Celebration of Early Astronomy / Expedições / EDSM

Expedições > Celebration of Early Astronomy

Resumo da expedição

Iniciando em	03/01/2020 19:00:00
Data de chegada	26/05/2020 23:59:59

Sistema inicial	Nu Tauri
Paradas	81
Sistema de destino	Trappist-1

Participantes	112
- Abandonment	71
- Success	42

Distância estimada	130.950,60 ano/luz

Anunciar expedição

Update 2022!

Celebration of Early Astronomy 5 is announced! Launching Jan 7 2023! Learn more about our latest expedition here!

Announcement: https://theexpedition.info/Announcement

And our trailer for it! https://theexpedition.info/Trailer

Our next expedition Celebration of Early Astronomy 2 has been officially announced! and will be taking Fleet Carriers to and returning from the Messier 67 star cluster: https://expedition.page.link/Announcement

-- Please make sure to sign up at the following link: https://forms.gle/FiKTvtYGdPQ3rwqc8 <- This is the official roster, the EDSM signup is just if you wish to track yourself.

"The early 2000s, they were often the speculative setting of early science fiction works. Early imaginings of interstellar travel, first contact with aliens, apocalypses, you name it, there was probably a movie or book set in the early 21st century of it. While humanity may not have invented interstellar travel by 2020 as many novels and films purported, they still discovered plenty of gems of our galaxy by then.

Lucky for us in 3305 we do have interstellar travel and can visit these gems that humans on Earth in the early 21st century could only dream of visiting. So that is just what we will be setting out to do. This expedition will visit many of the noteworthy celestial objects discovered by the early 21st century, some of which even still are considered noteworthy even today in 3305.

We will be setting off from the Simbad's Refuge station in Nu Tauri. Named after the SIMBAD star catalogue used in the late 20th and early 21st century, located in the Nu Tauri system of the Taurus constellation."

CMDR Kezika

Other information about the expedition can be found at https://theexpedition.info

Cronômetro da expedição

Esta expedição terminou.

Saltos até ao momento...

