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Update Digital Universe catalogue (#2729)
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@@ -30,11 +30,11 @@ asset.require("scene/digitaluniverse/constellations")
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asset.require("scene/digitaluniverse/deepsky")
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asset.require("scene/digitaluniverse/dwarfs")
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asset.require("scene/digitaluniverse/exoplanets")
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asset.require("scene/digitaluniverse/exoplanets_candidates")
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asset.require("scene/digitaluniverse/globularclusters")
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asset.require("scene/digitaluniverse/grids")
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asset.require("scene/digitaluniverse/groups")
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asset.require("scene/digitaluniverse/h2regions")
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asset.require("scene/digitaluniverse/kepler")
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asset.require("scene/digitaluniverse/localdwarfs")
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asset.require("scene/digitaluniverse/milkyway")
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asset.require("scene/digitaluniverse/milkyway_arm_labels")
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@@ -2,7 +2,7 @@ local speck = asset.syncedResource({
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Name = "Alternate Star Labels Speck Files",
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Type = "HttpSynchronization",
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Identifier = "digitaluniverse_alternatestarlabels_speck",
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Version = 1
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Version = 2
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})
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@@ -13,7 +13,7 @@ local Object = {
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Enabled = false,
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Labels = {
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Enabled = true,
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File = speck .. "stars-altlbl.label",
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File = speck .. "altstarlabels.label",
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Color = { 0.4, 0.4, 0.4 },
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Size = 14.7,
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MinMaxSize = { 6, 20 },
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@@ -26,13 +26,13 @@ local Object = {
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GUI = {
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Name = "Stars Labels - Alternate",
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Path = "/Milky Way/Stars",
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Description = [[Census 3,550 star names. DU Version 1.7. <br>The main star data
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identify the accepted IAU star names for the brightest stars. However, astronomers
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have long cataloged thousands of stars beyond the brightest ones we see. Several
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attempts over thousands of years to name all the visible stars have led to two
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main catalogs: Johann Bayer's Catalog from 1603 and John Flamsteed's Catalog
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published in 1725. (Description from URL) <br><br> Data Reference: Various
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sources]]
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Description = [[Census 3,395 star names. DU Version 1.8. <br>The main star data
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identify the accepted IAU star names for the brightest stars. However, astronomers
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have long cataloged thousands of stars beyond the brightest ones we see. Several
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attempts over thousands of years to name all the visible stars have led to two
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main catalogs: Johann Bayer's Catalog from 1603 and John Flamsteed's Catalog
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published in 1725. (Description from URL) <br><br> Data Reference: Various
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sources]]
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}
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}
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@@ -6,7 +6,7 @@ local speck = asset.syncedResource({
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Name = "Constellation Files",
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Type = "HttpSynchronization",
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Identifier = "digitaluniverse_constellations_data",
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Version = 1
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Version = 2
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})
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@@ -85,7 +85,7 @@ local Constellations = {
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GUI = {
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Name = "Constellations",
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Path = "/Milky Way/Constellations",
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Description = [[Census 88 constellations and labels. DU Version 2.3. <br> These
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Description = [[Census 88 constellations and labels. DU Version 3.4. <br> These
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modern constellations are largely based on those of the Babylonians and
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Greeks; however, most cultures have their own figures and stories of the sky.
