is composed of objects from almost every major star catalogue including HIP, HD, BD, HR, 2MASS, UGCS, PR, WBG, and BBG. There are few or no stars that are not "named". The cluster is approximately 500 light-years long and averages 10 light years wide. While composed of mostly red dwarf stars, it has stars of all major types (excepting O-type), and at least 10 stars of giant size. The cluster is roughly bounded by HIP 40361 at the lower end and DR Cancri at the upper end. The reference star Praesepe is one of the brighter stars, and also an older name for the entire cluster.
Carbon star X Cancri can be found approx 140 Ly above this cluster."
(no image)
POI Name: Beehive Cluster
POI Type: Star Cluster
Galmap ref: Praesepe
Desc: "The Beehive Cluster (also known as NGC 2632, M44, or Cr 189) is an open cluster in the constellation Cancer. It is one of the nearest open clusters to Sol, and it contains a larger star population than most other nearby clusters. The Beehive Cluster is one of the best studied open clusters, having been observed as far back as ancient times. It was one of the first objects studied by Galileo.
The cluster is composed of objects from almost every major star catalogue including HIP, HD, BD, HR, 2MASS, UGCS, PR, WBG, and BBG. There are few or no stars that are not "named". The cluster is approximately 500 light-years long and averages 10 light years wide. While composed of mostly red dwarf stars, it has stars of all major types (excepting O-type), and at least 10 stars of giant size. The cluster is roughly bounded by HIP 40361 at the lower end and DR Cancri at the upper end. The reference star Praesepe is one of the brighter stars, and also an older name for the entire cluster.
Carbon star X Cancri can be found approx 140 Ly above this cluster."
(no image)
A Note On Planetary Nebulas
Due to the very large number of planetary nebula that have been submitted in the core region, we would ask that users not submit planetary nebula that are in and around the core, unless they are particularly interesting. "Particularly interesting" includes things such as: Multiple earth-like worlds in the system; ringed M- or K- class companion stars; all jumponium materials present; highly unusual gas giants or other planets; multiple interesting geyser/fumarole sites inside the nebula. Other criteria can match, but if it's just a planetary nebula without much else... you can skip the submission. Every additional submission adds to a crowded map.
By contrast, if you find a planetary nebula on the outskirts of the galaxy, in areas otherwise without much around - submit it! These help fill out underdeveloped areas.
Due to the very large number of planetary nebula that have been submitted in the core region, we would ask that users not submit planetary nebula that are in and around the core, unless they are particularly interesting. "Particularly interesting" includes things such as: Multiple earth-like worlds in the system; ringed M- or K- class companion stars; all jumponium materials present; highly unusual gas giants or other planets; multiple interesting geyser/fumarole sites inside the nebula. Other criteria can match, but if it's just a planetary nebula without much else... you can skip the submission. Every additional submission adds to a crowded map.
By contrast, if you find a planetary nebula on the outskirts of the galaxy, in areas otherwise without much around - submit it! These help fill out underdeveloped areas.
Thank you for this clarification.