Distância total percorrida

Celestial bodies scanned

Celestial bodies mapped

Combustível usado

Probes used

Commanders dead

Commanders self destructed

Pontos de passagem da expedição

	Sistema	Distância do início	Participantes atingidos	Participantes visitados
#1	Nu Tauri		88,39%	76,79%	Nu Tauri http://simbad.u-strasbg.fr/simbad/sim-id?Ident=nu+tauri https://www.edsm.net/en/system/id/979/name/Nu+Tauri Basecamp: Simbad's Refuge (Asteroid Base) Coordinates: 8.65625, -62.78125, -98.3125 Nu Tauri is a star in the constellation Taurus. The asteroid base located here in the game is named after the SIMBAD database of celestial objects and will serve as the starting point of our expedition.
#2	W Ursae Majoris	186,49 ano/luz	87,50%	72,32%	W Ursae Majoris http://simbad.u-strasbg.fr/simbad/sim-basic?Ident=W+Ursae+Majoris&submit=SIMBAD+search https://www.edsm.net/en/system/id/27237/name/W+Ursae+Majoris Coordinates: -40, 117.15625, -104.03125 W Ursae Majoris is a binary star near to our departure point. It is too faint to see with the naked eye, but it can be viewed with the assistance of a telescope. The astronomical term "W Ursae Majoris variable" was named for this system, which refers to low mass eclipsing contact binaries.
#3	Betelgeuse	643,01 ano/luz	86,61%	71,43%	Betelgeuse http://simbad.u-strasbg.fr/simbad/sim-id?Ident=Betelgeuse&submit=submit+id https://www.edsm.net/en/system/id/23656/name/Betelgeuse Coordinates: 169.40625, -72.5, -462.625 Ninth brightest star in the night sky, and second brightest in the constellation Orion. Red supergiant of spectral type M1-2, one of the largest stars visible to the naked eye. This star is one of the shoulders of Orion.
#4	T Tauri (Hind Mine / Hind Nebula (T Tauri))	903,49 ano/luz	86,61%	70,54%	T Tauri (Hind Mine / Hind Nebula (T Tauri)) http://simbad.u-strasbg.fr/simbad/sim-id?Ident=T+Tau https://www.edsm.net/en/system/id/31528/name/T+Tauri Coordinates: -32.96875, -206.40625, -557-3125 The prototype star for the T Tauri class type of star, an early stage of stellar development for main sequence stars. For some reason this star is not actually a T Tauri class star in the game but shown as a G-class star, particluar reason is unknown, but perhaps despite odds it ended up finishing its T Tauri stage between 2019 and 3305, which is possible although unlikely.
#5	Y Canum Venaticorum	2.180,92 ano/luz	83,04%	65,18%	Y Canum Venaticorum http://simbad.u-strasbg.fr/simbad/sim-id?Ident=Y+Canum+Venaticorum&submit=submit+id https://www.edsm.net/en/system/id/2704366/name/Y+Canum+Venaticorum Coordinates: -264.8125, 993.90625, -186.75 Also known as "La Superba", this is the largest known Carbon Star. At a temperature of 2750K, it is one of the coldest known fusor stars. La Superba is most likely in the final stages of fusing it's remaining secondary fuel of helium into carbon and appears almost ready to eject its outer layers to form a planetary nebula, leaving behind its core in the form of a white dwarf.
#6	PSR J0751+1807 (Keck Binary Pulsar)	3.481,14 ano/luz	82,14%	69,64%	PSR J0751+1807 (Keck Binary Pulsar) Keck Binary Pulsar http://simbad.u-strasbg.fr/simbad/sim-id?Ident=PSR+J0751%2B1807&submit=submit+id https://www.edsm.net/en/system/id/3600665/name/PSR+J0751%2B1807 Coordinates: 470.09375, 469.125, -1122.21875 One of the earliest discovered millisecond pulsars, as discovered by the W. M. Keck observatory. It is accompanies by a white dwarf star, which is also notable for being one of the coldest and reddest among all known white dwarfs at a temperature of only 4,000K
#7	Pi Puppis (Pi Puppis Cluster (NGC 2451a))	4.562,74 ano/luz	80,36%	66,96%	Pi Puppis (Pi Puppis Cluster (NGC 2451a)) http://simbad.u-strasbg.fr/simbad/sim-basic?Ident=Pi+Puppis&submit=SIMBAD+search https://www.edsm.net/en/system/id/246667/name/Pi+Puppis Coordinates: 741.09375, -154.09375, -280.78125 Open cluster in the Puppis constellation. Discovered by Giovanni Battista Hodierna prior to 1654. Was postulated to be two open clusters lying along the same line of sight. This was later confirmed in the 20th century. The cluster's central star Pi Puppis is a red supergiant in its dying days. Is nearly 140 solar radii but only .5 solar masses.
#8	Vela Pulsar	4.829,24 ano/luz	80,36%	64,29%	Vela Pulsar http://simbad.u-strasbg.fr/simbad/sim-basic?Ident=Vela+Pulsar&submit=SIMBAD+search https://www.edsm.net/en/system/id/491743/name/Vela+Pulsar Coordinates: 905.9375, -44.40625, -102.40625 Brightest pulsar Recent news article: https://www.cnet.com/news/astronomers-watched-a-neutron-star-glitch-and-cant-yet-explain-it/
#9	HIP 38064 (Collinder 140 Open Cluster)	5.279,28 ano/luz	79,46%	65,18%	HIP 38064 (Collinder 140 Open Cluster) Collinder 140 Open Cluster http://simbad.u-strasbg.fr/simbad/sim-basic?Ident=HIP+38064&submit=SIMBAD+search http://simbad.u-strasbg.fr/simbad/sim-basic?Ident=Collinder+140&submit=SIMBAD+search https://www.edsm.net/en/system/id/40804/name/HIP+38064 Coordinates: 1152.9375, -60.6875, -478.25 One of multiple star clusters in the Canis Majoris constellation and contains approximately 40 stars. Estimated to be roughly 20 million years old and moves in the general direction of the Canis Majoris star stream. Its central star is HIP 38064. Planet 2 contains a tourist beacon with information on the original discovery of this area.
#10	VY Canis Majoris	5.899,31 ano/luz	79,46%	65,18%	VY Canis Majoris http://simbad.u-strasbg.fr/simbad/sim-id?Ident=VY+Canis+Majoris&submit=submit+id https://www.edsm.net/en/system/id/25862/name/VY+Canis+Majoris Coordinates: 1576.0625, -150.21875, -922.53125 The largest known star at the time of the in-game galaxy's creation. There have been larger stars, such as UY Scuti discovered since, but they do not appear in the game. At this time this is the largest known star in the in-game galaxy. It is a red hypergiant located in the constellation of Canis Major. If it was placed in the center of our solar system, its surface would extend beyond the orbit of Jupiter at the least. There is still considerable variation regarding the true radius of VY Canis Majoris, some estimates even have it large enough to extend past the orbit of Saturn.
