{
"id": 4425,
"url": "https://svs.gsfc.nasa.gov/4425/",
"page_type": "Visualization",
"title": "March 2016 Eclipse and the Moon's Orbit",
"description": "The Moon orbits the Earth in the months prior to the March 9, 2016 (March 8 in the Americas) total solar eclipse. Viewed from above, the Moon's shadow appears to cross the Earth every month, but a side view reveals the five-degree tilt of the Moon's orbit. Its shadow only hits the Earth when the line of nodes, the fulcrum of its orbital tilt, is pointed toward the Sun. || orbit.0360_print.jpg (1024x576) [38.2 KB] || orbit.0360_searchweb.png (320x180) [38.1 KB] || orbit.0360_thm.png (80x40) [4.0 KB] || 2016tse_orbit_1080p30.mp4 (1920x1080) [3.6 MB] || 2016tse_orbit_720p30.mp4 (1280x720) [1.7 MB] || orbit (1920x1080) [0 Item(s)] || 2016tse_orbit_720p30.webm (1280x720) [3.3 MB] || 2016tse_orbit_360p30.mp4 (640x360) [594.9 KB] || 2016tse_orbit_1080p30.mp4.hwshow [187 bytes] || ",
"release_date": "2016-02-12T10:00:00-05:00",
"update_date": "2025-01-05T22:59:03.786344-05:00",
"main_image": {
"id": 427255,
"url": "https://svs.gsfc.nasa.gov/vis/a000000/a004400/a004425/orbit.0360_print.jpg",
"filename": "orbit.0360_print.jpg",
"media_type": "Image",
"alt_text": "The Moon orbits the Earth in the months prior to the March 9, 2016 (March 8 in the Americas) total solar eclipse. Viewed from above, the Moon's shadow appears to cross the Earth every month, but a side view reveals the five-degree tilt of the Moon's orbit. Its shadow only hits the Earth when the line of nodes, the fulcrum of its orbital tilt, is pointed toward the Sun.",
"width": 1024,
"height": 576,
"pixels": 589824
},
"main_video": null,
"main_credits": {
"Visualizations by": [
{
"name": "Ernie Wright",
"employer": "USRA"
}
]
},
"progress": "Complete",
"media_groups": [
{
"id": 334985,
"url": "https://svs.gsfc.nasa.gov/4425/#media_group_334985",
"widget": "Video player",
"title": "",
"caption": "",
"description": "The Moon orbits the Earth in the months prior to the March 9, 2016 (March 8 in the Americas) total solar eclipse. Viewed from above, the Moon's shadow appears to cross the Earth every month, but a side view reveals the five-degree tilt of the Moon's orbit. Its shadow only hits the Earth when the line of nodes, the fulcrum
of its orbital tilt, is pointed toward the Sun.",
"items": [
{
"id": 272629,
"type": "media",
"extra_data": null,
"title": null,
"caption": null,
"instance": {
"id": 427255,
"url": "https://svs.gsfc.nasa.gov/vis/a000000/a004400/a004425/orbit.0360_print.jpg",
"filename": "orbit.0360_print.jpg",
"media_type": "Image",
"alt_text": "The Moon orbits the Earth in the months prior to the March 9, 2016 (March 8 in the Americas) total solar eclipse. Viewed from above, the Moon's shadow appears to cross the Earth every month, but a side view reveals the five-degree tilt of the Moon's orbit. Its shadow only hits the Earth when the line of nodes, the fulcrum of its orbital tilt, is pointed toward the Sun.",
"width": 1024,
"height": 576,
"pixels": 589824
}
},
{
"id": 272630,
"type": "media",
"extra_data": null,
"title": null,
"caption": null,
"instance": {
"id": 427256,
"url": "https://svs.gsfc.nasa.gov/vis/a000000/a004400/a004425/orbit.0360_searchweb.png",
"filename": "orbit.0360_searchweb.png",
"media_type": "Image",
