From 323416b99a37faef9249a0193e4e7b7341a20e39 Mon Sep 17 00:00:00 2001 From: Micah Date: Thu, 1 Oct 2020 17:56:12 -0400 Subject: [PATCH] du asset meta update --- data/assets/scene/digitaluniverse/2dF.asset | 35 ++++--- data/assets/scene/digitaluniverse/2mass.asset | 14 +-- data/assets/scene/digitaluniverse/6dF.asset | 28 +++--- data/assets/scene/digitaluniverse/abell.asset | 32 +++--- .../digitaluniverse/alternatestarlabels.asset | 11 ++- .../digitaluniverse/backgroundradiation.asset | 15 +++ .../scene/digitaluniverse/clusters.asset | 13 +++ .../digitaluniverse/constellationbounds.asset | 11 +++ .../digitaluniverse/constellations.asset | 17 ++++ .../scene/digitaluniverse/deepsky.asset | 19 ++++ .../assets/scene/digitaluniverse/dwarfs.asset | 22 ++++- .../scene/digitaluniverse/exoplanets.asset | 15 +++ .../digitaluniverse/globularclusters.asset | 20 ++++ data/assets/scene/digitaluniverse/grids.asset | 16 +++ .../assets/scene/digitaluniverse/groups.asset | 13 +++ .../scene/digitaluniverse/h2regions.asset | 19 ++++ .../assets/scene/digitaluniverse/kepler.asset | 19 ++++ .../scene/digitaluniverse/localdwarfs.asset | 19 ++++ .../scene/digitaluniverse/milkyway.asset | 98 ++++--------------- .../digitaluniverse/milkyway_arm_labels.asset | 34 +++++-- .../digitaluniverse/milkyway_label.asset | 56 +++++++++++ .../digitaluniverse/milkyway_sphere.asset | 51 ++++++++++ .../digitaluniverse/obassociations.asset | 19 ++++ .../scene/digitaluniverse/openclusters.asset | 20 ++++ .../digitaluniverse/planetarynebulae.asset | 16 +++ .../scene/digitaluniverse/pulsars.asset | 22 +++++ .../scene/digitaluniverse/quasars.asset | 17 ++++ data/assets/scene/digitaluniverse/sdss.asset | 24 +++++ .../scene/digitaluniverse/starlabels.asset | 10 ++ .../scene/digitaluniverse/starorbits.asset | 13 +++ data/assets/scene/digitaluniverse/stars.asset | 15 +++ .../scene/digitaluniverse/superclusters.asset | 15 +++ .../digitaluniverse/supernovaremnants.asset | 13 +++ data/assets/scene/digitaluniverse/tully.asset | 33 +++++++ data/assets/scene/digitaluniverse/voids.asset | 19 ++++ .../pluto/charon/default_layers.asset | 2 +- .../dwarf_planets/pluto/default_layers.asset | 2 +- .../solarsystem/planets/mercury/trail.asset | 2 +- .../planets/venus/trail_earth.asset | 7 +- data/web/documentation/scenelicense.hbs | 4 +- data/web/documentation/script.js | 4 + 41 files changed, 681 insertions(+), 153 deletions(-) create mode 100644 data/assets/scene/digitaluniverse/milkyway_label.asset create mode 100644 data/assets/scene/digitaluniverse/milkyway_sphere.asset diff --git a/data/assets/scene/digitaluniverse/2dF.asset b/data/assets/scene/digitaluniverse/2dF.asset index 56941b50c5..b352d38854 100644 --- a/data/assets/scene/digitaluniverse/2dF.asset +++ b/data/assets/scene/digitaluniverse/2dF.asset @@ -39,25 +39,28 @@ local object = { } } + +assetHelper.registerSceneGraphNodesAndExport(asset, { object }) + + asset.meta = { Name = "2dF Galaxies", Version = "2.0", - Description = [[ The Two-degree Field (2dF) Survey was a project designed - to map portions of the extragalactic universe. The 2dF instrument was - mounted on the 3.9-meter (12.8-foot) Anglo-Australian Telescope (AAT), - located 450 km (280 miles) northwest of Sydney. The telescope has a - two-degree field of view on the sky, enabling large parts of the sky to - be observed at one time. For each pointing of the telescope, the - instrument can acquire up to 400 spectra simultaneously via optical - fibers that feed into two spectrographs. Each spectrograph sees light - that is between 350 nm and 800 nm, spanning the visible spectrum. -

The 2dF survey has three main components: the North Galactic - Pole strip, the South Galactic Pole strip, and the random fields that - surround the South Galactic Pole strip. The galaxy survey is composed - of about 230,000 galaxies with brightness and redshift measurements. ]], - Author = "AMNH Digital Universe", + Description = [[Census 229,293 galaxies. DU Version 1.7. The Two-degree Field (2dF) + Survey was a project designed to map portions of the extragalactic universe. The + 2dF instrument was mounted on the 3.9-meter (12.8-foot) Anglo-Australian Telescope + (AAT), located 450 km (280 miles) northwest of Sydney. The telescope has a + two-degree field of view on the sky, enabling large parts of the sky to be + observed at one time. For each pointing of the telescope, the instrument can + acquire up to 400 spectra simultaneously via optical fibers that feed into two + spectrographs. Each spectrograph sees light that is between 350 nm and 800 nm, + spanning the visible spectrum.

The 2dF survey has three main components: + the North Galactic Pole strip, the South Galactic Pole strip, and the random + fields that surround the South Galactic Pole strip. The galaxy survey is composed + of about 230,000 galaxies with brightness and redshift measurements. (Description + from URL)

Data Reference: 2dF Galaxy Redshift Survey (2dFGRS Team, + 1998-2003)]], + Author = "Brian Abbott (AMNH), Eric Gawiser (Rutgers U)", URL = "https://www.amnh.org/research/hayden-planetarium/digital-universe", License = "AMNH Digital Universe" } - -assetHelper.registerSceneGraphNodesAndExport(asset, { object }) diff --git a/data/assets/scene/digitaluniverse/2mass.asset b/data/assets/scene/digitaluniverse/2mass.asset index c55ea083a0..508070b3af 100644 --- a/data/assets/scene/digitaluniverse/2mass.asset +++ b/data/assets/scene/digitaluniverse/2mass.asset @@ -41,6 +41,10 @@ local object = { } } + +assetHelper.registerSceneGraphNodesAndExport(asset, { object }) + + asset.meta = { Name = "2MASS Galaxies", Version = "1.0", @@ -50,10 +54,8 @@ asset.meta = { from this survey is starlight. In visible light, clouds of gas and dust obscure our view. However, in infrared, the longer wavelengths of light can penetrate these clouds without being scattered, thereby revealing stars - that would normally be hidden to our eye. ]], - Author = "AMNH Digital Universe", + that would normally be hidden to our eye. (Description from URL)]], + Author = "Brian Abbott (AMNH)", URL = "https://www.amnh.org/research/hayden-planetarium/digital-universe", - License = "custom" -} - -assetHelper.registerSceneGraphNodesAndExport(asset, { object }) + License = "AMNH Digital Universe" +} \ No newline at end of file diff --git a/data/assets/scene/digitaluniverse/6dF.asset b/data/assets/scene/digitaluniverse/6dF.asset index bbf1c4f7b3..c4f7c35b3f 100644 --- a/data/assets/scene/digitaluniverse/6dF.asset +++ b/data/assets/scene/digitaluniverse/6dF.asset @@ -39,21 +39,23 @@ local object = { } } + +assetHelper.registerSceneGraphNodesAndExport(asset, { object }) + + asset.meta = { Name = "6dF Galaxies", Version = "2.0", - Description = [[ The Six-degree Field (6dF) Galaxy Survey mapped nearly half - the sky from the Anglo-Australian Observatory. Unlike previous datasets, - this one is not all-sky, meaning there are patches of sky that are not - covered. In this case, the entire northern hemisphere has no coverage - at all. This catalog overlaps with the Tully dataset, and there is a - noticeable difference in the quality of these datasets. Tully is much - tighter and the structure is more apparent, while the 6dF data are more - spread out. This is because of local motions within galaxy clusters have - not been corrected in these data. ]], - Author = "AMNH Digital Universe", + Description = [[Census 109,569 galaxies. DU Version 1.4. The Six-degree Field (6dF) + Galaxy Survey mapped nearly half the sky from the Anglo-Australian Observatory. Unlike + previous datasets, this one is not all-sky, meaning there are patches of sky that are + not covered. In this case, the entire northern hemisphere has no coverage at all. This + catalog overlaps with the Tully dataset, and there is a noticeable difference in the + quality of these datasets. Tully is much tighter and the structure is more apparent, + while the 6dF data are more spread out. This is because of local motions within galaxy + clusters have not been corrected in these data. (Description from URL)