#11	Mu Columbae	6.680,56 ano/luz	78,57%	63,39%	Mu Columbae http://simbad.u-strasbg.fr/simbad/sim-id?Ident=HR+1996&submit=submit+id https://www.edsm.net/en/system/id/8053372/name/Mu+Columbae Coordinates: 1001.6875, -598.625, -640.78125 A runaway star that was believed to be ejected from the Orion Nebula 4 to 5 million years ago by the supernova that created Barnard's Loop. It also is one of the few O-class stars that is visible to the unaided eye.
#12	Alnitak	7.470,11 ano/luz	78,57%	63,39%	Alnitak http://simbad.u-strasbg.fr/simbad/sim-basic?Ident=Alnitak&submit=SIMBAD+search https://www.edsm.net/en/system/id/20175/name/Alnitak Coordinates: 318.375, -203.15625, -632.03125 The easternmost star of Orion's Belt, a very recognizable landmark in the night sky. POI: There is a POI there named "Impressive Rings" on one of the other stars in the system.
#13	Mintaka	7.525,61 ano/luz	78,57%	63,39%	Mintaka http://simbad.u-strasbg.fr/simbad/sim-basic?Ident=Mintaka&submit=SIMBAD+search https://www.edsm.net/en/system/id/22048/name/Mintaka Coordinates: 270.625, -204.34375, -603.78125 The westernmost star of Orion's Belt, a very recognizable landmark in the night sky. Also was featured in an episode of Star Trek: The Next Generation POI: POI called "Blue Light" around A 4, 1,047 Ls away, Surface POI, 2.38G planet.
#14	Rigel	7.734,93 ano/luz	78,57%	63,39%	Rigel http://simbad.u-strasbg.fr/simbad/sim-id?Ident=Rigel&submit=submit+id https://www.edsm.net/en/system/id/25601/name/Rigel Coordinates: 385.78125, -360.40625, -682.53125 Rigel is the brightest star in the constellation Orion. It is expected to eventually end in supernova. Additionally it has two known companions Rigel B and Rigel C. You will be able to route to EZ Orionis once you enter into this system. Trying to route prior to reaching Rigel will most likely bump the router into the permit locked regions around Barnard's Loop.
#15	BD-12 1172 (Spirograph Nebula)	7.988,13 ano/luz	78,57%	64,29%	BD-12 1172 (Spirograph Nebula) Spirograph Nebula Basecamp: Planet 2 \| Bio Site 1 http://simbad.u-strasbg.fr/simbad/sim-basic?Ident=BD-12+1172&submit=SIMBAD+search https://www.edsm.net/en/system/id/15683/name/BD-12+1172 Coordinates: 577.875, -452.6875, -819.25 Officially designated as IC 418, The nebula has an intricate pattern to it resembling patterns made from a spirograph. POI: Sanchez Class Science Vessel POI: Notable Stellar Phenomena, in rings Prasinum Metalli Crystals in one of them Another with Rubeum Metallica Crystals, and Solid Mineral Spheres Third with Rubeum Metallic Crystals and Lattice Mineral Spheres
#16	EZ Orionis	8.230,53 ano/luz	75,89%	62,50%	EZ Orionis Begin Leg 2 http://simbad.u-strasbg.fr/simbad/sim-basic?Ident=EZ+Orionis&submit=SIMBAD+search https://www.edsm.net/en/system/id/21228/name/EZ+Orionis Coordinates: 578.09375, -426.65625, -1060.25 Part of the Orion Nebula
#17	OW Orionis	8.249,28 ano/luz	75,89%	61,61%	OW Orionis http://simbad.u-strasbg.fr/simbad/sim-id?Ident=OW+Orionis&submit=submit+id https://www.edsm.net/en/system/id/83379/name/OW+Orionis Coordinates: 595.25, -427.375, -1067.78125 The Orion Nebula is a diffuse nebula situated south of Orion's Belt in the constellation of Orion. It is one of the brightest nebulae in the night sky and is visible to the naked eye. It is also the closest region of massive star formation to our solar system. One of the most photographed objects in the night sky, and subject of intense study. Station nearby! POI: Orion Nebula Tourist Centre in PMD2009 48
#18	HD 39716	8.400,12 ano/luz	75,00%	60,71%	HD 39716 http://simbad.u-strasbg.fr/simbad/sim-id?Ident=HD+39716&submit=submit+id https://www.edsm.net/en/system/id/630694/name/HD+39716 Coordinates: 721.3125, -364.125, -1125.25 Positioned near Barnard's Loop, should be a good view of it from there.
#19	HR 1950	8.524,95 ano/luz	75,00%	60,71%	HR 1950 http://simbad.u-strasbg.fr/simbad/sim-id?Ident=HR+1950&submit=submit+id https://www.edsm.net/en/system/id/85136/name/HR+1950 Coordinates: 605, -386.6875, -1160.5625 Positioned near the Horsehead Nebula, should have a good view of the Horsehead Nebula
#20	Trapezium Sector CB-W c2-3	8.620,46 ano/luz	74,11%	60,71%	Trapezium Sector CB-W c2-3 Messier 78 SIMBAD: [http://simbad.u-strasbg.fr/simbad/sim-basic?Ident=Messier+78&submit=SIMBAD+search]http://simbad.u-strasbg.fr/simbad/sim-basic?Ident=Messier+78&submit=SIMBAD+search EDSM: [https://www.edsm.net/en/system/id/54219/name/Trapezium+Sector+CB-W+c2-3]https://www.edsm.net/en/system/id/54219/name/Trapezium+Sector+CB-W+c2-3 Coordinates: 538.53125, -321.5, -1139.25 Messier 78 is a nebula in the Barnard's Loop area, blue and black in colouration. It is a reflection Nebula discovered by Pierre Méchain in 1780 and then included by Charles Messier in his catalog that members of are now referred to as Messier objects. This object was also featured in the 1960s era Japanese anime Ultraman as the location of "The Land of Light" that acted as the homeworld of the Ultramen.
#21	Trapezium Sector VY-A c8	8.780,59 ano/luz	74,11%	59,82%	Trapezium Sector VY-A c8 Horsehead Nebula http://simbad.u-strasbg.fr/simbad/sim-id?Ident=Horsehead+Nebula&submit=submit+id https://www.edsm.net/en/system/id/550842/name/Trapezium+Sector+VY-A+c8 Coordinates: 607.5625, -417.875, -1246.90625 Also known as Barnard 33, is a dark nebula in the constellation Orion, located just south of Alnitak, the easternmost star of Orion's Belt, and is part of the Orion Molecular Cloud Complex. It appears in the southern region of the Lynds 1630 dust cloud. -- Trapezium Sector VY-A C5 seems like it should be the closest with the correct viewing angle of the Horsehead Nebula.
#22	HD 38563C	8.945,98 ano/luz	74,11%	59,82%	HD 38563C Basecamp: Planet ABCDE 1 J Coordinates: -23.8962, 87.232, -1400.84375 This system acts as our basecamp for this leg at the coordinates -23.8962, 87.232 on planet ABCDE 1 J. HD 38563 is a cluster of stars. In-game this includes the stars in this system as well as the stars in the systems titled "HD 38563 South" as well as "HD 38563North" which are in extremely close proximity to each other in terms of lightyears, but just far enough away from each other that they were made as seperate systems rather than a single one.
#23	DM99 58.3	9.281,45 ano/luz	73,21%	58,93%	DM99 58.3 This system marks the start of the Collinder 69 Open Cluster. SIMBAD Link: http://simbad.u-strasbg.fr/simbad/sim-id?Ident=%40797493&Name=%5bDM99%5d%20%2058&submit=submit
#24	BSM2011 e110	9.479,48 ano/luz	72,32%	56,25%	BSM2011 e110 This system marks the end of the Collinder 69 Open Cluster. SIMBAD Link: http://simbad.u-strasbg.fr/simbad/sim-id?Ident=BSM2011+E110&submit=submit+id
