APOD API

What's this API for?

This API is for fetching data from NASA's APOD website - a popular service showing the most beautiful astronomical photographs in the world. The data is returned in JSON format and can be used for many applications, such as developing mobile apps for viewing APODs. My API is much faster, has no limit regarding dates and has more functions than the official one (eg. thumbnail_url value, returned while an APOD is a video).

How to deploy it?

Check out the project repository on GitHub

To test the API locally, clone the repository, install dependencies using npm install and then run the API using node index.js. The API will be running on localhost:3000.

To run on production server, check the server instructions (this process is different for servers based on Linux, Windows etc.)

How to use it?

The API is very easy to use, the syntax is similar to the official API. The API's endpoint is: /api/, the search function's endpoint is /search/ (search endpoint documentation here). Without any parameters, the API will return the latest APOD. You can specify parameters listed below.

Available query parameters:
Available query parameters for search endpoint:
Returned fields:

Examples

Example url: /api/

This query will return the latest available APOD, with no additional options:

{
   "apod_site":"https://apod.nasa.gov/apod/ap181027.html",
   "copyright":"Yuri Beletsky (Carnegie Las Campanas Observatory, TWAN)",
   "date":"2018-10-27",
   "description":"The best known asterism in northern skies hangs over the Canadian Rockies in this mountain and night skyscape taken last week from Banff National Park. But most remarkable is the amazing greenish airglow. With airglow visible to the eye, but not in color, the scene was captured in two exposures with a single camera, one exposure made while tracking the stars and one fixed to a tripod. Airglow emission is predominately from atmospheric oxygen atoms at extremely low densities. Commonly recorded in color by sensitive digital cameras the eerie, diffuse light is seen here in waves across the northern night. Originating at an altitude similar to aurorae, the luminous airglow is due to chemiluminescence, the production of light through chemical excitation and radiative decay. Energy for the chemical excitation is provided during daytime by the Sun's extreme ultraviolet radiation. Unlike aurorae which are limited to high latitudes, airglow can be found around the globe.",
   "hdurl":"https://apod.nasa.gov/apod/image/1810/airglow_banff_beletsky.jpg",
   "media_type":"image",
   "title":"Airglow Borealis",
   "url":"https://apod.nasa.gov/apod/image/1810/airglow_banff_beletsky1082.jpg"
}

Example url: /api/?date=2005-12-24&html_tags=true&image_thumbnail_size=450&absolute_thumbnail_url=true

This query will return APOD from Dec 24, 2005, with the original HTML tags in the text and with an absolute path to the 450px thumbnail of the image

{
   "apod_site":"https://apod.nasa.gov/apod/ap051224.html",
   "copyright":"Apollo 8, NASA",
   "date":"2005-12-24",
   "description":"In December of 1968, the <a href=\"http://www.lpi.usra.edu/expmoon/Apollo8/Apollo8.html\">Apollo 8</a> crew flew from the <a href=\"http://jv.gilead.org.il/pg/moon/\">Earth to the Moon</a> and back again. <a href=\"http://www.jsc.nasa.gov/Bios/htmlbios/borman-f.html\">Frank Borman</a>, <a href=\"http://www.jsc.nasa.gov/Bios/htmlbios/lovell-ja.html\">James Lovell</a>, and <a href=\"http://www.jsc.nasa.gov/Bios/htmlbios/anders-wa.html\">William Anders</a> were launched atop a <a href=\"http://www.apollosaturn.com/saturnv.htm\">Saturn V rocket</a> on December 21, circled the Moon ten times in their command module, and returned to Earth on December 27. The <a href=\"http://nssdc.gsfc.nasa.gov/database/MasterCatalog?sc=1968-118A\">Apollo 8</a> mission&apos;s impressive list of firsts includes: the first humans to journey to the <a href=\"http://www.nineplanets.org/luna.html\">Earth&apos;s Moon</a>, the first manned flight using the <a href=\"https://apod.nasa.gov/apod/ap010525.html\">Saturn V</a>, and the first <a href=\"http://www.lpi.usra.edu/expmoon/Apollo8/A08_Photography.html\">to photograph</a> the Earth from deep space. As the Apollo 8 command module rounded the farside of the Moon, the crew could look toward the <a href=\"https://apod.nasa.gov/apod/ap010713.html\">lunar horizon</a> and see the Earth appear to rise, due to their spacecraft&apos;s orbital motion. The <a href=\"http://www.abc.net.au/science/moon/earthrise.htm\">famous picture </a> that resulted, of a distant <a href=\"https://apod.nasa.gov/apod/ap030426.html\">blue Earth</a> above the Moon&apos;s limb, was a marvelous gift to the world.",
   "hdurl":"https://apod.nasa.gov/apod/image/0512/as8-14-2383HR.jpg",
   "image_thumbnail":"apod.api.example.com/image/?image=https://apod.nasa.gov/apod/image/0512/as8-14-2383c75.jpg&width=450",
   "media_type":"image",
   "title":"Earthrise",
   "url":"https://apod.nasa.gov/apod/image/0512/as8-14-2383c75.jpg"
}