data + Reference: The 6dF Galaxy Survey Redshift Catalogue (Jones+, 2009)]], + Author = "Brian Abbott (AMNH)", URL = "https://www.amnh.org/research/hayden-planetarium/digital-universe", - License = "custom" + License = "AMNH Digital Universe" } - -assetHelper.registerSceneGraphNodesAndExport(asset, { object }) diff --git a/data/assets/scene/digitaluniverse/abell.asset b/data/assets/scene/digitaluniverse/abell.asset index fc1c90d8cf..8fcd3ae5d6 100644 --- a/data/assets/scene/digitaluniverse/abell.asset +++ b/data/assets/scene/digitaluniverse/abell.asset @@ -47,23 +47,25 @@ local object = { } } + +assetHelper.registerSceneGraphNodesAndExport(asset, { object }) + + asset.meta = { Name = "Abell Galaxy Clusters", Version = "2.0", - Description = [[The Abell catalog includes all the nearby, and not so - nearby, galaxy clusters. The northern hemisphere survey, published in - 1958, was compiled by George Abell (1927 - 1983) from the Palomar Sky - Survey plates. A subsequent southern hemisphere catalog was published - posthumously in 1989. Further analysis by Brent Tully determined their - distance and three-dimensional distribution.

Each point in this - data set represents a cluster of tens to hundreds (possibly even - thousands) of galaxies, similar to the Virgo or Fornax Clusters. - You will notice some points are assigned colors while most are gray. - The data set also has an arbitrary cut-off for completeness, resulting - in the rectangular shape of the data set.]], - Author = "AMNH Digital Universe", + Description = [[Census 2,246 galaxies. DU Version 1.4. The Abell catalog includes all + the nearby, and not so nearby, galaxy clusters. The northern hemisphere survey, + published in 1958, was compiled by George Abell (1927–1983) from the Palomar Sky + Survey plates. A subsequent southern hemisphere catalog was published posthumously in + 1989. Further analysis by Brent Tully determined their distance and three-dimensional + distribution. Each point in this data set represents a cluster of tens to hundreds + (possibly even thousands) of galaxies, similar to the Virgo or Fornax Clusters. You + will notice some points are assigned colors while most are gray. The data set also has + an arbitrary cut-off for completeness, resulting in the rectangular shape of the data + set. (Description from URL)

Data Reference: Abell Clusters of Rich Galaxies, + Brent Tully (U Hawaii), Stuart Levy (NCSA/UIUC)]], + Author = "Stuart Levy (NCSA/UIUC), Brian Abbott (AMNH)", URL = "https://www.amnh.org/research/hayden-planetarium/digital-universe", - License = "custom" + License = "AMNH Digital Universe" } - -assetHelper.registerSceneGraphNodesAndExport(asset, { object }) diff --git a/data/assets/scene/digitaluniverse/alternatestarlabels.asset b/data/assets/scene/digitaluniverse/alternatestarlabels.asset index 272ca87615..e1ad7853f0 100644 --- a/data/assets/scene/digitaluniverse/alternatestarlabels.asset +++ b/data/assets/scene/digitaluniverse/alternatestarlabels.asset @@ -32,11 +32,12 @@ local object = { asset.meta = { Name = "Stars Labels - Alternate", Version = "1.0", - Description = [[The main star data identify the accepted IAU star names for - the brightest stars. However, astronomers have long cataloged thousands of - stars beyond the brightest ones we see. Several attempts over thousands of - years to name all the visible stars have led to two main catalogs: Johann - Bayer's Catalog from 1603 and John Flamsteed's Catalog published in 1725.]], + Description = [[Census 3,550 star names. DU Version 1.7. The main star data identify + the accepted IAU star names for the brightest stars. However, astronomers have long + cataloged thousands of stars beyond the brightest ones we see. Several attempts over + thousands of years to name all the visible stars have led to two main catalogs: Johann + Bayer's Catalog from 1603 and John Flamsteed's Catalog published in 1725. (Description + from URL)

Data Reference: Various sources]], Author = "Brian Abbott (AMNH)", URL = "https://www.amnh.org/research/hayden-planetarium/digital-universe", License = "AMNH Digital Universe" diff --git a/data/assets/scene/digitaluniverse/backgroundradiation.asset b/data/assets/scene/digitaluniverse/backgroundradiation.asset index 66a2c70a46..ec87c3544e 100644 --- a/data/assets/scene/digitaluniverse/backgroundradiation.asset +++ b/data/assets/scene/digitaluniverse/backgroundradiation.asset @@ -89,6 +89,7 @@ local planck = { FadeInThreshold = 0.4 }, GUI = { + Name = "Planck", Path = "/Universe/Cosmic Microwave Background" } } @@ -246,3 +247,17 @@ assetHelper.registerSceneGraphNodesAndExport(asset, { wmap, cbe, planck, multiverse_planck_1, multiverse_planck_2, multiverse_planck_3, multiverse_planck_4, Halpha }) + + +asset.meta = { + Name = "Background Radiation", + Version = "2.0", + Description = [[Various AllSky images for the Milky Way and observable Universe. + Included: Wilkinson Microwave Anisotropy Probe (WMAP), Cosmic Background Explorer, + Planck, Planck Multiverse 1-4, and H Alpha

Data Reference: Planck/ESA and + the Planck Collaboration, Wilkinson Microwave Anisotropy Probe/NASA, Doug + Finkbeiner (Princeton)]], + Author = "Brian Abbott (AMNH), OpenSpace Team", + URL = "https://www.amnh.org/research/hayden-planetarium/digital-universe", + License = "AMNH Digital Universe" +} diff --git a/data/assets/scene/digitaluniverse/clusters.asset b/data/assets/scene/digitaluniverse/clusters.asset index 3f0475d98b..c690c4ac84 100644 --- a/data/assets/scene/digitaluniverse/clusters.asset +++ b/data/assets/scene/digitaluniverse/clusters.asset @@ -38,3 +38,16 @@ local object = { assetHelper.registerSceneGraphNodesAndExport(asset, { object }) + + +asset.meta = { + Name = "Stars Labels - Alternate", + Version = "1.0", + Description = [[Census 15 galaxy cluster labels. DU Version 1.2. The Galaxy Clusters + dataset is a series of labels that mark where the large clusters of galaxies are in + the nearby universe. These labels must be used in conjunction with the Tully galaxy + group.(Description from URL)