#25	AE Aurigae	10.269,24 ano/luz	71,43%	57,14%	AE Aurigae http://simbad.u-strasbg.fr/simbad/sim-id?Ident=Ae+Aurigae&submit=submit+id https://www.edsm.net/en/system/id/2582080/name/AE+Aurigae Coordinates: -246.71875, -54.6875, -1857.40625 A runaway star that was ejected from the Orion Nebula 4 to 5 million years ago by the supernova that created Barnard's Loop.
#26	EES2009 Persei J03286006+3122826	11.073,17 ano/luz	70,54%	55,36%	EES2009 Persei J03286006+3122826 This system marks the start of a cluster of real world objects known as NGC 1333 SIMBAD Link: http://simbad.u-strasbg.fr/simbad/sim-id?Ident=WMW2010+59&submit=submit+id
#27	2MASS J03292407+3119577	11.496,23 ano/luz	70,54%	55,36%	2MASS J03292407+3119577 This system marks the end of a cluster of real world objects known as NGC 1333 SIMBAD Link: http://simbad.u-strasbg.fr/simbad/sim-id?Ident=NGC+1333+IRS+2&submit=submit+id
#28	53 Arietis	11.774,27 ano/luz	70,54%	54,46%	53 Arietis http://simbad.u-strasbg.fr/simbad/sim-id?Ident=53+Arietis&submit=submit+id https://www.edsm.net/en/system/id/34271/name/53+Arietis Coordinates: -196.84375, -461.09375, -664.0625 A runaway star that was ejected from the Orion Nebula 4 to 5 million years ago by the supernova that created Barnard's Loop. Also known as UW Arietis
#29	HIP 102082 (HIP 102082 Carbon Star)	13.119,14 ano/luz	67,86%	50,00%	HIP 102082 (HIP 102082 Carbon Star) http://simbad.u-strasbg.fr/simbad/sim-basic?Ident=HIP+102082&submit=SIMBAD+search https://www.edsm.net/en/system/id/760935/name/HIP+102082 Coordinates: -1190.5, 76.375, 65.625 A very large carbon star with only twice the mass of our sun, but nearly 200 times the size of our sun.
#30	Alpha Cygni (Deneb (Alpha Cygni))	13.345,85 ano/luz	66,96%	49,11%	Alpha Cygni (Deneb (Alpha Cygni)) Deneb http://simbad.u-strasbg.fr/simbad/sim-basic?Ident=Deneb&submit=SIMBAD+search https://www.edsm.net/en/system/id/23434/name/Alpha+Cygni Coordinates: -1405, 46.125, 132.5 The brightest star in the Cygni constellation and 19th brightest star in the night sky. This star is hypothesized to be the star ionizing a band of interstellar dust between our solar system and the North America Nebula. Was also featured multiple times in the science fiction series Star Trek and its various iterations.
#31	Veil West Sector DL-Y d68 (Funfair Geysers / Veil Nebula West)	13.719,38 ano/luz	66,96%	52,68%	Veil West Sector DL-Y d68 (Funfair Geysers / Veil Nebula West) Veil West Nebula http://simbad.u-strasbg.fr/simbad/sim-basic?Ident=Deneb&submit=SIMBAD+search https://www.edsm.net/en/system/id/23434/name/Alpha+Cygni Coordinates: -1405, 46.125, 132.5 The brightest star in the Cygni constellation and 19th brightest star in the night sky. This star is hypothesized to be the star ionizing a band of interstellar dust between our solar system and the North America Nebula.
#32	North America Sector LC-V c2-3 (North America Nebula)	14.304,01 ano/luz	64,29%	49,11%	North America Sector LC-V c2-3 (North America Nebula) North America Nebula http://simbad.u-strasbg.fr/simbad/sim-basic?Ident=NGC+7000&submit=SIMBAD+search https://www.edsm.net/en/system/id/28554/name/North+America+Sector+LC-V+c2-3 Coordinates: -1891.46875, -30.8125, 150.5 Officially designated as NGC 7000, it is a very large, but very dim nebula, so despite taking up a larger area in the sky than the full moon, it is not visible unaided to the naked eye. Even regular telescopes will merely show it as a foggy patch of light, even in the most dark skies. The shape of the nebula resembles the North American continent, including a prominent Gulf of Mexico. The section resembling Mexico and Central America is the Cygnus Wall. It is hypothesized that the star Deneb, is ionizing a band of interstellar dust between Earth and the North American and Pelican nebulae causing it to appear in the shape it does to us from Earth.
#33	North America Sector JH-V c2-26 (Pelican Nebula)	14.343,06 ano/luz	64,29%	50,00%	North America Sector JH-V c2-26 (Pelican Nebula) Pelican Nebula http://simbad.u-strasbg.fr/simbad/sim-basic?Ident=IC+5070&submit=SIMBAD+search https://www.edsm.net/en/system/id/35057/name/North+America+Sector+JH-V+c2-26 Coordinates: -1886.625, -0.15625, 174.1875 Officially designated as IC 5070, a nebula that is associated with and near the North America Nebula. It is the subject of study due to being a particularly active mix of star formation and evolving gas clouds. It is expected to look vastly different within millions of years, unlike most other nebulae.
#34	S171 43	15.981,51 ano/luz	64,29%	50,00%	S171 43 This star is part of the NGC 7822 nebula and stellar formation region. SIMBAD Links: http://simbad.u-strasbg.fr/simbad/sim-id?Ident=%5BGMM2009%5D+S171+43&submit=submit+id http://simbad.u-strasbg.fr/simbad/sim-basic?Ident=NGC+7822&submit=SIMBAD+search
#35	Hypoae Ain MO-I d9-37 (Heart & Soul Nebulae)	20.805,07 ano/luz	62,50%	47,32%	Hypoae Ain MO-I d9-37 (Heart & Soul Nebulae) Heart and Soul Nebulae POI: Heart Nebula http://simbad.u-strasbg.fr/simbad/sim-id?Ident=Heart+Nebula&submit=submit+id POI: Soul Nebula http://simbad.u-strasbg.fr/simbad/sim-id?Ident=IC+1848&submit=submit+id https://www.edsm.net/en/system/id/2325302/name/Hypoae+Ain+MO-I+d9-37 Coordinates: -5150.90625, 98.625, -5326.6875 Major star formation region that forms two nebula. The Heart Nebula is so named because of it's resemblance to a human heart when viewed from Earth. The Soul Nebula is also known as the Embryo Nebula. Stations nearby! POI: Base Camp in Soul Sector EL-Y d7 POI: Farsight Expedition Base in Heart Sector IR-V B2-0
#36	RS Persei	21.445,89 ano/luz	61,61%	45,54%	RS Persei http://simbad.u-strasbg.fr/simbad/sim-id?Ident=RS+Persei&submit=submit+id https://www.edsm.net/en/system/id/449812/name/RS+Persei Coordinates: -5405.78125, -481.90625, -5419.8125 Red Supergiant located in the Double Cluster (Caldwell 14) in the Perseus constellation. In the game galaxy version it is orbited by a landable planet so close that you can fuel scoop while in orbital flight. NGC 281
#37	Bubble Sector PD-S b4-4 (Bubble Nebula)	24.466,40 ano/luz	60,71%	49,11%	Bubble Sector PD-S b4-4 (Bubble Nebula) Bubble Nebula http://simbad.u-strasbg.fr/simbad/sim-id?Ident=Bubble+Nebula&submit=submit+id https://www.edsm.net/en/system/id/67028/name/Bubble+Sector+PD-S+b4-4 Coordinates: -6570.5, 29.84375, -2680.28125 Also known as NGC 7635, Sharpless 162, or Caldwell 11, it is an emission nebula in the constellation of Cassiopeia. The bubble is created by the stellar wind from a massive central star SAO 20575.
