mirror of
https://github.com/OpenSpace/OpenSpace.git
synced 2026-01-06 11:39:49 -06:00
reworked decription and meta for orion nebula (#1429)
* reworked decription and meta for orion nebula * update orion gui path * update gui path for transform
This commit is contained in:
@@ -23,18 +23,9 @@ local OrionClusterStars = {
|
||||
},
|
||||
GUI = {
|
||||
Name = "Orion Nebula Star Cluster",
|
||||
Path = "/Milky Way/Stars"
|
||||
}
|
||||
}
|
||||
|
||||
assetHelper.registerSceneGraphNodesAndExport(asset, { OrionClusterStars })
|
||||
|
||||
|
||||
asset.meta = {
|
||||
Name = "Orion Nebula Star Cluster",
|
||||
Version = "1.0",
|
||||
Description = [[ In order to have an accurate depiction of the Orion nebula, we need
|
||||
to include the star cluster that was birthed from it. We turned to a study of the
|
||||
Path = "/Milky Way/Orion",
|
||||
Description = [[ In order to have an accurate depiction of the Orion nebula, we
|
||||
need to include the star cluster that was birthed from it. We turned to a study of the
|
||||
cluster's stellar population by Lynne Hillenbrand, who was working at the University of
|
||||
California, Berkeley at the time. The catalog from her paper contains more than 1500
|
||||
stars, about half the stars in the actual cluster. The cluster is very crowded, with a
|
||||
@@ -45,7 +36,18 @@ Knowing the size of the cluster and approximating the shape to be roughly spheri
|
||||
placed each star along a line of sight through this imaginary sphere centered on the
|
||||
cluster. In this sense, these data are observed data and the view from Earth is accurate.
|
||||
But the distance of each star has been derived from this educated-guess approach for the
|
||||
cluster distribution. ]],
|
||||
cluster distribution. ]]
|
||||
}
|
||||
}
|
||||
|
||||
assetHelper.registerSceneGraphNodesAndExport(asset, { OrionClusterStars })
|
||||
|
||||
|
||||
asset.meta = {
|
||||
Name = "Orion Nebula Star Cluster",
|
||||
Version = "1.0",
|
||||
Description = [[ Digital Universe asset for the Orion star cluster. To be used in
|
||||
conjunction with nebula model. Use orionnebula.asset to include both.]],
|
||||
Author = "AMNH Digital Universe",
|
||||
URL = "https://www.amnh.org/research/hayden-planetarium/digital-universe",
|
||||
License = "AMNH Digital Universe",
|
||||
|
||||
@@ -31,7 +31,20 @@ local NebulaHolder = {
|
||||
},
|
||||
GUI = {
|
||||
Name = "Orion Nebula",
|
||||
Path = "/Milky Way/Objects",
|
||||
Path = "/Milky Way/Orion",
|
||||
Description = [[ In the Digital Universe model of the Orion Nebula, we depict the
|
||||
ionization front effectively as a terrain, with a flat Hubble image of the nebula mapped
|
||||
on the undulating surface. In reality, the ionization front has a slight thickness to
|
||||
it - about a third of a light year - but is quite thin compared to the overall size of
|
||||
the nebula, which stretches about ten light years from side to side.<br><br>Close into
|
||||
the center, we see small teardrop-shaped structures with their narrow ends pointing away
|
||||
from the bright star: these are protoplanetary disks, or proplyds, of dense gas and dust
|
||||
surrounding young stars. The larger formations that one sees farther away from the center
|
||||
of the nebula take on a cup-like shape, with the narrow end pointing away from the
|
||||
nebulas center. These enormous structures are bow shocks that delineate the region where
|
||||
highspeed winds from the central star slow from supersonic to subsonic speeds. You can
|
||||
think of an HII region as a sort of tremendous explosion, taking place over millennia,
|
||||
and the bow shocks are part of the outward rush of material. ]]
|
||||
}
|
||||
}
|
||||
|
||||
@@ -62,8 +75,9 @@ local OrionNebulaModel = {
|
||||
},
|
||||
GUI = {
|
||||
Name = "Orion Nebula Model",
|
||||
Path = "/Milky Way/Objects",
|
||||
Hidden = true
|
||||
Path = "/Milky Way/Orion",
|
||||
Hidden = true,
|
||||
Description = "Orion Nebula 3D model. See Orion Nebula for description."