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More than half the official constellations adopted by scientists in 1930 were
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@@ -11,11 +11,11 @@ asset.require("./constellations")
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asset.require("./deepsky")
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asset.require("./dwarfs")
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asset.require("./exoplanets")
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asset.require("./exoplanets_candidates")
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asset.require("./globularclusters")
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asset.require("./grids")
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asset.require("./groups")
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asset.require("./h2regions")
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asset.require("./kepler")
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asset.require("./localdwarfs")
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asset.require("./milkyway")
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asset.require("./milkyway_arm_labels")
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@@ -9,7 +9,7 @@ local speck = asset.syncedResource({
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Name = "Exoplanets Speck Files",
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Type = "HttpSynchronization",
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Identifier = "digitaluniverse_exoplanets_speck",
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Version = 2
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Version = 3
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})
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@@ -39,7 +39,7 @@ local Object = {
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GUI = {
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Name = "Exoplanets",
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Path = "/Milky Way/Exoplanets",
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Description = [[Census: 4,055 planets in 3,023 systems. DU Version 20.11. <br>
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Description = [[Census: 5,361 planets in 3,982 systems. DU Version 20.12. <br>
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Extrasolar planets, or exoplanets, are a relatively new phenomenon in
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astronomy. While many astronomers believed in their existence, no
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observational evidence was available until 1995. Since that time, scientists
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@@ -0,0 +1,68 @@
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local textures = asset.syncedResource({
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Name = "Exoplanets Candidates Textures",
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Type = "HttpSynchronization",
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Identifier = "digitaluniverse_exoplanets_candidates_textures",
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Version = 1
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})
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local speck = asset.syncedResource({
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Name = "Exoplanets Candidates Speck Files",
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Type = "HttpSynchronization",
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Identifier = "digitaluniverse_exoplanets_candidates_speck",
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Version = 1
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})
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local Object = {
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Identifier = "PlanetaryCandidates",
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Renderable = {
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Type = "RenderableBillboardsCloud",
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Enabled = false,
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Color = { 1.0, 1.0, 0.0 },
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Opacity = 0.99,
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ScaleFactor = 410.0,
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File = speck .. "exoplanet_candidates.speck",
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Unit = "pc",
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Texture = textures .. "halo.png",
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CorrectionSizeEndDistance = 15.86,
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CorrectionSizeFactor = 8.59,
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BillboardMinMaxSize = { 0.0, 30.0 },
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EnablePixelSizeControl = true
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},
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GUI = {
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Name = "Planetary Candidates",
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Path = "/Milky Way/Exoplanets",
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Description = [[Census: 6,082 stars with candidate planetary systems. DU Version 11.8.
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<br> The exoplanet candidate stars are likely hosts for exoplanets. These are stars
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plucked from NASA's Kepler and TESS space telescopes. The Kepler mission was
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designed to stare at one spot, roughly twelve degrees across, in the constellation
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Cygnus. By staring at one spot, the spacecraft could monitor over 500,000 stars in
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that field for subtle variations in brightness. The data included here are the stars
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that are considered good candidates to host planets. Rather than represent them
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photo-realistically, with accurate colors, we choose to visualize them as generic,
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pure yellow stars. (Description from URL) <br><br> Data Reference: NASA Exoplanet
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Archive (CalTech/NASA)]]
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}
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}
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asset.onInitialize(function()
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openspace.addSceneGraphNode(Object)
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end)
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asset.onDeinitialize(function()
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openspace.removeSceneGraphNode(Object)
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end)
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asset.export(Object)
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asset.meta = {
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Name = "Planetary Candidates",
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Version = "2.1",
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Description = "Digital Universe asset for Planetary Candidates",
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Author = "Brian Abbott, Emily Rice, and Jason No (AMNH)",
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URL = "https://www.amnh.org/research/hayden-planetarium/digital-universe",
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License = "AMNH Digital Universe"
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}
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@@ -1,68 +0,0 @@
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local textures = asset.syncedResource({
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Name = "Kepler Textures",
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Type = "HttpSynchronization",
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Identifier = "digitaluniverse_kepler_textures",
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Version = 1
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})
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local speck = asset.syncedResource({
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Name = "Kepler Speck Files",
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Type = "HttpSynchronization",
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Identifier = "digitaluniverse_kepler_speck",
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Version = 3
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})
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local Object = {
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Identifier = "KeplerPlanetaryCandidates",
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Renderable = {
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Type = "RenderableBillboardsCloud",
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Enabled = false,
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Color = { 1.0, 1.0, 0.0 },
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Opacity = 0.99,
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ScaleFactor = 410.0,
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File = speck .. "kepler.speck",
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Unit = "pc",
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Texture = textures .. "halo.png",
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CorrectionSizeEndDistance = 15.86,
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CorrectionSizeFactor = 8.59,
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BillboardMinMaxSize = { 0.0, 30.0 },
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EnablePixelSizeControl = true
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},
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GUI = {
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Name = "Kepler Planetary Candidates",
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Path = "/Milky Way/Exoplanets",
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Description = [[Census: 3,254 stars. DU Version 9.3. <br> The exoplanet candidate
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stars are likely hosts for exoplanets. These are stars plucked from NASA's Kepler
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and TESS space telescopes. The Kepler mission was designed to stare at one spot,
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roughly twelve degrees across, in the constellation Cygnus. By staring at one
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spot, the spacecraft could monitor over 500,000 stars in that field for subtle
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variations in brightness.The data included here are the stars that are considered
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good candidates to host planets. Rather than represent them photo-realistically,
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with accurate colors, we choose to visualize them as generic, pure yellow stars.