#38	Mu Cephei	26.255,94 ano/luz	56,25%	43,75%	Mu Cephei http://simbad.u-strasbg.fr/simbad/sim-id?Ident=Mu+Cephei&submit=submit+id https://www.edsm.net/en/system/id/2531913/name/Mu+Cephei Coordinates: -5806.46875, 451, -1117.8125 One of the largest red supergiants. Also known as Herschel's Garnet Star. In the constellation Cepheus. Since 1943 the spectrum of this star has served as the M2 Ia standard by which other stars are classified. It is one of the largest known stars, and if it was placed in the center of our solar system would extend to between the orbits of Jupiter and Saturn.
#39	KY Cygni	28.723,68 ano/luz	56,25%	43,75%	KY Cygni http://simbad.u-strasbg.fr/simbad/sim-id?Ident=KY+Cygni&submit=submit+id https://www.edsm.net/en/system/id/25043/name/KY+Cygni Coordinates: -4871.9375, 15.75, 1124.28125 One of the top 10 largest known stars. If placed in the center of the solar system, it would extend past the orbit of Jupiter. It is also quite close to the Crescent Nebula. It is estimated to go supernova within 2 million years. Station nearby! POI: Medusa's Rock in Crescent Sector GW-W C1-8
#40	HIP 101364 (Cygnus OB2-12)	31.901,40 ano/luz	55,36%	42,86%	HIP 101364 (Cygnus OB2-12) Begin Leg 5 Cygnus OB2-12 http://simbad.u-strasbg.fr/simbad/sim-basic?Ident=HIP+101364&submit=SIMBAD+search https://www.edsm.net/en/system/id/8664337/name/HIP+101364 Coordinates: -8040.375, 94.25, 1353.875 A Blue Hypergiant in the Cygnus OB2 Association, one of the heaviest known areas of star formation in the Mily Way. It is 2 million times as luminous as Sol, and one of the brightest stars in the galaxy.
#41	V1357 Cygni	33.341,88 ano/luz	55,36%	42,86%	V1357 Cygni http://simbad.u-strasbg.fr/simbad/sim-basic?Ident=V1357+Cygni&submit=SIMBAD+search https://www.edsm.net/en/system/id/53352/name/V1357+Cygni Coordinates: -7095.375, 401.25, 2396.8025 Binary system of a black hole and a blue giant. Discovered in 1964 due to the very high levels of x-rays produced by mass of the blue giant falling into the black hole. Was the first source of such powerful x-rays that was widely accepted to be a black hole.
#42	Csi+19-20105 (NGC 6886)	36.022,69 ano/luz	55,36%	42,86%	Csi+19-20105 (NGC 6886) NGC 6886 http://simbad.u-strasbg.fr/simbad/sim-basic?Ident=NGC+6886 https://www.edsm.net/en/system/id/121063/name/Csi%2B19-20105 Coordinates: -7731.75, -1205.90625, 4445.90625 Planetary nebula in the constellation Sagitta around a Wolf-Rayet star. Discovered by Ralph Copeland on September 17, 1884.
#43	Lgm-1 (LGM-1 Pulsar)	37.922,25 ano/luz	54,46%	41,07%	Lgm-1 (LGM-1 Pulsar) http://simbad.u-strasbg.fr/simbad/sim-basic?Ident=PSR+B1919%2B21&submit=SIMBAD+search https://www.edsm.net/en/system/id/677507/name/Lgm-1 Coordinates: -7533.46875, 557.34375, 5124.125 Official designation: PSR B1919+21 First ever discovered pulsar in 1967. Due to the nature of pulsars as a repeating radio source not being a known phenomenon at the time, it was at first thought to be a signal from an alien intelligence. Originally named LGM-1 standing for "Little Green Men" because of that assumption. Later observation into it led to the discovery of pulsars and their nature.
#44	PSR J1901+0716	40.366,82 ano/luz	54,46%	41,07%	PSR J1901+0716 http://simbad.u-strasbg.fr/simbad/sim-basic?Ident=PSR+J1901%2B0716&submit=SIMBAD+search https://www.edsm.net/en/system/id/5477849/name/PSR+J1901%2B0716 Coordinates: -5935,46875, 168.25, 6932.6875 An unusual pulsar that changes its pulse length down from 644ms temporarily on occasion. The cause of this behaviour is unknown.
#45	V1343 Aquilae	47.276,43 ano/luz	53,57%	39,29%	V1343 Aquilae http://simbad.u-strasbg.fr/simbad/sim-basic?Ident=V1343+Aquilae&submit=SIMBAD+search https://www.edsm.net/en/system/id/15272950/name/V1343+Aquilae Coordinates: -10211.1875, -626.65625, 12301.96875 Microquasar that emits x-ray radiation. Consists of an A-class star and a black hold named SS 433
#46	PSR J1846-0258 (The Kes-75 Magnetar)	50.847,86 ano/luz	53,57%	41,07%	PSR J1846-0258 (The Kes-75 Magnetar) Kes-75 Magnetar http://simbad.u-strasbg.fr/simbad/sim-basic?Ident=PSR+J1846-0258&submit=SIMBAD+search https://www.edsm.net/en/system/id/2715365/name/PSR+J1846-0258 Coordinates: -8886.75, -75.15625, 15572.5625 The youngest known pulsar to exist. Believed to be a magnetar, a type of pulsar that has an extremely powerful magnetic field. -- Station after this one near route to next waypoint POI: Polo Harbour in Boewnst KS-S C20-959
#47	XTE J1752-223	57.990,33 ano/luz	53,57%	40,18%	XTE J1752-223 http://simbad.u-strasbg.fr/simbad/sim-basic?Ident=XTE+J1752-223&submit=SIMBAD+search https://www.edsm.net/en/system/id/53326/name/XTE+J1752-223 Coordinates: -1900.5, 627.125, 16881.78125 A low-intermediate mass black hole of 118 solar masses with dramatic outbursts of increased emission, first discovered as an active radio source in 2009. In game this system is interesting for being a black hole with an asteroid belt.
#48	GRS 1758-258	59.508,21 ano/luz	53,57%	40,18%	GRS 1758-258 Begin Leg 6 http://simbad.u-strasbg.fr/simbad/sim-id?Ident=GRS+1758-258 https://www.edsm.net/en/system/id/53355/name/GRS+1758-258 Coordinates: -1257.1875, -380.0625, 15946 The first discovered winged microquasar
#49	OGLE235-MOA53	60.847,65 ano/luz	52,68%	39,29%	OGLE235-MOA53 This system contains a confirmed extrasolar planet discovered in 2003 during the Optical Gravitation Lensing Experiment. http://simbad.u-strasbg.fr/simbad/sim-id?Ident=%403755458&Name=NAME%20OGLE%202003-BLG-235Lb&submit=submit https://www.edsm.net/en/system/id/53345/name/OGLE235-MOA53 Coordinates: -650.1875, -1092.375, 16904.25 Description needed
#50	OGLE-2007-BLG-368L	63.427,83 ano/luz	52,68%	39,29%	OGLE-2007-BLG-368L http://simbad.u-strasbg.fr/simbad/sim-id?Ident=OGLE-2007-BLG-368L https://www.edsm.net/en/system/id/46422/name/OGLE-2007-BLG-368L Coordinates: 552.9375, -1236.3125, 19182.21875 In 2009 during a gravitational microlensing event, a Neptune-mass planet was discovered with a distance of 3.3 AU and a mass 22 times that of Earth.