Data Reference: Brian Abbott (AMNH)]], + Author = "Brian Abbott (AMNH)", + URL = "https://www.amnh.org/research/hayden-planetarium/digital-universe", + License = "AMNH Digital Universe" +} diff --git a/data/assets/scene/digitaluniverse/constellationbounds.asset b/data/assets/scene/digitaluniverse/constellationbounds.asset index 35dd792e2c..4323b87180 100644 --- a/data/assets/scene/digitaluniverse/constellationbounds.asset +++ b/data/assets/scene/digitaluniverse/constellationbounds.asset @@ -43,3 +43,14 @@ local object = { assetHelper.registerSceneGraphNodesAndExport(asset, { object }) + + +asset.meta = { + Name = "Constellation Bounds", + Version = "1.0", + Description = [[A Spherical mesh dividing the sky into regions that fit the + constellations.]], + Author = "Brian Abbott (AMNH)", + URL = "https://www.amnh.org/research/hayden-planetarium/digital-universe", + License = "AMNH Digital Universe" +} diff --git a/data/assets/scene/digitaluniverse/constellations.asset b/data/assets/scene/digitaluniverse/constellations.asset index 216a320283..4dd1bc2783 100644 --- a/data/assets/scene/digitaluniverse/constellations.asset +++ b/data/assets/scene/digitaluniverse/constellations.asset @@ -55,3 +55,20 @@ local constellations = { assetHelper.registerSceneGraphNodesAndExport(asset, { constellationsExtragalactic, constellations }) + + +asset.meta = { + Name = "Constellations", + Version = "1.0", + Description = [[Census 88 constellations and labels. DU Version 2.3. These modern + constellations are largely based on those of the Babylonians and Greeks; however, most + cultures have their own figures and stories of the sky. More than half the official + constellations adopted by scientists in 1930 were known to the ancients over 2,000 + years ago. Each star falls into one of these 88 regions. Of course, today we know the + stars in any given constellation do not necessarily have any physical relationship + with one another. One star may be nearby, while an adjacent star in the sky may be + far away.(Description from URL)

Data Reference: various]], + Author = "Brian Abbott (AMNH)", + URL = "https://www.amnh.org/research/hayden-planetarium/digital-universe", + License = "AMNH Digital Universe" +} diff --git a/data/assets/scene/digitaluniverse/deepsky.asset b/data/assets/scene/digitaluniverse/deepsky.asset index 4789551408..766b04aa4a 100644 --- a/data/assets/scene/digitaluniverse/deepsky.asset +++ b/data/assets/scene/digitaluniverse/deepsky.asset @@ -85,3 +85,22 @@ local deepSkyImages = { } assetHelper.registerSceneGraphNodesAndExport(asset, { deepSkyPoints, deepSkyImages }) + + +asset.meta = { + Name = "Deep Sky Objects Images", + Version = "1.0", + Description = [[Census: 63 images and labels. DU Version 1.3. These data are 2-D + images of Messier objects placed in 3-D space. Not only do we place these images at + the proper location and give them the correct orientation, we also size them + accurately so that you can fly to the globular cluster M13, for example, and see just + how small the cluster of hundreds of thousands of stars is relative to the rest of the + Galaxy. Included Messier Objects by number are: 6, 7, 11, 16, 18, 21, 23-26, 29, 34-39 + , 41, 46-48, 50, 52, 67, 93, 103, 2-5, 9, 10, 12-15, 19, 22, 28, 30, 53-56, 68-72, 75, + 79, 80, 92, 107, 27, 57, 76, 97, 8, 17, 20, 78, 1 (Description from URL)

Data + Reference: Largely NOAO and various other sources (each image has a ref)]], + Author = "Nate Greenstein, Matt Everhart, Brian Abbott (AMNH)", + URL = "https://www.amnh.org/research/hayden-planetarium/digital-universe", + License = "AMNH Digital Universe" +} + diff --git a/data/assets/scene/digitaluniverse/dwarfs.asset b/data/assets/scene/digitaluniverse/dwarfs.asset index aa2b32effa..998f4a5bc6 100644 --- a/data/assets/scene/digitaluniverse/dwarfs.asset +++ b/data/assets/scene/digitaluniverse/dwarfs.asset @@ -49,10 +49,26 @@ local object = { assetHelper.registerSceneGraphNodesAndExport(asset, { object }) + asset.meta = { Name = "Brown Dwarfs", - Version = "5.3", - Description = [[Brown dwarf catalog, including L, T, and Y dwarfs.]], + Version = "2.0", + Description = [[Census: 785 L dwarfs, 101 T dwarfs, 17 Y dwarfs. DU Version 6.4. In + astronomy, there are dwarf stars-red, white, and brown-dwarf novae, and even dwarf + galaxies. As you might imagine, astronomers use the term dwarf when they refer to the + smaller objects in any given class. For decades it was believed that M stars were the + coolest stars in the Galaxy. Some M stars, called red dwarfs, make up 70% of the stars + in the Galaxy, including our nearest known neighbor, Proxima Centauri. However, a new + class of objects, even cooler than M stars, was recently discovered and given a + spectral type of L. L-type objects straddle the boundary between red dwarfs and brown + dwarfs, the latter of which are not massive enough to ignite the nuclear processes + necessary for it to shine as a star. L-type objects are typically very dim stars or + brown dwarfs. Even cooler than L-type objects are T-type objects. These are mostly + brown dwarfs and resemble large, massive, Jupiter-like objects, too large to be + planets and typically too small to be stars. Beyond the T dwarfs are the Y-type + objects, which are even more dim.(Description from URL)

Data Reference: The + Brown Dwarf Kinematics Project (Faherty+ 2019)]], + Author = "Brian Abbott (AMNH)", URL = "https://www.amnh.org/research/hayden-planetarium/digital-universe", - License = "custom" + License = "AMNH Digital Universe" } diff --git a/data/assets/scene/digitaluniverse/exoplanets.asset b/data/assets/scene/digitaluniverse/exoplanets.asset index c3063aa918..cb8fdd0efd 100644 --- a/data/assets/scene/digitaluniverse/exoplanets.asset +++ b/data/assets/scene/digitaluniverse/exoplanets.asset @@ -45,3 +45,18 @@ local object = { assetHelper.registerSceneGraphNodesAndExport(asset, { object }) + + +asset.meta = { + Name = "Exoplanets", + Version = "1.0", + Description = [[Census: 4,055 planets in 3,023 systems. DU Version 20.11. Extrasolar + planets, or exoplanets, are a relatively new phenomenon in astronomy. While many + astronomers believed in their existence, no observational evidence was available until + 1995. Since that time, scientists have discovered thousands of systems consisting of + one or more planets around a host star.(Description from URL)

Data Reference: + NASA Exoplanet Archive (CalTech/NASA)]], + Author = "Brian Abbott (AMNH)", + URL = "https://www.amnh.org/research/hayden-planetarium/digital-universe", + License = "AMNH Digital Universe" +} diff --git a/data/assets/scene/digitaluniverse/globularclusters.asset b/data/assets/scene/digitaluniverse/globularclusters.asset index 035052eea1..8e031c4072 100644 --- a/data/assets/scene/digitaluniverse/globularclusters.asset +++ b/data/assets/scene/digitaluniverse/globularclusters.asset @@ -45,3 +45,23 @@ local object = { assetHelper.registerSceneGraphNodesAndExport(asset, { object }) + + +asset.meta = { + Name = "Globular Clusters", + Version = "2.0", + Description = [[Census: 157 globular clusters. DU Version 2.6. Globular star clusters + are gravitationally bound groups of 100,000 to 1 million stars. They are compact, + spherical “balls” of stars with very high stellar densities in their centers (stars + near their center are within a light year of one another). These clusters are + typically 30 to 100 light years in diameter. If Earth were located inside one of these + clusters, our sky would be lit by an abundance of stars brighter than the Sun. The + globular clusters form one of the most complete data sets in the Atlas. Data for the + clusters represent almost all the clusters in our Galaxy—several on the opposite side + of Galactic center may be invisible to us. The clusters orbit the Milky Way in random + orientations, as comets orbit the Sun.(Description from URL)