"alt_text": "The Moon orbits the Earth in the months prior to the March 9, 2016 (March 8 in the Americas) total solar eclipse. Viewed from above, the Moon's shadow appears to cross the Earth every month, but a side view reveals the five-degree tilt of the Moon's orbit. Its shadow only hits the Earth when the line of nodes, the fulcrum of its orbital tilt, is pointed toward the Sun.",
"width": 320,
"height": 180,
"pixels": 57600
}
},
{
"id": 272631,
"type": "media",
"extra_data": null,
"title": null,
"caption": null,
"instance": {
"id": 427257,
"url": "https://svs.gsfc.nasa.gov/vis/a000000/a004400/a004425/orbit.0360_thm.png",
"filename": "orbit.0360_thm.png",
"media_type": "Image",
"alt_text": "The Moon orbits the Earth in the months prior to the March 9, 2016 (March 8 in the Americas) total solar eclipse. Viewed from above, the Moon's shadow appears to cross the Earth every month, but a side view reveals the five-degree tilt of the Moon's orbit. Its shadow only hits the Earth when the line of nodes, the fulcrum of its orbital tilt, is pointed toward the Sun.",
"width": 80,
"height": 40,
"pixels": 3200
}
},
{
"id": 272625,
"type": "media",
"extra_data": null,
"title": null,
"caption": null,
"instance": {
"id": 427251,
"url": "https://svs.gsfc.nasa.gov/vis/a000000/a004400/a004425/2016tse_orbit_1080p30.mp4",
"filename": "2016tse_orbit_1080p30.mp4",
"media_type": "Movie",
"alt_text": "The Moon orbits the Earth in the months prior to the March 9, 2016 (March 8 in the Americas) total solar eclipse. Viewed from above, the Moon's shadow appears to cross the Earth every month, but a side view reveals the five-degree tilt of the Moon's orbit. Its shadow only hits the Earth when the line of nodes, the fulcrum of its orbital tilt, is pointed toward the Sun.",
"width": 1920,
"height": 1080,
"pixels": 2073600
}
},
{
"id": 272626,
"type": "media",
"extra_data": null,
"title": null,
"caption": null,
"instance": {
"id": 427252,
"url": "https://svs.gsfc.nasa.gov/vis/a000000/a004400/a004425/2016tse_orbit_720p30.mp4",
"filename": "2016tse_orbit_720p30.mp4",
"media_type": "Movie",
"alt_text": "The Moon orbits the Earth in the months prior to the March 9, 2016 (March 8 in the Americas) total solar eclipse. Viewed from above, the Moon's shadow appears to cross the Earth every month, but a side view reveals the five-degree tilt of the Moon's orbit. Its shadow only hits the Earth when the line of nodes, the fulcrum of its orbital tilt, is pointed toward the Sun.",
"width": 1280,
"height": 720,
"pixels": 921600
}
},
{
"id": 272628,
"type": "media",
"extra_data": null,
"title": null,
"caption": null,
"instance": {
"id": 427254,
"url": "https://svs.gsfc.nasa.gov/vis/a000000/a004400/a004425/frames/1920x1080_16x9_30p/orbit/",
"filename": "orbit",
"media_type": "Frames",
"alt_text": "The Moon orbits the Earth in the months prior to the March 9, 2016 (March 8 in the Americas) total solar eclipse. Viewed from above, the Moon's shadow appears to cross the Earth every month, but a side view reveals the five-degree tilt of the Moon's orbit. Its shadow only hits the Earth when the line of nodes, the fulcrum of its orbital tilt, is pointed toward the Sun.",
"width": 1920,
"height": 1080,
"pixels": 2073600
}
},
{
"id": 272632,
"type": "media",
"extra_data": null,
"title": null,
"caption": null,
"instance": {
"id": 427258,
"url": "https://svs.gsfc.nasa.gov/vis/a000000/a004400/a004425/2016tse_orbit_720p30.webm",