#51	GRS 1730-312	65.912,81 ano/luz	52,68%	37,50%	GRS 1730-312 http://simbad.u-strasbg.fr/simbad/sim-basic?Ident=GRS+1730-312&submit=SIMBAD+search https://www.edsm.net/en/system/id/45864/name/GRS+1730-312 Coordinates: 1216.8125, 20961.5, 366.34375 First detected in 1994 by the GRANAT orbital observatory and Kvant module on the space station Mir. Was the most intensive X-ray source in the galactic center region.
#52	OGLE-05-390L	67.669,31 ano/luz	52,68%	37,50%	OGLE-05-390L OGLE-05-390L This system contains a confirmed extrasolar planet discovered by the Optical Gravitational Lensing Experiment. http://simbad.u-strasbg.fr/simbad/sim-id?Ident=%402430171&Name=NAME%20OGLE%202005-BLG-390Lb&submit=submit https://www.edsm.net/en/system/id/45038/name/OGLE-05-390L Coordinates: 100.25, -885.9375, 21481.5 In the year of 2005 gravitational microlensing showed that it was very plausible, that this distant system would contain an extrasolar planet (source). More than a millenia should pass however, before this early discovery of an exoplanet were confirmed by deep space explorers. The planet itself is a class 1 Jovian.
#53	PSR J1748-2446A	70.364,04 ano/luz	52,68%	36,61%	PSR J1748-2446A http://simbad.u-strasbg.fr/simbad/sim-basic?Ident=PSR+J1748-2446A&submit=SIMBAD+search https://www.edsm.net/en/system/id/5452479/name/PSR+J1748-2446A Coordinates: -1538.125, 680.8125, 22938.40625 The currently fastest known spinning celestial object, spinning at 716 RPS (Rotation Per Second) and an equator that moves at roughly 25% of c.
#54	Sagittarius A*	73.785,63 ano/luz	52,68%	49,11%	Sagittarius A* POI: http://simbad.u-strasbg.fr/simbad/sim-id?Ident=Sagittarius+A&submit=submit+id S2 POI: http://simbad.u-strasbg.fr/simbad/sim-id?Ident=%5BEG97%5D+S2 https://www.edsm.net/en/system/id/25635/name/Sagittarius+A%2A Coordinates: 25.21875, -20.90625, 25899.96875 Sagittarius A is the Supermassive Black Hole at the center of the Milky Way Galaxy, the type of black hole generally accepted to be at the center of most, if not all spiral and elliptical galaxies. Observations of stars, most notably S2 that orbit around Sagittarius A have been used to show the presence of a supermassive black hole at that location. S2's highly eccentric orbit and proximity to Sagittarius A has been instrumental for scientists use in determining the location and mass of Sagittarius A. At it's closest to Sagittarius A S2 was recorded to travel at a speed of 7650 km/s, or 2.55% the speed of light. Station nearby! POI: Explorer's Anchorage in Stuemeae FG-Y D7561
#55	G2 Dust Cloud Sector JH-V c2-7255	75.787,77 ano/luz	42,86%	37,50%	G2 Dust Cloud Sector JH-V c2-7255 G2 Gas Cloud Basecamp: Body A 2 E @ 60.2937, -119.28 POI: G2 Dust Cloud Sector JH-V C2-7255 http://simbad.u-strasbg.fr/simbad/sim-basic?Ident=Name+G2+Dust+Cloud&submit=SIMBAD+search https://www.edsm.net/en/system/id/1395969/name/G2+Dust+Cloud+Sector+JH-V+c2-7255 The remnant of an event in 2013 of a gas cloud roughly three times the mass of earth passing within 36 lighthours of Sagittarius A. It survived the encounter and has continued moving past Sagittarius A since 2013.
#56	GRS 1737-31	76.947,34 ano/luz	42,86%	37,50%	GRS 1737-31 Begin Leg 7 http://simbad.u-strasbg.fr/simbad/sim-basic?Ident=GRS+1737-31&submit=SIMBAD+search https://www.edsm.net/en/system/id/35865/name/GRS+1737-31 Coordinates: 1178.375, -48.40625, 27975.125 GRS 1737-31 is a stellar-mass black hole located in the Galactic Bar. This system was first observed in the year 1997 during observations of the galactic core, where it was detected as a source of gamma and X-rays. Today, three other stars have been found in the system; two of very hot O-class, and one hot B-class. The high mass and very similar young age of these objects suggests that they originate from a similar area. Orbital periods are also quite short, which appears to point towards either a shared origin or capture. No planets are present in this system.
#57	SLX 1746-331	78.691,60 ano/luz	42,86%	37,50%	SLX 1746-331 http://simbad.u-strasbg.fr/simbad/sim-basic?Ident=SLX+1746-331&submit=SIMBAD+search https://www.edsm.net/en/system/id/19332584/name/SLX+1746-331 Coordinates: 1501.90625, -1400.53125, 26921.78125 A low mass X-ray source with regular outbursts every 5-10 years located in the galaxy center 2000 light years from Sagittarius A*. The main body of the system is a black hole of 170 solar masses which makes it one of the most massive objects of this type in the galaxy. It is orbited by three ordinary white stars and also a neutron star which itself is orbited by 3 brown dwarfs and an Y-type dwarf. 4 D A had a good view from it at -22.0209, -130.3600 with the black hole, the neutron star, and the G class star near each other in the sky.
#58	V821 Arae	87.084,12 ano/luz	41,07%	35,71%	V821 Arae More commonly known as GX 339-4 http://simbad.u-strasbg.fr/simbad/sim-basic?Ident=GX+339-4&submit=SIMBAD+search https://www.edsm.net/en/system/id/53349/name/V821+Arae Coordinates: 9675, -2036.84375, 25124.5625 GX 339-4 is a moderately strong variable galactic low-mass X-ray binary source and black-hole candidate that flares from time to time. From spectroscopic measurements, the mass of the black-hole was found to be at least of 5.8 solar masses. During the outbursts GX 339-4 shows evolution of quasi-periodic oscillations
#59	GHJ2008 3	88.574,98 ano/luz	41,07%	35,71%	GHJ2008 3 http://simbad.u-strasbg.fr/simbad/sim-basic?Ident=GHJ2008+3&submit=SIMBAD+search https://www.edsm.net/en/system/id/53397/name/GHJ2008+3 Coordinates: 10258.15625, -1554.25, 23840.15625 The least massive known black hole in existence at only 3.8 solar masses.
#60	V381 Normae	98.427,37 ano/luz	41,07%	35,71%	V381 Normae http://simbad.u-strasbg.fr/simbad/sim-basic?Ident=V381+Normae&submit=SIMBAD+search https://www.edsm.net/en/system/id/53396/name/V381+Normae Coordinates: 9530.28125, -542, 14066.96875 Low mass X-ray binary, black hole, and gamma ray source
#61	Circinus Pulsar (The Circinus Pulsar)	100.088,17 ano/luz	41,07%	35,71%	Circinus Pulsar (The Circinus Pulsar) http://simbad.u-strasbg.fr/simbad/sim-basic?Ident=+PSR+1509-58&submit=SIMBAD+search https://www.edsm.net/en/system/id/53348/name/Circinus+Pulsar Coordinates: 10852.09375, -344.6875, 13081 Official Desingation: PSR 1509-58; A pulsar with a very distant 4.4-solar mass orbiting black hole situated within the Scutum-Centaurus Arm, approx. 17,000 LYs from Sol.