Data Reference: + Properties of Galactic Globular Clusters, C. Francis+ (U Cambridge)]], + Author = "Brian Abbott (AMNH)", + URL = "https://www.amnh.org/research/hayden-planetarium/digital-universe", + License = "AMNH Digital Universe" +} diff --git a/data/assets/scene/digitaluniverse/grids.asset b/data/assets/scene/digitaluniverse/grids.asset index dcb069250a..3c1fa6ba6d 100644 --- a/data/assets/scene/digitaluniverse/grids.asset +++ b/data/assets/scene/digitaluniverse/grids.asset @@ -533,3 +533,19 @@ assetHelper.registerSceneGraphNodesAndExport(asset, { galacticLabels, plane1ld, plane1lm, plane1ly, plane10ly, plane100ly, plane1kly, plane10kly, plane100kly, plane1Mly, plane10Mly, plane100Mly, plane20Gly }) + + +asset.meta = { + Name = "Grids", + Version = "2.0", + Description = [[Various grids for showing size reference. Included: 10,000 light year + grid, 10 light year grid, 20 billion light year grid, 10 million light year grid, + 100 light year grid, 100 million light year grid, Ecliptic Coordinate Sphere + (500-light-year radius), Galactic Coordinate Sphere (1000-light-year radius), + Galaxy Coordinate Grid, Celestial Coordinates / Radio Sphere (dynamic radius), 1 + billion light year grid, Celestial Coordinate Sphere (1000000-light-year radius), + 1,000 light year grid, 1 million light year grid, 1 light year grid]], + Author = "Brian Abbott (AMNH)", + URL = "https://www.amnh.org/research/hayden-planetarium/digital-universe", + License = "AMNH Digital Universe" +} diff --git a/data/assets/scene/digitaluniverse/groups.asset b/data/assets/scene/digitaluniverse/groups.asset index 682f7fb65b..11792e5726 100644 --- a/data/assets/scene/digitaluniverse/groups.asset +++ b/data/assets/scene/digitaluniverse/groups.asset @@ -39,3 +39,16 @@ local object = { assetHelper.registerSceneGraphNodesAndExport(asset, { object }) + + +asset.meta = { + Name = "Galaxy Group Labels", + Version = "1.0", + Description = [[Census: 62 galaxy group labels. DU Version 1.2. The Galaxy Groups data + are a set of labels that mark the nearby galaxy groups. The Milky Way is in the Local + Group, and we are surrounded by many other groups.(Description from URL)

Data + Reference: Brian Abbott (AMNH)]], + Author = "Brian Abbott (AMNH)", + URL = "https://www.amnh.org/research/hayden-planetarium/digital-universe", + License = "AMNH Digital Universe" +} diff --git a/data/assets/scene/digitaluniverse/h2regions.asset b/data/assets/scene/digitaluniverse/h2regions.asset index db9cf215c6..1f74221271 100644 --- a/data/assets/scene/digitaluniverse/h2regions.asset +++ b/data/assets/scene/digitaluniverse/h2regions.asset @@ -45,3 +45,22 @@ local object = { assetHelper.registerSceneGraphNodesAndExport(asset, { object }) + + +asset.meta = { + Name = "HII Regions", + Version = "1.0", + Description = [[Census: 1,271 nebulae. DU Version 4.6. H ii (pronounced H-two) regions + are stellar nurseries for newborn stars. Stars are born from condensing clouds of + hydrogen gas. As these clouds condense, the densities become high enough to form + stars. From Earth's perspective, you'll notice that the H ii regions all lie close + to the Galactic plane. This is not an accident of nature. These star-forming + regions lie in the plane of the Galaxy because that is where star formation occurs + in spiral galaxies such as our Milky Way. Because of this, they are great tracers + of the spiral arms of the Galaxy, and were instrumental in our understanding of + the Galaxy's overall structure.(Description from URL)

Data Reference: The + WISE catalog of Galactic HII Regions (Anderson+, 2014)]], + Author = "Carter Emmart, Brian Abbott (AMNH)", + URL = "https://www.amnh.org/research/hayden-planetarium/digital-universe", + License = "AMNH Digital Universe" +} diff --git a/data/assets/scene/digitaluniverse/kepler.asset b/data/assets/scene/digitaluniverse/kepler.asset index 75e102fe89..e242c2d2a2 100644 --- a/data/assets/scene/digitaluniverse/kepler.asset +++ b/data/assets/scene/digitaluniverse/kepler.asset @@ -41,3 +41,22 @@ local object = { assetHelper.registerSceneGraphNodesAndExport(asset, { object }) + + +asset.meta = { + Name = "Kepler Planetary Candidates", + Version = "2.0", + Description = [[Census: 3,254 stars. DU Version 9.3. The exoplanet candidate stars + are likely hosts for exoplanets. These are stars plucked from NASA's Kepler and + TESS space telescopes. The Kepler mission was designed to stare at one spot, + roughly twelve degrees across, in the constellation Cygnus. By staring at one + spot, the spacecraft could monitor over 500,000 stars in that field for subtle + variations in brightness.The data included here are the stars that are considered + good candidates to host planets. Rather than represent them photo-realistically, + with accurate colors, we choose to visualize them as generic, pure yellow stars. + (Description from URL)

Data Reference: NASA Exoplanet Archive + (CalTech/NASA)]], + Author = "Brian Abbott, Emily Rice, and Jason No (AMNH)", + URL = "https://www.amnh.org/research/hayden-planetarium/digital-universe", + License = "AMNH Digital Universe" +} diff --git a/data/assets/scene/digitaluniverse/localdwarfs.asset b/data/assets/scene/digitaluniverse/localdwarfs.asset index df011129ee..a796e4523f 100644 --- a/data/assets/scene/digitaluniverse/localdwarfs.asset +++ b/data/assets/scene/digitaluniverse/localdwarfs.asset @@ -46,3 +46,22 @@ local object = { assetHelper.registerSceneGraphNodesAndExport(asset, { object }) + + +asset.meta = { + Name = "Local Group", + Version = "2.0", + Description = [[Census: 102 galaxies. DU Version 6.4. A group of galaxies is a small + number of large galaxies that are typically surrounded by a large number of small + galaxies. The Milky Way belongs to the Local Group, and is one of roughly 100 + galaxies in that group. The Milky Way, the Andromeda Galaxy (also known as Messier + 31, or M31), and the Triangulum Galaxy (M33) are three of the largest galaxies in + the Local Group. Each is a spiral galaxy containing hundreds of billions of stars. + Surrounding the Milky Way and Andromeda are a bevy of dwarf galaxies-smaller, + often irregular galaxies, that contain hundreds of millions to a few billion + stars. (Description from URL)