"filename": "2016tse_orbit_720p30.webm",
"media_type": "Movie",
"alt_text": "The Moon orbits the Earth in the months prior to the March 9, 2016 (March 8 in the Americas) total solar eclipse. Viewed from above, the Moon's shadow appears to cross the Earth every month, but a side view reveals the five-degree tilt of the Moon's orbit. Its shadow only hits the Earth when the line of nodes, the fulcrum of its orbital tilt, is pointed toward the Sun.",
"width": 1280,
"height": 720,
"pixels": 921600
}
},
{
"id": 272627,
"type": "media",
"extra_data": null,
"title": null,
"caption": null,
"instance": {
"id": 427253,
"url": "https://svs.gsfc.nasa.gov/vis/a000000/a004400/a004425/2016tse_orbit_360p30.mp4",
"filename": "2016tse_orbit_360p30.mp4",
"media_type": "Movie",
"alt_text": "The Moon orbits the Earth in the months prior to the March 9, 2016 (March 8 in the Americas) total solar eclipse. Viewed from above, the Moon's shadow appears to cross the Earth every month, but a side view reveals the five-degree tilt of the Moon's orbit. Its shadow only hits the Earth when the line of nodes, the fulcrum of its orbital tilt, is pointed toward the Sun.",
"width": 640,
"height": 360,
"pixels": 230400
}
},
{
"id": 439319,
"type": "media",
"extra_data": null,
"title": null,
"caption": null,
"instance": {
"id": 1100980,
"url": "https://svs.gsfc.nasa.gov/vis/a000000/a004400/a004425/2016tse_orbit_1080p30.mp4.hwshow",
"filename": "2016tse_orbit_1080p30.mp4.hwshow",
"media_type": "HyperwallShow",
"alt_text": "",
"width": 0,
"height": 0,
"pixels": null
}
}
],
"extra_data": {}
},
{
"id": 334984,
"url": "https://svs.gsfc.nasa.gov/4425/#media_group_334984",
"widget": "Basic text with HTML",
"title": "",
"caption": "",
"description": "Solar eclipses can only occur at New Moon, when the Moon is between the Earth and the Sun. But not every New Moon produces an eclipse. The Moon's orbit is slightly tilted, and as seen in this animation, the tilt causes the Moon's shadow to miss the Earth during most New Moons—about five out of six, in fact.
As the Earth-Moon system orbits the Sun throughout the year, the Moon's orbital tilt changes direction relative to the Sun. Sometimes the up
side of the orbit is facing the Sun, and sometimes the down
side. Twice a year, for about a month, what's facing the Sun is the line dividing the up and down sides. This is the line of nodes, the intersection of the Earth-Moon plane and the ecliptic or Earth-Sun plane. A solar eclipse can only occur at a New Moon that falls within one of these month-long eclipse seasons. That's when the Moon is close enough to the ecliptic to actually come between the Earth and the Sun.
In this animation, the olive-colored square represents the ecliptic plane, while the light blue circle shows the plane of the Moon's orbit. The darker half of the lunar orbit plane is below (south of) the ecliptic, and the dividing line between light and dark is the line of nodes.
The radial grid on the lunar orbit plane is stationary relative to the stars. It appears to rotate because our point of view is fixed to the Earth-Sun line; we're following the Earth as it orbits the Sun. At first glance, the line of nodes appears to be tracking with the grid, but in reality it's slowly turning westward (clockwise), completing a full revolution in 18.6 years.