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(Description from URL) <br><br> Data Reference: NASA Exoplanet Archive
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(CalTech/NASA)]]
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}
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}
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asset.onInitialize(function()
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openspace.addSceneGraphNode(Object)
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end)
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asset.onDeinitialize(function()
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openspace.removeSceneGraphNode(Object)
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end)
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asset.export(Object)
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asset.meta = {
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Name = "Kepler Planetary Candidates",
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Version = "2.1",
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Description = "Digital Universe asset for Kepler Planetary Candidates",
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Author = "Brian Abbott, Emily Rice, and Jason No (AMNH)",
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URL = "https://www.amnh.org/research/hayden-planetarium/digital-universe",
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License = "AMNH Digital Universe"
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}
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@@ -9,7 +9,7 @@ local speck = asset.syncedResource({
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Name = "Open Clusters Speck Files",
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Type = "HttpSynchronization",
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Identifier = "digitaluniverse_openclusters_speck",
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Version = 2
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Version = 3
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})
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@@ -38,7 +38,7 @@ local Object = {
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GUI = {
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Name = "Open Star Clusters",
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Path = "/Milky Way",
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Description = [[Census: 2,040 clusters. DU Version 5.7. <br> An open star cluster is a
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Description = [[Census: 1,867 clusters. DU Version 7.8. <br> An open star cluster is a
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loose assemblage of stars numbering from hundreds to thousands that are bound by
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their mutual gravitation. Astronomers know from their stellar spectra that stars in
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open clusters are typically young. (With a star's spectrum, we can determine the
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@@ -49,7 +49,7 @@ local Object = {
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night sky. Because of this, open clusters were originally known as Galactic
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clusters, but this term fell out of favor once astronomers began to understand that
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the Galaxy includes objects beyond the Milky Way's disk. <br><br> Data Reference:
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Optically visible open clusters and Candidates (Dias+ 2002-2015)]]
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Galactic spiral structure revealed by Gaia EDR3 (Poggio+, 2021)]]
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}
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}
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@@ -2,7 +2,7 @@ local speck = asset.syncedResource({
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Name = "Stars Speck Files",
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Type = "HttpSynchronization",
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Identifier = "stars_du",
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Version = 4
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Version = 5
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})
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local sunspeck = asset.syncedResource({
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@@ -55,13 +55,13 @@ local Stars = {
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GUI = {
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Name = "Stars",
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Path = "/Milky Way/Stars",
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Description = [[Census: 117,003 stars with 321 labels.<br> DU Version 7.8. This
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Description = [[Census: 116,584 stars with 321 labels.<br> DU Version 8.10. This
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star catalog is a combination of all available star catalogs, wherein we
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choose the best distance available to place the stars around the Sun as
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accurately as is possible. (Description from URL) <br><br> Data Reference:
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XHIP: An Extended Hipparcos Compilation (Anderson E., Francis C. 2012);
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Hipparcos Catalog (European Space Agency 1997); Gliese Catalog (Gliese and
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Jahriess 1991)]]
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Gaia Data Release 3 (Gaia Collaboration, 2022); XHIP: An Extended Hipparcos
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Compilation (Anderson E., Francis C. 2012); Hipparcos Catalog (European Space Agency
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1997); Gliese Catalog (Gliese and Jahriess 1991)]]
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}
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}
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