Data Reference: Properties of dwarf + galaxies in the Local Group (McConnachie+, 2012)]], + Author = "Brian Abbott (AMNH)", + URL = "https://www.amnh.org/research/hayden-planetarium/digital-universe", + License = "AMNH Digital Universe" +} diff --git a/data/assets/scene/digitaluniverse/milkyway.asset b/data/assets/scene/digitaluniverse/milkyway.asset index 814ce42fe2..6dcadd0dff 100644 --- a/data/assets/scene/digitaluniverse/milkyway.asset +++ b/data/assets/scene/digitaluniverse/milkyway.asset @@ -2,13 +2,6 @@ local assetHelper = asset.require('util/asset_helper') -local sphereTextures = asset.syncedResource({ - Name = "Milky Way Sphere Textures", - Type = "HttpSynchronization", - Identifier = "milkyway_textures", - Version = 2 -}) - local planeTextures = asset.syncedResource({ Name = "Milky Way Plane Textures", Type = "HttpSynchronization", @@ -23,39 +16,6 @@ local planeSpeck = asset.syncedResource({ Version = 1 }) -local homespeck = asset.syncedResource({ - Name = "Home Speck File", - Type = "HttpSynchronization", - Identifier = "digitaluniverse_home_speck", - Version = 1 -}) - -local sphere = { - Identifier = "MilkyWay", - Transform = { - Rotation = { - Type = "StaticRotation", - Rotation = {0, 0, 3.14159265359} - } - }, - Renderable = { - Type = "RenderableSphere", - Size = 9.2E21, - Segments = 40, - Opacity = 0.35, - Texture = sphereTextures .. "/DarkUniverse_mellinger_4k.jpg", - Orientation = "Inside", - UseAdditiveBlending = true, - MirrorTexture = true, - FadeOutThreshold = 0.0015, - Background = true - }, - GUI = { - Name = "Milky Way Sphere", - Path = "/Milky Way" - } -} - local plane = { Identifier = "MilkyWayGalaxyImage", Parent = "Root", @@ -69,7 +29,6 @@ local plane = { TexturePath = planeTextures, Luminosity = "size", ScaleLuminosity = 1.0, - -- Fade in value in the same unit as "Unit" FadeInDistances = { 3000.0, 50000.0 }, PlaneMinSize = 5.0, Unit = "pc" @@ -80,43 +39,22 @@ local plane = { } } -local homeLabel = { - Identifier = "HomeLabel", - Renderable = { - Type = "RenderableBillboardsCloud", - Enabled = false, - Color = { 1.0, 0.4, 0.2 }, - Opacity = 0.99, - ScaleFactor = 500.0, - --File = homespeck .. "/home.speck", - -- Texture = textures .. "/point3.png", - DrawLabels = true, - LabelFile = homespeck .. "/home.label", - TextColor = { 0.8, 0.8, 0.8 }, - TextSize = 20.50, - TextMinSize = 16.0, - TransformationMatrix = { - -0.7357425748, 0.67726129641, 0.0, 0.0, - -0.074553778365, -0.080991471307, 0.9939225904, 0.0, - 0.67314530211, 0.73127116582, 0.11008126223, 0.0, - 0.0, 0.0, 0.0, 1.0 - }, - Unit = "Mpc", - -- Fade in value in the same unit as "Unit" - FadeInDistances = { 0.05, 1.0 }, - -- Max size in pixels - BillboardMaxSize = 8.22, - BillboardMinSize = 0.0, - --CorrectionSizeEndDistance = 22.0, - --CorrectionSizeFactor = 10.45 - EnablePixelSizeControl = true - }, - GUI = { - Name = "Home Label", - Path = "/Universe/Galaxies" - } + +assetHelper.registerSceneGraphNodesAndExport(asset, { plane }) + + +asset.meta = { + Name = "MilkyWay Galaxy", + Version = "2.0", + Description = [[Census: 1 image. DU Version 2.2. The exterior view of the Milky Way is + simply a two-dimensional image. The image is that of NGC 1232, a galaxy thought to + resemble our Milky Way. The image has been properly sized and approximately + oriented to function as a placeholder, allowing one to see the context of the + Galaxy relative to other data in the atlas. The features you see in the image, of + course, do not represent our Galaxy, per se, but resemble similar features found + in our Galaxy.(Description from URL)

Data Reference: European Southern + Observatory]], + Author = "Brian Abbott, Carter Emmart (AMNH)", + URL = "https://www.amnh.org/research/hayden-planetarium/digital-universe", + License = "AMNH Digital Universe" } - - - -assetHelper.registerSceneGraphNodesAndExport(asset, { sphere, plane, homeLabel }) diff --git a/data/assets/scene/digitaluniverse/milkyway_arm_labels.asset b/data/assets/scene/digitaluniverse/milkyway_arm_labels.asset index b330400462..bab87cb461 100644 --- a/data/assets/scene/digitaluniverse/milkyway_arm_labels.asset +++ b/data/assets/scene/digitaluniverse/milkyway_arm_labels.asset @@ -32,7 +32,7 @@ local plane = { Unit = "pc" }, GUI = { - Name = "Milky Way Spiral Arm Labels", + Name = "Milky Way Arms Labels", Path = "/Universe/Galaxies" } } @@ -41,13 +41,33 @@ assetHelper.registerSceneGraphNodesAndExport(asset, { plane }) asset.meta = { - Name = "Milky Way Spiral Arm Labels", + Name = "Milky Way Arms Labels", Version = "1.0", - Description = [[ This image contains labels for the Milky Way’s spiral arms. We label - them in this manner ("hard coding" the labels into an image rather than having - native labels) so that they can retain their size, shape, and location as they - overlay the galaxy. (Description from AMNH Digital Universe)]], + Description = [[ Census: 1 image. DU Version: 1.2. This image contains labels for the + Milky Way's spiral arms. We label them in this manner ("hard coding" the labels + into an image rather than having native labels) so that they can retain their + size, shape, and location as they overlay the galaxy. (Description from Digital + Universe Data Profiles)]], Author = "Brian Abbott (AMNH)", URL = "https://www.amnh.org/research/hayden-planetarium/digital-universe", - License = "AMNH Digital Universe" + License = [[ Copyright © American Museum of Natural History. All rights reserved. +

Downloading the Atlas: AMNH offers the Atlas free of charge via our + website, http://www.haydenplanetarium.org/. The User is free to download and/or + duplicate verbatim copies of the Atlas provided this license and copyright + information accompany the Atlas.

Modifying the Atlas: The user is free to + modify the Atlas by either adding data or altering existing data, provided it is + for personal use only. Once the user modifies the Atlas, it is no longer part of + AMNH's Atlas and cannot be used publicly alongside or within the Atlas without + written permission from AMNH.

Distributing the Atlas: The user is + forbidden to distribute and use the Atlas for profit, as part of a software and/or + production system that will subsequently be redistributed, or for public + consumption (via print, electronic media, or broadcast/produced pieces) without + written permission from AMNH.

Neither the names of American Museum of + Natural History and Hayden Planetarium nor the names of their contributors may be + used to endorse or promote products derived from this Atlas without specific, + prior written permission.

The Atlas is free but is offered WITHOUT ANY + WARRANTY of any kind. We provide the Atlas as is and take no responsibility for + any damage resulting from the use of this Atlas. The entire risk as to the quality + and performance of this product is with the user.