Unlike most illustrations of this kind, the Earth and the Moon are to scale. The Sun is off-screen to the left, about 400 times farther than the Earth-Moon distance and roughly twice as big as the Moon's orbit.",
"items": [],
"extra_data": {}
},
{
"id": 334986,
"url": "https://svs.gsfc.nasa.gov/4425/#media_group_334986",
"widget": "Video player",
"title": "",
"caption": "",
"description": "In this oblique view, the umbra component of the Moon's shadow barely reaches the Earth as it traces a path across the Pacific Ocean.",
"items": [
{
"id": 272637,
"type": "media",
"extra_data": null,
"title": null,
"caption": null,
"instance": {
"id": 427263,
"url": "https://svs.gsfc.nasa.gov/vis/a000000/a004400/a004425/orbit.0250_print.jpg",
"filename": "orbit.0250_print.jpg",
"media_type": "Image",
"alt_text": "In this oblique view, the umbra component of the Moon's shadow barely reaches the Earth as it traces a path across the Pacific Ocean.",
"width": 1024,
"height": 576,
"pixels": 589824
}
},
{
"id": 272633,
"type": "media",
"extra_data": null,
"title": null,
"caption": null,
"instance": {
"id": 427259,
"url": "https://svs.gsfc.nasa.gov/vis/a000000/a004400/a004425/2016tse_orbit_oblique_1080p30.mp4",
"filename": "2016tse_orbit_oblique_1080p30.mp4",
"media_type": "Movie",
"alt_text": "In this oblique view, the umbra component of the Moon's shadow barely reaches the Earth as it traces a path across the Pacific Ocean.",
"width": 1920,
"height": 1080,
"pixels": 2073600
}
},
{
"id": 272634,
"type": "media",
"extra_data": null,
"title": null,
"caption": null,
"instance": {
"id": 427260,
"url": "https://svs.gsfc.nasa.gov/vis/a000000/a004400/a004425/2016tse_orbit_oblique_720p30.mp4",
"filename": "2016tse_orbit_oblique_720p30.mp4",
"media_type": "Movie",
"alt_text": "In this oblique view, the umbra component of the Moon's shadow barely reaches the Earth as it traces a path across the Pacific Ocean.",
"width": 1280,
"height": 720,
"pixels": 921600
}
},
{
"id": 272636,
"type": "media",
"extra_data": null,
"title": null,
"caption": null,
"instance": {
"id": 427262,
"url": "https://svs.gsfc.nasa.gov/vis/a000000/a004400/a004425/frames/1920x1080_16x9_30p/oblique/",
"filename": "oblique",
"media_type": "Frames",
"alt_text": "In this oblique view, the umbra component of the Moon's shadow barely reaches the Earth as it traces a path across the Pacific Ocean.",
"width": 1920,
"height": 1080,
"pixels": 2073600
}
},
{
"id": 272638,
"type": "media",
"extra_data": null,
"title": null,
"caption": null,
"instance": {
"id": 427264,
"url": "https://svs.gsfc.nasa.gov/vis/a000000/a004400/a004425/2016tse_orbit_oblique_720p30.webm",
"filename": "2016tse_orbit_oblique_720p30.webm",
"media_type": "Movie",
"alt_text": "In this oblique view, the umbra component of the Moon's shadow barely reaches the Earth as it traces a path across the Pacific Ocean.",
"width": 1280,
"height": 720,
"pixels": 921600
}
},
{
"id": 272635,
"type": "media",
"extra_data": null,
"title": null,
"caption": null,
"instance": {
"id": 427261,
"url": "https://svs.gsfc.nasa.gov/vis/a000000/a004400/a004425/2016tse_orbit_oblique_360p30.mp4",
"filename": "2016tse_orbit_oblique_360p30.mp4",
"media_type": "Movie",