#62	TrA X-1	103.214,34 ano/luz	41,07%	35,71%	TrA X-1 Begin Leg 8 http://simbad.u-strasbg.fr/simbad/sim-basic?Ident=TrA+X-1&submit=SIMBAD+search https://www.edsm.net/en/system/id/7302429/name/TrA+X-1 Coordinates: 8912.4375, -1080.71875, 10742.4375 First discovered in 1974 and classified as an X-Ray Nova, it was for a brief time emitting more X-Ray emission than the entire Crab Nebula. In-game it is a trinary black hole system
#63	PSR J1709-4429	110.648,07 ano/luz	41,07%	35,71%	PSR J1709-4429 http://simbad.u-strasbg.fr/simbad/sim-basic?Ident=PSR+J1709-4429&submit=SIMBAD+search https://www.edsm.net/en/system/id/53334/name/PSR+J1709-4429 Coordinates: 2272.21875, -366.625, 7477.78125 One of the EGRET six pulsars, studied between 1991 and 2002 and was early evidence that pulsars are the best sources of high-energy gamma ray radiation, an important milestone in astronomy.
#64	V1033 Scorpii	111.424,12 ano/luz	40,18%	33,93%	V1033 Scorpii http://simbad.u-strasbg.fr/simbad/sim-basic?Ident=V1033+Scorpii&submit=SIMBAD+search https://www.edsm.net/en/system/id/53353/name/V1033+Scorpii Coordinates: 2071.0625, 342.8125, 7719.625 Contains the black hole GRO J1655-40, a microquasar. Also near the NGC 6357 nebula, also known as the Lobster Nebula.
#65	Cl Pismis 2 (NGC 6357)	112.606,32 ano/luz	40,18%	33,93%	Cl Pismis 2 (NGC 6357) Pismis 24-1 POI: Pismis 24-1NE http://simbad.u-strasbg.fr/simbad/sim-basic?Ident=Pismis+24-1NE&submit=SIMBAD+search POI: Pismis 24-1SW http://simbad.u-strasbg.fr/simbad/sim-basic?Ident=Pismis+24-1SW&submit=SIMBAD+search Lobster Nebula POI: http://simbad.u-strasbg.fr/simbad/sim-basic?Ident=NGC+6357&submit=SIMBAD+search https://www.edsm.net/en/system/id/44945/name/Cl+Pismis+2 Coordinates: 963.65625, 142.0625, 8081.5 Originally thought to be one single massive star of over 300 stellar masses, that would've been the most massive star. However, it was later discovered to be two massive O Class stars that are both themselves still individually amongst the largest known stars in existence. Those are Pismis 24-1NE and Pismis 24-1SW. These are located within the Lobster Nebula, which is one of the most prominent sites of massive-star formation in our neighborhood of the Milky Way, containing a variety of O-type stars.
#66	BD-21 4483 (IC 4634)	114.523,56 ano/luz	40,18%	33,04%	BD-21 4483 (IC 4634) Begin Leg 9 http://simbad.u-strasbg.fr/simbad/sim-id?Ident=BD-21+4483+&submit=submit+id https://www.edsm.net/en/system/id/2715430/name/BD-21+4483 Coordinates: -51.1875, 1584.90625, 7330.4375 Wolf-Rayet N star located within a green planetary nebula.
#67	CD-23 14350 (NGC 6629)	117.112,68 ano/luz	39,29%	34,82%	CD-23 14350 (NGC 6629) NGC 6629 http://simbad.u-strasbg.fr/simbad/sim-basic?Ident=NGC+6629&submit=SIMBAD+search https://www.edsm.net/en/system/id/7107016/name/CD-23+14350 Coordinates: -1041.15625, -568.9375, 6289.0625 A nebula discovered in 1784 by William Herschel at the beginning of his second deep sky survey. The white core of the nebula is a Wolf-Rayet star surrounded by a blue and purple planetary nebula.
#68	SSTGLMC G014.1819-00.5307	118.230,99 ano/luz	38,39%	33,93%	SSTGLMC G014.1819-00.5307 This is a cluster of stars along the route that may have some interesting members in it. They are considered "intrinsically res sources" and were studied by the Spitzer telescope. SSTGLMC G014.1819-00.5307 14.1819 -0.5307 274.5486 -16.8753 12.34 10.88 10.09 9.41 10.93 9.17 5.05 AI Information about the star cluster that this system is a part of can be found here: https://iopscience.iop.org/1538-3881/136/6/2413/suppdata/aj285677t2_mrt.txt
#69	SO4-H1E 2000 (Guardians of Scorpius)	121.793,21 ano/luz	38,39%	33,93%	SO4-H1E 2000 (Guardians of Scorpius) Zeta-1 Scorpii POI: http://simbad.u-strasbg.fr/simbad/sim-id?Ident=zet01+Sco HR 6260 POI: http://simbad.u-strasbg.fr/simbad/sim-id?Ident=HR+6260&submit=submit+id https://www.edsm.net/en/system/id/3095069/name/SO4-H1E+2000 Coordinates: 734.65625, 14, 2460.84375 Located on the near edge of the Sagittarius Gap, two blue-white hyper-giants are found just 32 Ly apart. HR 6260 (also known as HD 152234) and SO4-H1E 2000 (also known as Zeta-1 Scorpii) serve as warning beacons for travelers about to enter the Sagittarius Gap. These hyper-giants are both part of the extended open cluster NGC 6231. Zeta-1 Scorpii was known by earth astronomers from antiquity, and is currently classified as one of the very rare 'S Doradus' type of variable star.
#70	HD 112272 (Variabilis)	123.467,79 ano/luz	36,61%	32,14%	HD 112272 (Variabilis) http://simbad.u-strasbg.fr/simbad/sim-id?Ident=HD+112272&submit=submit+id https://www.edsm.net/en/system/id/2837484/name/HD+112272 Coordinates: 1934.625, -72.09375, 1296 This star (also known as HIPP 63170) is a variable class-A super-giant. As an Alpha Cygni type variable, the star has irregular pulsations with periods from several days to several weeks, and brightens up to 0.1 magnitude. The system also has a total of 8 stellar bodies below the limit for hydrogen fusion (class L, T and Y dwarves). Many of these hot dwarves have ring systems.
#71	OGLE2-TR-L9	124.317,14 ano/luz	36,61%	32,14%	OGLE2-TR-L9 This system contains a confirmed extrasolar planet discovered by the Optical Gravitational Lensing Experiment. http://simbad.u-strasbg.fr/simbad/sim-id?Ident=%404981397&Name=NAME%20OGLE2-TR-L9b&submit=submit https://www.edsm.net/en/system/id/53346/name/OGLE2-TR-L9 Coordinates: 2744, -38.0625, 1040.75 This star is home to the transiting extrasolar planet OGLE2-TR-L9b discovered in 2008 AD.
#72	QZ Carinae	125.305,95 ano/luz	36,61%	32,14%	QZ Carinae http://simbad.u-strasbg.fr/simbad/sim-id?Ident=QZ+Carinae&submit=submit+id https://www.edsm.net/en/system/id/34123/name/QZ+Carinae Coordinates: 1857.125, -36.25, 603.5 QZ Carinae (also called HD 93026) consists of three massive and highly luminous O-class stars, with a total of 121 solar masses. As seen from Sol, this system appears as one of the brightest stars in the Carina Nebula.
#73	OGLE-TR-113	125.465,76 ano/luz	36,61%	32,14%	OGLE-TR-113 The star of this system is also known as V752 Carinae, the system also contains a confirmed extrasolar planet that was discovered by the Optical Gravitational Lensing Experiment. http://simbad.u-strasbg.fr/simbad/sim-id?Ident=%403206263&Name=NAME%20OGLE-TR-113b&submit=submit https://www.edsm.net/en/system/id/53347/name/OGLE-TR-113 Coordinates: 1699, -56.21875, 591.71875 In the 21st Century (2002 AD) the Optical Gravitational Lensing Experiment (OGLE) detected periodic dimming in the star's light curve indicating a transiting, planetary-sized object. Since low-mass red dwarfs and brown dwarfs may mimic a planet, radial velocity measurements were necessary to calculate the mass of the body. In 2004, the object was proved to be a new transiting extrasolar planet.