For more information, + please visit http://www.haydenplanetarium.org/universe]] } diff --git a/data/assets/scene/digitaluniverse/milkyway_label.asset b/data/assets/scene/digitaluniverse/milkyway_label.asset new file mode 100644 index 0000000000..e40ddefab6 --- /dev/null +++ b/data/assets/scene/digitaluniverse/milkyway_label.asset @@ -0,0 +1,56 @@ +--milkyway_label.asset +local assetHelper = asset.require('util/asset_helper') + + + +local homespeck = asset.syncedResource({ + Name = "Home Speck File", + Type = "HttpSynchronization", + Identifier = "digitaluniverse_home_speck", + Version = 1 +}) + +local homeLabel = { + Identifier = "HomeLabel", + Renderable = { + Type = "RenderableBillboardsCloud", + Enabled = false, + Color = { 1.0, 0.4, 0.2 }, + Opacity = 0.99, + ScaleFactor = 500.0, + DrawLabels = true, + LabelFile = homespeck .. "/home.label", + TextColor = { 0.8, 0.8, 0.8 }, + TextSize = 20.50, + TextMinSize = 16.0, + TransformationMatrix = { + -0.7357425748, 0.67726129641, 0.0, 0.0, + -0.074553778365, -0.080991471307, 0.9939225904, 0.0, + 0.67314530211, 0.73127116582, 0.11008126223, 0.0, + 0.0, 0.0, 0.0, 1.0 + }, + Unit = "Mpc", + FadeInDistances = { 0.05, 1.0 }, + BillboardMaxSize = 8.22, + BillboardMinSize = 0.0, + EnablePixelSizeControl = true + }, + GUI = { + Name = "Home Label", + Path = "/Universe/Galaxies" + } +} + + + +assetHelper.registerSceneGraphNodesAndExport(asset, { homeLabel }) + + +asset.meta = { + Name = "Home Label", + Version = "1.0", + Description = [[Label for the Milky Way titled "Home", sided for the galactic level]], + Author = "OpenSpace Team", + URL = "http://openspaceproject.com", + License = "MIT license" +} diff --git a/data/assets/scene/digitaluniverse/milkyway_sphere.asset b/data/assets/scene/digitaluniverse/milkyway_sphere.asset new file mode 100644 index 0000000000..0fb5a085d0 --- /dev/null +++ b/data/assets/scene/digitaluniverse/milkyway_sphere.asset @@ -0,0 +1,51 @@ +local assetHelper = asset.require('util/asset_helper') + + + +local sphereTextures = asset.syncedResource({ + Name = "Milky Way Sphere Textures", + Type = "HttpSynchronization", + Identifier = "milkyway_textures", + Version = 2 +}) + + +local sphere = { + Identifier = "MilkyWay", + Transform = { + Rotation = { + Type = "StaticRotation", + Rotation = {0, 0, 3.14159265359} + } + }, + Renderable = { + Type = "RenderableSphere", + Size = 9.2E21, + Segments = 40, + Opacity = 0.35, + Texture = sphereTextures .. "/DarkUniverse_mellinger_4k.jpg", + Orientation = "Inside", + UseAdditiveBlending = true, + MirrorTexture = true, + FadeOutThreshold = 0.0015, + Background = true + }, + GUI = { + Name = "Milky Way Sphere", + Path = "/Milky Way" + } +} + + +assetHelper.registerSceneGraphNodesAndExport(asset, { sphere }) + + +asset.meta = { + Name = "Milky Way Galaxy Sphere", + Version = "2.0", + Description = [[All sky image of the Milky Way that is visible when inside. Fades out + when zooming away from the Milky Way]], + Author = "OpenSpace Team", + URL = "http://openspaceproject.com", + License = "MIT license" +} diff --git a/data/assets/scene/digitaluniverse/obassociations.asset b/data/assets/scene/digitaluniverse/obassociations.asset index ad25602989..77ed118180 100644 --- a/data/assets/scene/digitaluniverse/obassociations.asset +++ b/data/assets/scene/digitaluniverse/obassociations.asset @@ -49,3 +49,22 @@ local object = { assetHelper.registerSceneGraphNodesAndExport(asset, { object }) + + +asset.meta = { + Name = "OB Associations", + Version = "2.0", + Description = [[Census: 61 OB associations. DU Version 2.4. OB associations are young + groups of stars that were formed within a giant molecular cloud, but have + dispersed after the original gas and dust from the cloud was blown away by the + star's radiation pressure. Although an association's stars are no longer + gravitationally bound to one another, they share a common motion in space because + they were formed from the same cloud. This allows astronomers to easily determine + OB association membership stars. These objects are color coded by their spiral arm + membership. Blue associations trace the Sagittarius Arm. Purple associations are + in the local Orion Spur. Orange associations are in the Perseus Arm (Description + from URL)

Data Reference: New List of OB Associations (Melnik+)]], + Author = "Brian Abbott (AMNH)", + URL = "https://www.amnh.org/research/hayden-planetarium/digital-universe", + License = "AMNH Digital Universe" +} diff --git a/data/assets/scene/digitaluniverse/openclusters.asset b/data/assets/scene/digitaluniverse/openclusters.asset index d060f744db..9964bbbc8d 100644 --- a/data/assets/scene/digitaluniverse/openclusters.asset +++ b/data/assets/scene/digitaluniverse/openclusters.asset @@ -45,3 +45,23 @@ local object = { assetHelper.registerSceneGraphNodesAndExport(asset, { object }) + + +asset.meta = { + Name = "Open Star Clusters", + Version = "2.0", + Description = [[Census: 2,040 clusters. DU Version 5.7. OB associations are young + groups of stars that were formed within a giant molecular cloud, but have + dispersed after the original gas and dust from the cloud was blown away by the + star's radiation pressure. Although an association's stars are no longer + gravitationally bound to one another, they share a common motion in space because + they were formed from the same cloud. This allows astronomers to easily determine + OB association membership stars. These objects are color coded by their spiral arm + membership. Blue associations trace the Sagittarius Arm. Purple associations are + in the local Orion Spur. Orange associations are in the Perseus Arm (Description + from URL)

Data Reference: Optically visible open clusters and Candidates + (Dias+ 2002-2015)]], + Author = "Brian Abbott (AMNH)", + URL = "https://www.amnh.org/research/hayden-planetarium/digital-universe", + License = "AMNH Digital Universe" +} diff --git a/data/assets/scene/digitaluniverse/planetarynebulae.asset b/data/assets/scene/digitaluniverse/planetarynebulae.asset index 685cd6d21a..e0f85cc26d 100644 --- a/data/assets/scene/digitaluniverse/planetarynebulae.asset +++ b/data/assets/scene/digitaluniverse/planetarynebulae.asset @@ -45,3 +45,19 @@ local object = { assetHelper.registerSceneGraphNodesAndExport(asset, { object }) + + +asset.meta = { + Name = "Planetary Nebulae", + Version = "2.0", + Description = [[Census: 283 nebulae. DU Version 2.8. A planetary nebula is an + expanding shell of gas ejected from a star late in its life cycle. Appearing like + greenish disks to a telescopic observer, planetary nebulae received their name from + their resemblance to the gaseous planets of our solar system. In no way are they + related to planets, rather, they are products of dying stars. (Description from URL) +

Data Reference: Planetary Nebulae distances in Gaia DR2 (Kimeswenger+, 2018), + Strasbourg-ESO Catalog of Planetary Nebulae (Acker+ 1992)]], + Author = "Brian Abbott (AMNH)", + URL = "https://www.amnh.org/research/hayden-planetarium/digital-universe", + License = "AMNH Digital Universe" +} diff --git a/data/assets/scene/digitaluniverse/pulsars.asset b/data/assets/scene/digitaluniverse/pulsars.asset index bd58260f22..1728ba5dcf 100644 --- a/data/assets/scene/digitaluniverse/pulsars.asset +++ b/data/assets/scene/digitaluniverse/pulsars.asset @@ -37,6 +37,7 @@ local object = { EnablePixelSizeControl = false }, GUI = { + Name = "Pulsars", Path = "/Milky Way" } } @@ -44,3 +45,24 @@ local object = { assetHelper.registerSceneGraphNodesAndExport(asset, { object }) + + +asset.meta = { + Name = "Pulsars", + Version = "2.0", + Description = [[Census: 2,498 pulsars. DU Version 5.6. Upon death, stars leave behind + one of three possible remnants: a white dwarf, a neutron star, or a black hole. + Stars that are more massive than the sun will often become neutron stars in a + violent explosion called a supernova. During a supernova, the core of the star + collapses under such high pressure that the electrons, which normally remain + outside the atomic nucleus, are forced to combine with the protons in the nucleus. + Atomic nuclei break apart, producing what is called a degenerate state of matter. + The collapse is halted when the material cannot be packed any tighter. At this + point, the star has a radius of about 10-15 kilometers. The density of this + material is so high that a teaspoonful would weigh about 100 million tons on + Earth. (Description from URL)

Data Reference: ATNF Pulsar Catalogue, + (Manchester+, 2005)]], + Author = "Brian Abbott (AMNH)", + URL = "https://www.amnh.org/research/hayden-planetarium/digital-universe", + License = "AMNH Digital Universe" +} diff --git a/data/assets/scene/digitaluniverse/quasars.asset b/data/assets/scene/digitaluniverse/quasars.asset index be9b11e59b..81dc10dbfe 100644 --- a/data/assets/scene/digitaluniverse/quasars.asset +++ b/data/assets/scene/digitaluniverse/quasars.asset @@ -35,6 +35,7 @@ local object = { EnablePixelSizeControl = true }, GUI = { + Name = "Quasars", Path = "/Universe" } } @@ -42,3 +43,19 @@ local object = { assetHelper.registerSceneGraphNodesAndExport(asset, { object }) + + +asset.meta = { + Name = "Quasars", + Version = "2.0", + Description = [[Census: 569,442 quasars. DU Version 2.2. Quasars are the most distant + objects we can see. They are extremely active galaxies that contain supermassive + black holes which are gobbling up material at a furious rate. The Million Quasars + Catalogue is an aggregate catalog of several surveys, including 2dF and Sloan. So, + it should not be surprising that the shape of these data mimic the shape of the + Sloan and 2dF galaxy surveys, with large parts of the sky unobserved.(Description + from URL)