"alt_text": "In this oblique view, the umbra component of the Moon's shadow barely reaches the Earth as it traces a path across the Pacific Ocean.",
"width": 640,
"height": 360,
"pixels": 230400
}
},
{
"id": 439320,
"type": "media",
"extra_data": null,
"title": null,
"caption": null,
"instance": {
"id": 1100981,
"url": "https://svs.gsfc.nasa.gov/vis/a000000/a004400/a004425/2016tse_orbit_oblique_1080p30.mp4.hwshow",
"filename": "2016tse_orbit_oblique_1080p30.mp4.hwshow",
"media_type": "HyperwallShow",
"alt_text": "",
"width": 0,
"height": 0,
"pixels": null
}
}
],
"extra_data": {}
}
],
"studio": "svs",
"funding_sources": [
"NASA Heliophysics"
],
"credits": [
{
"role": "Visualizer",
"people": [
{
"name": "Ernie Wright",
"employer": "USRA"
}
]
},
{
"role": "Producer",
"people": [
{
"name": "Genna Duberstein",
"employer": "USRA"
}
]
}
],
"missions": [],
"series": [],
"tapes": [],
"papers": [],
"datasets": [
{
"name": "JPL DE421",
"common_name": "DE421",
"platform": null,
"sensor": null,
"type": "Ephemeris",
"organizations": [
"NASA/JPL"
],
"description": "Planetary ephemerides",
"credit": "",
"url": "http://ssd.jpl.nasa.gov/?ephemerides#planets",
"date_range": null
}
],
"nasa_science_categories": [
"Earth",
"Planets & Moons",
"Sun"
],
"keywords": [
"Eclipse",
"HDTV",
"Heliophysics",
"Hyperwall",
"Moon",
"Orbit",
"Solar Eclipse",
"Sun and Earth",
"Sun-Earth-Moon Interactions"
],
"recommended_pages": [],
"related": [
{
"id": 4424,
"url": "https://svs.gsfc.nasa.gov/4424/",
"page_type": "Visualization",
"title": "March 2016 Eclipse Shadow Cones",
"description": "The umbral and penumbral shadow cones travel across the surface of the Earth during the March 9, 2016 total solar eclipse. || cones.0850_print.jpg (1024x576) [92.5 KB] || cones.0850_searchweb.png (320x180) [56.7 KB] || cones.0850_thm.png (80x40) [5.0 KB] || tse2016_cones_1080p30.mp4 (1920x1080) [19.0 MB] || tse2016_cones_720p30.mp4 (1280x720) [9.4 MB] || 1920x1080_16x9_30p (1920x1080) [0 Item(s)] || tse2016_cones_720p30.webm (1280x720) [6.8 MB] || tse2016_cones_360p30.mp4 (640x360) [3.0 MB] || tse2016_cones_1080p30.mp4.hwshow [187 bytes] || ",
"release_date": "2016-02-12T10:00:00-05:00",
"update_date": "2025-01-05T22:59:03.371967-05:00",
"main_image": {
"id": 427208,
"url": "https://svs.gsfc.nasa.gov/vis/a000000/a004400/a004424/cones.0850_print.jpg",
"filename": "cones.0850_print.jpg",
"media_type": "Image",
"alt_text": "The umbral and penumbral shadow cones travel across the surface of the Earth during the March 9, 2016 total solar eclipse.",
"width": 1024,
"height": 576,
"pixels": 589824
}
},
{
"id": 4426,
"url": "https://svs.gsfc.nasa.gov/4426/",
"page_type": "Visualization",
"title": "March 2016 Eclipse: Earth, Moon and Sun",
"description": "The Moon moves right to left in its orbit around the Earth. The shadow it casts hits the Earth during the March 9, 2016 total solar eclipse. || sun_earth.0270_print.jpg (1024x576) [43.2 KB] || sun_earth.0270_searchweb.png (320x180) [38.3 KB] || sun_earth.0270_print_thm.png (80x40) [4.3 KB] || 2016tse_sun_earth_1080p30.mp4 (1920x1080) [4.7 MB] || 2016tse_sun_earth_720p30.mp4 (1280x720) [2.1 MB] || 1920x1080_16x9_30p (1920x1080) [0 Item(s)] || 2016tse_sun_earth_720p30.webm (1280x720) [3.4 MB] || 2016tse_sun_earth_360p30.mp4 (640x360) [681.1 KB] || 2016tse_sun_earth_1080p30.mp4.hwshow [191 bytes] || ",