|
||||
}
|
||||
}
|
||||
|
||||
@@ -94,8 +108,9 @@ local OrionNebulaShocksModel = {
|
||||
},
|
||||
GUI = {
|
||||
Name = "Orion Nebula Shocks",
|
||||
Path = "/Milky Way/Objects",
|
||||
Hidden = false
|
||||
Path = "/Milky Way/Orion",
|
||||
Hidden = false,
|
||||
Description = "Orion Nebula Shocks 3D model. See Orion Nebula for description."
|
||||
}
|
||||
}
|
||||
|
||||
@@ -126,8 +141,9 @@ local OrionNebulaProplydsModel = {
|
||||
},
|
||||
GUI = {
|
||||
Name = "Orion Nebula Proplyds",
|
||||
Path = "/Milky Way/Objects",
|
||||
Hidden = false
|
||||
Path = "/Milky Way/Orion",
|
||||
Hidden = false,
|
||||
Description = "Orion Nebula Proplyds 3D model. See Orion Nebula for description."
|
||||
}
|
||||
}
|
||||
|
||||
@@ -142,22 +158,12 @@ assetHelper.registerSceneGraphNodesAndExport(asset, {
|
||||
asset.meta = {
|
||||
Name = "Orion Nebula Model",
|
||||
Version = "1.0",
|
||||
Description = [[ In the Digital Universe model of the Orion Nebula, we depict the
|
||||
ionization front effectively as a terrain, with a flat Hubble image of the nebula mapped
|
||||
on the undulating surface. In reality, the ionization front has a slight thickness to
|
||||
it - about a third of a light year - but is quite thin compared to the overall size of
|
||||
the nebula, which stretches about ten light years from side to side.<br><br>Close into
|
||||
the center, we see small teardrop-shaped structures with their narrow ends pointing away
|
||||
from the bright star: these are protoplanetary disks, or proplyds, of dense gas and dust
|
||||
surrounding young stars. The larger formations that one sees farther away from the center
|
||||
of the nebula take on a cup-like shape, with the narrow end pointing away from the
|
||||
nebulas center. These enormous structures are bow shocks that delineate the region where
|
||||
highspeed winds from the central star slow from supersonic to subsonic speeds. You can
|
||||
think of an HII region as a sort of tremendous explosion, taking place over millennia,
|
||||
and the bow shocks are part of the outward rush of material. ]],
|
||||
Description = [[ Digital Universe asset for the Orion nebula 3D model. This asset
|
||||
contains seperate models for the nebula, proplyds and shocks. To be used in
|
||||
conjunction with orion star cluster. Use orionnebula.asset to include both.]],
|
||||
Author = "AMNH Digital Universe",
|
||||
URL = "https://www.amnh.org/research/hayden-planetarium/digital-universe",
|
||||
License = "AMNH Digital Universe",
|
||||
Identifiers = {"OrionNebulaModel", "OrionNebulaModel", "OrionNebulaProplydsModel",
|
||||
Identifiers = {"OrionNebulaHolder", "OrionNebulaModel", "OrionNebulaProplydsModel",
|
||||
"OrionNebulaShocksModel"}
|
||||
}
|
||||
|
||||
@@ -18,8 +18,9 @@ local NebulaPosition = {
|
||||
},
|
||||
GUI = {
|
||||
Name = "Orion Nebula Position",
|
||||
Path = "/Milky Way/Objects",
|
||||
Hidden = true
|
||||
Path = "/Milky Way/Orion",
|
||||
Hidden = true,
|
||||
Description = "Static position for Orion Nebula"
|
||||
}
|
||||
}
|
||||
|
||||
|
||||
Reference in New Issue
Block a user