Data Reference: The Million Quasars catalog (Flesch, 2017)]], + Author = "Brian Abbott (AMNH)", + URL = "https://www.amnh.org/research/hayden-planetarium/digital-universe", + License = "AMNH Digital Universe" +} diff --git a/data/assets/scene/digitaluniverse/sdss.asset b/data/assets/scene/digitaluniverse/sdss.asset index 56d92df264..2637234935 100644 --- a/data/assets/scene/digitaluniverse/sdss.asset +++ b/data/assets/scene/digitaluniverse/sdss.asset @@ -51,3 +51,27 @@ local object = { assetHelper.registerSceneGraphNodesAndExport(asset, { object }) + + +asset.meta = { + Name = "Sloan Digital Sky Survey", + Version = "2.0", + Description = [[Census: 2,600,258 galaxies. DU Version 10.6. The Sloan Digital Sky + Survey (SDSS) is an ambitious project to image about 35% of the sky, deep into the + universe. The survey measured the position and brightness of almost 1 billion + objects, and obtained spectra to more than 4 million objects. This is not an + all-sky survey, so there are large parts of the sky that remain unobserved, which + produces the bow tie distribution and the black areas where there surely are + galaxies, but we have yet to observe them. These galaxies appear to extend beyond + the 2dF survey to distances that exceed 5 billion light years. However, the + weblike structure of clusters, filaments, and voids seems to fade by about 2 + billion light years. Beyond this distance, the completeness of the survey drops so + that only the intrinsically bright galaxies are visible. The weblike cosmic + structure is echoed in these data, with orange clusters standing out among the + less dense aqua-colored galaxies and the less dense regions of green-colored + galaxies. (Description from URL)

Data Reference: Sloan Digital Sky Survey + (http://www.sdss.org/)]], + Author = "Brian Abbott (AMNH)", + URL = "https://www.amnh.org/research/hayden-planetarium/digital-universe", + License = "AMNH Digital Universe" +} diff --git a/data/assets/scene/digitaluniverse/starlabels.asset b/data/assets/scene/digitaluniverse/starlabels.asset index 6e12b8e7eb..64025a69e8 100644 --- a/data/assets/scene/digitaluniverse/starlabels.asset +++ b/data/assets/scene/digitaluniverse/starlabels.asset @@ -33,3 +33,13 @@ local object = { assetHelper.registerSceneGraphNodesAndExport(asset, { object }) + + +asset.meta = { + Name = "Star Labels", + Version = "2.0", + Description = [[Labels for stars in the Milky Way. See 'Stars' asset for more info.]], + Author = "Brian Abbott (AMNH)", + URL = "https://www.amnh.org/research/hayden-planetarium/digital-universe", + License = "AMNH Digital Universe" +} diff --git a/data/assets/scene/digitaluniverse/starorbits.asset b/data/assets/scene/digitaluniverse/starorbits.asset index 212d2a9b3f..67e5b6120f 100644 --- a/data/assets/scene/digitaluniverse/starorbits.asset +++ b/data/assets/scene/digitaluniverse/starorbits.asset @@ -168,3 +168,16 @@ assetHelper.registerSceneGraphNodesAndExport(asset, { sunOrbit, barnardsOrbit, pM_J13420Orbit, lSRJ0822Orbit, lSR1826Orbit, lacaille9352Orbit, kapteynsOrbit }) + + +asset.meta = { + Name = "Star Orbits", + Version = "1.0", + Description = [[Select Star Orbital paths that delineate their trajectory around the + Milky Way over 1 billion years into the future. Included: Sun, Barnards, Kapteyns, + Lacaille 9352, LSR1826+3014, LSRJ0822+1700, PM_J13420-3415.

Data + Reference: Sebastien Lepine (AMNH)]], + Author = "Brian Abbott (AMNH)", + URL = "https://www.amnh.org/research/hayden-planetarium/digital-universe", + License = "AMNH Digital Universe" +} diff --git a/data/assets/scene/digitaluniverse/stars.asset b/data/assets/scene/digitaluniverse/stars.asset index 0407908aab..9a1d5b31be 100644 --- a/data/assets/scene/digitaluniverse/stars.asset +++ b/data/assets/scene/digitaluniverse/stars.asset @@ -67,3 +67,18 @@ local sunstar = { } assetHelper.registerSceneGraphNodesAndExport(asset, { stars, sunstar }) + + +asset.meta = { + Name = "Stars", + Version = "2.0", + Description = [[Census: 117,003 stars with 321 labels. DU Version 7.8. This star + catalog is a combination of all available star catalogs, wherein we choose the + best distance available to place the stars around the Sun as accurately as is + possible. (Description from URL)

Data Reference: XHIP: An Extended + Hipparcos Compilation (Anderson E., Francis C. 2012); Hipparcos Catalog + (European Space Agency 1997); Gliese Catalog (Gliese and Jahriess 1991)]], + Author = "Brian Abbott (AMNH)", + URL = "https://www.amnh.org/research/hayden-planetarium/digital-universe", + License = "AMNH Digital Universe" +} diff --git a/data/assets/scene/digitaluniverse/superclusters.asset b/data/assets/scene/digitaluniverse/superclusters.asset index 6ebbb1f488..107c0fab0c 100644 --- a/data/assets/scene/digitaluniverse/superclusters.asset +++ b/data/assets/scene/digitaluniverse/superclusters.asset @@ -45,3 +45,18 @@ local object = { assetHelper.registerSceneGraphNodesAndExport(asset, { object }) + + +asset.meta = { + Name = "Galaxy Superclusters", + Version = "2.0", + Description = [[Census: 33 labels. DU Version 1.3. The superclusters dataset is a set + of labels that mark the major galaxy superclusters in the local universe. They + correspond to, and should be viewed with, the Abell clusters. Astronomers estimate + there are 10 million superclusters in the observable universe. (Description from + URL)

Data Reference: Superclusters of Abell and X-ray clusters (Einasto+, + 2001)]], + Author = "Brian Abbott (AMNH)", + URL = "https://www.amnh.org/research/hayden-planetarium/digital-universe", + License = "AMNH Digital Universe" +} diff --git a/data/assets/scene/digitaluniverse/supernovaremnants.asset b/data/assets/scene/digitaluniverse/supernovaremnants.asset index c821080e65..fe81aa9c73 100644 --- a/data/assets/scene/digitaluniverse/supernovaremnants.asset +++ b/data/assets/scene/digitaluniverse/supernovaremnants.asset @@ -47,3 +47,16 @@ local object = { assetHelper.registerSceneGraphNodesAndExport(asset, { object }) + + +asset.meta = { + Name = "Supernova Remnants", + Version = "2.0", + Description = [[Census: 112 supernova remnants. DU Version 3.7. A supernova remnant is + the ejected gas that results from a supernova. It glows for a cosmically short + period of time before mixing with the interstellar medium. (Description from URL) +

Data Reference: The First Fermi LAT SNR Catalog (Acero+, 2016)]], + Author = "Brian Abbott (AMNH)", + URL = "https://www.amnh.org/research/hayden-planetarium/digital-universe", + License = "AMNH Digital Universe" +} diff --git a/data/assets/scene/digitaluniverse/tully.asset b/data/assets/scene/digitaluniverse/tully.asset index 45ce730432..f8cada0262 100644 --- a/data/assets/scene/digitaluniverse/tully.asset +++ b/data/assets/scene/digitaluniverse/tully.asset @@ -89,3 +89,36 @@ local tullyImages = { assetHelper.registerSceneGraphNodesAndExport(asset, { tullyPoints, tullyImages }) + + +asset.meta = { + Name = "Tully Galaxies", + Version = "3.0", + Description = [[Census: 30,059 galaxies. DU Version 1.5. The Tully Catalog is the most + polished, accurate catalog of nearby galaxies. It includes over 30,000 galaxies in + the local universe that surround the Milky Way. This catalog demonstrates the + large-scale structure of the universe exceptionally well. And, each galaxy has a + representative image reflecting its morphological type, and is properly sized and + inclined. Size and shape. The data form a cube, which is an arbitrary cutoff based + on the completeness of these data. Beyond this, data from these sources are not as + reliable, so effort is made to show a complete picture, albeit limited by + observations (for example, we cannot see dwarf galaxies much beyond the Local + Group). The size of the cube is roughly 1 billion light years on a diagonal (so + the farthest galaxies in the dataset are about 1 billion light years from the + Milky Way), or about 700 million light years per side.