"release_date": "2016-02-12T10:00:00-05:00",
"update_date": "2025-01-05T22:59:04.194943-05:00",
"main_image": {
"id": 427269,
"url": "https://svs.gsfc.nasa.gov/vis/a000000/a004400/a004426/sun_earth.0270_print.jpg",
"filename": "sun_earth.0270_print.jpg",
"media_type": "Image",
"alt_text": "The Moon moves right to left in its orbit around the Earth. The shadow it casts hits the Earth during the March 9, 2016 total solar eclipse.",
"width": 1024,
"height": 576,
"pixels": 589824
}
},
{
"id": 4427,
"url": "https://svs.gsfc.nasa.gov/4427/",
"page_type": "Visualization",
"title": "March 2016 Total Solar Eclipse Path",
"description": "The animated shadow path of the March 9, 2016 total solar eclipse, showing the umbra (black oval), penumbra (concentric shaded ovals), and path of totality (red) through Indonesia and the western Pacific.This video is also available on our YouTube channel. || path.0885_print.jpg (1024x576) [108.6 KB] || path.0885_searchweb.png (320x180) [76.0 KB] || path.0885_thm.png (80x40) [6.9 KB] || 2016tse_path_1080p30.mp4 (1920x1080) [21.6 MB] || 2016tse_path_720p30.mp4 (1280x720) [12.0 MB] || fancy (1920x1080) [0 Item(s)] || 2016tse_path_720p30.webm (1280x720) [6.6 MB] || 2016tse_path_360p30.mp4 (640x360) [4.8 MB] || 2016tse_path_1080p30.mp4.hwshow [186 bytes] || ",
"release_date": "2016-02-12T10:00:00-05:00",
"update_date": "2025-01-05T22:59:04.605746-05:00",
"main_image": {
"id": 427277,
"url": "https://svs.gsfc.nasa.gov/vis/a000000/a004400/a004427/path.0885_print.jpg",
"filename": "path.0885_print.jpg",
"media_type": "Image",
"alt_text": "The animated shadow path of the March 9, 2016 total solar eclipse, showing the umbra (black oval), penumbra (concentric shaded ovals), and path of totality (red) through Indonesia and the western Pacific.This video is also available on our YouTube channel.",
"width": 1024,
"height": 576,
"pixels": 589824
}
}
],
"sources": [
{
"id": 14325,
"url": "https://svs.gsfc.nasa.gov/14325/",
"page_type": "Produced Video",
"title": "What Is an Annular Eclipse?",
"description": "On Oct. 14, 2023, an annular solar eclipse will cross North, Central, and South America. Visible in parts of the United States, Mexico, and many countries in South and Central America, millions of people in the Western Hemisphere can experience this eclipse. But what is an annular eclipse? Why does it happen? And why does it create a “ring of fire” in the sky? || ",
"release_date": "2023-04-14T08:00:00-04:00",
"update_date": "2023-11-01T15:08:24.072102-04:00",
"main_image": {
"id": 860715,
"url": "https://svs.gsfc.nasa.gov/vis/a010000/a014300/a014325/14325_AnnularEclipseExplainer_FB.00120_print.jpg",
"filename": "14325_AnnularEclipseExplainer_FB.00120_print.jpg",
"media_type": "Image",
"alt_text": "Credit: NASA's Goddard Space Flight CenterMusic: \"Insect Village\" by Anthony Donje [PRS] from Universal Production MusicComplete transcript available.",
"width": 1024,
"height": 576,
"pixels": 589824
}
}
],
"products": [
{
"id": 13668,
"url": "https://svs.gsfc.nasa.gov/13668/",
"page_type": "Produced Video",