#74	Shapley 1 (Shapley 1 (The Fine Ring Nebula))	126.684,38 ano/luz	36,61%	32,14%	Shapley 1 (Shapley 1 (The Fine Ring Nebula)) Fine Ring Nebula http://simbad.u-strasbg.fr/simbad/sim-id?Ident=%403474714&Name=PN%20Sp%20%20%20%201&submit=submit https://www.edsm.net/en/system/id/35977/name/Shapley+1 Coordinates: 513.21875, 34.875, 857.53125 The Fine Ring Nebula, planetary nebula with a unique ring structure. Has a Wolf-Rayet star inside.
#75	HR 6164 (The View)	127.115,99 ano/luz	35,71%	32,14%	HR 6164 (The View) The View http://simbad.u-strasbg.fr/simbad/sim-id?Ident=HR+6164&submit=submit+id https://www.edsm.net/en/system/id/21566/name/HR+6164 Coordinates: 444.34375, 58.3125, 1282.96875
#76	46 Upsilon Sagittarii	128.362,72 ano/luz	35,71%	32,14%	46 Upsilon Sagittarii http://simbad.u-strasbg.fr/simbad/sim-basic?Ident=HR+7342&submit=SIMBAD+search https://www.edsm.net/en/system/id/193544/name/46+Upsilon+Sagittarii Coordinates: -653.1875, -442, 1598.3125 A blue supergiant visible from Earth by the naked eye. Also listed as a green system in case you need to restock on your FSD injection materials. Mammon Monitoring Facility is also near this location if you are looking to offload some of your data. Station near route from this waypoint to next: POI: Mammon Monitoring Facility in Mammon
#77	Snake Sector PD-S b4-1	129.642,56 ano/luz	35,71%	31,25%	Snake Sector PD-S b4-1 Additional viewing suggestion: The get the same angle as from Sol and more of the "snake" shape: Pipe (Stem) Sector QT-R C4-8 Snake Nebula http://simbad.u-strasbg.fr/simbad/sim-basic?Ident=Barnard+72&submit=SIMBAD+search https://www.edsm.net/en/system/id/112483/name/Snake+Sector+PD-S+b4-1 Coordinates: -14.4375, 69.90625, 614.46875 A thin wavy "snake shaped" dark nebula, also known as Barnard 72
#78	Antares	129.780,34 ano/luz	35,71%	31,25%	Antares NOTE: For some reason this system has you jump in to the secondary star rather than the primary star. The primary star Antares is actually the point of interest. http://simbad.u-strasbg.fr/simbad/sim-basic?Ident=Antares&submit=SIMBAD+search https://www.edsm.net/en/system/id/20242/name/Antares Coordinates: 71.5, 138.40625, 531.375 The 15th brightest star in the night sky and the brightest star in the Scorpius constellation. It is often referred to as The Heart of the Scorpion because of its distinct red hue when viewed with the naked eye. It is a red supergiant and among the largest known stars. It also has a companion star Antares B which is a typical B-class star.
#79	HR 6628	129.955,75 ano/luz	35,71%	32,14%	HR 6628 http://simbad.u-strasbg.fr/simbad/sim-basic?Ident=HR+6628&submit=SIMBAD+search https://www.edsm.net/en/system/id/243252/name/HR+6628 Coordinates: 15.78125, -26.125, 555.75 Real star along the route that should be visible to the naked eye from Earth as well.
#80	HIP 84605 (The Great Rift)	130.048,32 ano/luz	35,71%	32,14%	HIP 84605 (The Great Rift) Pipe Nebula http://simbad.u-strasbg.fr/simbad/sim-basic?Ident=HIP+84605&submit=SIMBAD+search https://www.edsm.net/en/system/id/176894/name/HIP+84605 Coordinates: 9.625, 51.75, 506.09375 SIMBAD Links POI: http://simbad.u-strasbg.fr/simbad/sim-basic?Ident=Barnard+59&submit=SIMBAD+search POI: http://simbad.u-strasbg.fr/simbad/sim-basic?Ident=Barnard+65&submit=SIMBAD+search POI: http://simbad.u-strasbg.fr/simbad/sim-basic?Ident=Barnard+66&submit=SIMBAD+search POI: http://simbad.u-strasbg.fr/simbad/sim-basic?Ident=Barnard+67&submit=SIMBAD+search POI: http://simbad.u-strasbg.fr/simbad/sim-basic?Ident=Barnard+78&submit=SIMBAD+search Description needed A dark nebula shaped like a smoking pipe.
#81	PSR J1856-3754 (Coronet Pulsar)	130.254,61 ano/luz	35,71%	32,14%	PSR J1856-3754 (Coronet Pulsar) Coronet Pulsar http://simbad.u-strasbg.fr/simbad/sim-basic?Ident=PSR+J1856-3754&submit=SIMBAD+search https://www.edsm.net/en/system/id/449175/name/PSR+J1856-3754 Coordinates: 12.09375, -154.375, 498.09375 The 'Coronet' Pulsar is the colloquial term for the double neutron star system of PSR J1856-3754, the closest pulsar to Sol with a mere 521 light years. It lies in the Corona Austrinae molecular cloud and is associated with the so-called Coronet Cluster (CrA), a small cluster of young stars embedded in a small emission nebula (R CrA/NGC 6729) in that same region. The pulsar is also a member of the Magnificent Seven, a group of isolated neutron stars that are all relatively close to Sol and fall in line with the Gould Belt. The pulsar was once suspected to be a quark star, a hypothetical type of compact exotic star composed of quark matter, where extremely high temperature and pressure forces nuclear particles to dissolve into a continuous phase consisting of free quarks. Later observations determined it did not have sufficient temperature and size for this type of star.
#82	HIP 91911	130.548,24 ano/luz	35,71%	32,14%	HIP 91911 http://simbad.u-strasbg.fr/simbad/sim-basic?Ident=HIP+91911&submit=SIMBAD+search https://www.edsm.net/en/system/id/593506/name/HIP+91911 Coordinates: -204.28125, 5.0625, 367.3125 Wolf-Rayet Star near the route back.
#83	Trappist-1	130.950,60 ano/luz	35,71%	35,71%	Trappist-1 http://simbad.u-strasbg.fr/simbad/sim-basic?Ident=TRAPPIST-1&submit=SIMBAD+search https://www.edsm.net/en/system/id/10435482/name/Trappist-1 Coordinates: -21.65625, -35, 10.03125 We end out expedition at the system where the real world and the Elite: Dangerous procedurally generated galaxy collided with each other. In early 2017 astronomers discovered seven approximately Earth-sized rocky exoplanets in orbit of Trappist-1. Three of which were within the habitable zone of this ultra-cool red dwarf star roughly 39.5 light years from Earth. Players of Elite: Dangerous quickly realized that there was a system in roughly the correct location called Core Sys Sector XU-P A5-0 at 42 Ly from Sol that happened to be a brown dwarf, not much colder than the red dwarf named Trappist-1 with seven terrestrial worlds around it. The system was officially tweaked to be a red dwarf and renamed to Trappist-1 for the 2.3 update.