Colors. Orange + denotes more dense regions of the local universe, aqua is given to galaxies in an + intermediate-density area, and green is given to lower density regions.

+ Galaxy images. Each galaxy is represented by an image that represents its + morphological type (spiral, elliptical, etc.). Most of these come from The Galaxy + Catalog. A handful of nearby galaxies are represented by their actual images, + which come mostly from the National Optical Astronomy Observatory (NOAO). Each of + these images has been altered from its original state. These images were taken + from Earth on some of the world’s largest telescopes, so foreground stars from our + own Galaxy appear in each image. We are representing galaxies in extragalactic + space, so we have removed the stars from each image. (Description from + URL)

Data Reference: Tully Galaxy Catalog: Brent Tully (U Hawaii), Stuart + Levy (NCSA/UIUC)]], + Author = "Stuart Levy (NCSA/UIUC), Brian Abbott (AMNH)", + URL = "https://www.amnh.org/research/hayden-planetarium/digital-universe", + License = "AMNH Digital Universe" +} diff --git a/data/assets/scene/digitaluniverse/voids.asset b/data/assets/scene/digitaluniverse/voids.asset index 420ebe54b7..7cf0d9a289 100644 --- a/data/assets/scene/digitaluniverse/voids.asset +++ b/data/assets/scene/digitaluniverse/voids.asset @@ -25,6 +25,7 @@ local object = { Unit = "Mpc" }, GUI = { + Name = "Voids", Path = "/Universe/Galaxies" } } @@ -32,3 +33,21 @@ local object = { assetHelper.registerSceneGraphNodesAndExport(asset, { object }) + + +asset.meta = { + Name = "Voids", + Version = "2.0", + Description = [[Census: 24 cosmic voids. DU Version 1.2. Cosmic voids are vast, empty + spaces where there are either no galaxies, or very few galaxies. They are + associated with cold spots in the cosmic microwave background (CMB) light, the + earliest picture we have of the universe (see page 58). Those cold spots in the + CMB evolved into large voids, some as much as 300 million light years in diameter. + Labels roughly denote the location of cosmic voids in the Tully galaxies. Voids + are only visible with motion cuing as you spin around these data. The labels help + to guide the eye and provide sign posts for the largest voids in our cosmic + neighborhood. (Description from URL)

Data Reference: various sources]], + Author = "Brian Abbott (AMNH)", + URL = "https://www.amnh.org/research/hayden-planetarium/digital-universe", + License = "AMNH Digital Universe" +} diff --git a/data/assets/scene/solarsystem/dwarf_planets/pluto/charon/default_layers.asset b/data/assets/scene/solarsystem/dwarf_planets/pluto/charon/default_layers.asset index f1bb6e13c7..fa48f1b2ef 100644 --- a/data/assets/scene/solarsystem/dwarf_planets/pluto/charon/default_layers.asset +++ b/data/assets/scene/solarsystem/dwarf_planets/pluto/charon/default_layers.asset @@ -13,7 +13,7 @@ end) asset.meta = { Name = "Default Charon Layers", Version = "1.0", - Description = [[ Default Charon layers are: Black & White [USGS]]], + Description = [[ Default Charon layers are: Black & White USGS]], Author = "OpenSpace Team", URL = "http://openspaceproject.com", License = "MIT license" diff --git a/data/assets/scene/solarsystem/dwarf_planets/pluto/default_layers.asset b/data/assets/scene/solarsystem/dwarf_planets/pluto/default_layers.asset index 43af4ff920..b5e907d024 100644 --- a/data/assets/scene/solarsystem/dwarf_planets/pluto/default_layers.asset +++ b/data/assets/scene/solarsystem/dwarf_planets/pluto/default_layers.asset @@ -13,7 +13,7 @@ end) asset.meta = { Name = "Default Pluto Layers", Version = "1.0", - Description = [[ Default Pluto layers are: Black & White [USGS]]], + Description = [[ Default Pluto layers are: Black & White USGS]], Author = "OpenSpace Team", URL = "http://openspaceproject.com", License = "MIT license" diff --git a/data/assets/scene/solarsystem/planets/mercury/trail.asset b/data/assets/scene/solarsystem/planets/mercury/trail.asset index 6f9febd412..8037c6bf31 100644 --- a/data/assets/scene/solarsystem/planets/mercury/trail.asset +++ b/data/assets/scene/solarsystem/planets/mercury/trail.asset @@ -21,7 +21,7 @@ local MercuryTrail = { Tag = { "planetTrail_solarSystem", "planetTrail_terrestrial" }, GUI = { Name = "Mercury Trail", - Path = "/Solar System/Planets/Mercury" + Path = "/Milky Way/Gaia/Mercury" } } diff --git a/data/assets/scene/solarsystem/planets/venus/trail_earth.asset b/data/assets/scene/solarsystem/planets/venus/trail_earth.asset index eb55c4b3d5..4573474634 100644 --- a/data/assets/scene/solarsystem/planets/venus/trail_earth.asset +++ b/data/assets/scene/solarsystem/planets/venus/trail_earth.asset @@ -3,10 +3,11 @@ local transforms = asset.require('scene/solarsystem/sun/transforms') asset.require("spice/base") +local etransforms = asset.require('scene/solarsystem/planets/earth/transforms') local VenusTrailEarth = { Identifier = "VenusTrailEarth", - Parent = transforms.SolarSystemBarycenter.Identifier, + Parent = etransforms.EarthBarycenter.Identifier, Renderable = { Type = "RenderableTrailOrbit", Translation = { @@ -20,9 +21,9 @@ local VenusTrailEarth = { }, Tag = { "planetTrail_solarSystem", "planetTrail_terrestrial" }, GUI = { - Name = "Venus Trail from Earth", + Name = "Venus trail from Earth", Path = "/Solar System/Planets/Venus", - Hidden = true + Hidden = false } } diff --git a/data/web/documentation/scenelicense.hbs b/data/web/documentation/scenelicense.hbs index f60b719a53..7fd118c072 100644 --- a/data/web/documentation/scenelicense.hbs +++ b/data/web/documentation/scenelicense.hbs @@ -8,9 +8,9 @@

{{{description}}}

Version - {{version}}

-

Author - {{author}}

+

Author - {{{author}}}

Associated URL - {{url}}

-

License - {{license}}

+

License - {{{license}}}

Filepath - {{path}}

diff --git a/data/web/documentation/script.js b/data/web/documentation/script.js index ba8e45eb4b..280ea2cd8f 100644 --- a/data/web/documentation/script.js +++ b/data/web/documentation/script.js @@ -133,6 +133,10 @@ window.onload = function () { /\\n/g, "" ); documentation[i].data[j].description = escaped; + var escapedLicense = documentation[i].data[j].license.replace( + /\\n/g, "" + ); + documentation[i].data[j].license = escapedLicense; } }