"title": "Cómo ver un eclipse solar de forma segura",
"description": "Nunca es seguro mirar directamente al Sol, incluso si está parcialmente oscurecido. Al observar un eclipse parcial, debes usar gafas de eclipse en todo momento si deseas mirar el Sol, o utilizar un método indirecto alternativo. Esto también se aplica durante un eclipse total hasta el momento en que el Sol está total y completamente bloqueado por la Luna.Durante el breve período de tiempo en que la Luna oscurece por completo al Sol, el llamado período de totalidad, es seguro mirar directamente al astro rey, pero es crucial que sepas cuándo desviar la vista y volver a ponerte los lentes de eclipse.Primero, lo más importante: busca información local sobre el momento en que comenzará y terminará el eclipse total.Segundo: el Sol también proporciona pistas importantes sobre cuándo la totalidad está a punto de comenzar y terminar. || ",
"release_date": "2020-12-10T14:00:00-05:00",
"update_date": "2023-05-03T13:44:25.771707-04:00",
"main_image": {
"id": 380720,
"url": "https://svs.gsfc.nasa.gov/vis/a010000/a013600/a013668/EclipseSafetyVideo_Spanish.00140_print.jpg",
"filename": "EclipseSafetyVideo_Spanish.00140_print.jpg",
"media_type": "Image",
"alt_text": "Mira este video en el canal de YouTube en español de la NASA.Créditos de Música: “Perfect Horizon” por Sam Joseph Delves [PRS] de Universal Production Music",
"width": 1024,
"height": 576,
"pixels": 589824
}
},
{
"id": 12147,
"url": "https://svs.gsfc.nasa.gov/12147/",
"page_type": "Produced Video",
"title": "2016 Eclipse",
"description": "Solar scientists Natchimuthuk Gopalswamy, Nelson Reginal, Eric Christian, and Sarah Jaeggli discuss the 2016 eclipse and how it is great preparation for the 2017 eclipse.Complete transcript available. || eclipse_promo_thumb.jpg (1280x720) [53.1 KB] || eclipse_promo_thumb_searchweb.png (320x180) [69.9 KB] || eclipse_promo_thumb_thm.png (80x40) [12.8 KB] || YOUTUBE_HQ_12147_2016.eclipse_promo_V2_youtube_hq.mov (1920x1080) [534.5 MB] || PRORES_B-ROLL_12147_2016.eclipse_promo_V2_prores.mov (1280x720) [1.5 GB] || APPLE_TV_12147_2016.eclipse_promo_V2_appletv.m4v (1280x720) [63.3 MB] || NASA_TV_12147_2016.eclipse_promo_V2.mpeg (1280x720) [383.5 MB] || 12147_2016.eclipse_promo_V2.mov (1920x1080) [2.7 GB] || YOUTUBE_HQ_12147_2016.eclipse_promo_V2_youtube_hq.webm (1920x1080) [11.6 MB] || APPLE_TV_12147_2016.eclipse_promo_V2_appletv_subtitles.m4v (1280x720) [63.4 MB] || 12147_2016_eclipse_PROMO.en_US.srt [2.0 KB] || 12147_2016_eclipse_PROMO.en_US.vtt [2.0 KB] || NASA_PODCAST_12147_2016.eclipse_promo_V2_ipod_sm.mp4 (320x240) [21.4 MB] || ",
"release_date": "2016-03-03T10:00:00-05:00",
"update_date": "2023-05-03T13:48:50.523148-04:00",
"main_image": {
"id": 427218,
"url": "https://svs.gsfc.nasa.gov/vis/a010000/a012100/a012147/eclipse_promo_thumb.jpg",
"filename": "eclipse_promo_thumb.jpg",
"media_type": "Image",
"alt_text": "Solar scientists Natchimuthuk Gopalswamy, Nelson Reginal, Eric Christian, and Sarah Jaeggli discuss the 2016 eclipse and how it is great preparation for the 2017 eclipse.Complete transcript available.",
"width": 1280,
"height": 720,
"pixels": 921600
}
}
],
"newer_versions": [],
"older_versions": [],
"alternate_versions": []
}