Example url: /api/?start_date=2018-10-05&end_date=2018-10-10&thumbs=true&image_thumbnail_size=480&image_thumbnail_size=240

This query will return all the APODs between Oct 05, 2018 and Oct 10, 2018, with video thumbnails and 480 and 240 px thumbnails of the images:

[
   {
      "apod_site":"https://apod.nasa.gov/apod/ap181010.html",
      "copyright":"NASA, SDO; Processing: Alan Watson via Helioviewer",
      "date":"2018-10-10",
      "description":"Sometimes, the surface of our Sun seems to dance. In the middle of 2012, for example, NASA's Sun-orbiting Solar Dynamic Observatory spacecraft imaged an impressive prominence that seemed to perform a running dive roll like an acrobatic dancer. The dramatic explosion was captured in ultraviolet light in the featured time-lapse video covering about three hours. A looping magnetic field directed the flow of hot plasma on the Sun. The scale of the dancing prominence is huge -- the entire Earth would easily fit under the flowing arch of hot gas. A quiescent prominence typically lasts about a month, and may erupt in a Coronal Mass Ejection (CME) expelling hot gas into the Solar System. The energy mechanism that creates a solar prominence is still a topic of research. Unlike 2012, this year the Sun's surface is significantly more serene, featuring fewer spinning prominences, as it is near the minimum in its 11-year magnetic cycle.",
      "image_thumbnail":[
         "image/?image=https://img.youtube.com/vi/hQFEHH5E69s/0.jpg&width=480",
         "image/?image=https://img.youtube.com/vi/hQFEHH5E69s/0.jpg&width=240"
      ],
      "media_type":"video",
      "thumbnail_url":"https://img.youtube.com/vi/hQFEHH5E69s/0.jpg",
      "title":"Sun Dance",
      "url":"https://www.youtube.com/embed/hQFEHH5E69s?rel=0"
   },
   {
      "apod_site":"https://apod.nasa.gov/apod/ap181009.html",
      "copyright":"Hubble Legacy Archive, NASA, ESA; Processing &  Domingo Pestana & Raul Villaverde",
      "date":"2018-10-09",
      "description":"Many spiral galaxies have bars across their centers. Even our own Milky Way Galaxy is thought to have a modest central bar. Prominently barred spiral galaxy NGC 1672, featured here, was captured in spectacular detail in an image taken by the orbiting Hubble Space Telescope. Visible are dark filamentary dust lanes, young clusters of bright blue stars, red emission nebulas of glowing hydrogen gas, a long bright bar of stars across the center, and a bright active nucleus that likely houses a supermassive black hole. Light takes about 60 million years to reach us from NGC 1672, which spans about 75,000 light years across. NGC 1672, which appears toward the constellation of the Dolphinfish (Dorado), is being studied to find out how a spiral bar contributes to star formation in a galaxy's central regions.",
      "hdurl":"https://apod.nasa.gov/apod/image/1810/NGC1672_Hubble_3600.jpg",
      "image_thumbnail":[
         "image/?image=https://apod.nasa.gov/apod/image/1810/NGC1672_Hubble_1080.jpg&width=480",
         "image/?image=https://apod.nasa.gov/apod/image/1810/NGC1672_Hubble_1080.jpg&width=240"
      ],
      "media_type":"image",
      "title":"NGC 1672: Barred Spiral Galaxy from Hubble",
      "url":"https://apod.nasa.gov/apod/image/1810/NGC1672_Hubble_1080.jpg"
   },
   {
      "apod_site":"https://apod.nasa.gov/apod/ap181008.html",
      "copyright":"Fritz Helmut Hemmerich",
      "date":"2018-10-08",
      "description":"Small bits of this greenish-gray comet are expected to streak across Earth's atmosphere tonight. Specifically, debris from the eroding nucleus of Comet 21P / Giacobini-Zinner, pictured, causes the annual Draconids meteor shower, which peaks this evening. Draconid meteors are easy to enjoy this year because meteor rates will likely peak soon after sunset with the Moon's glare nearly absent. Patience may be needed, though, as last month's passing of 21P near the Earth's orbit is not expected to increase the Draconids' normal meteor rate this year of (only) a few meteors per hour. Then again, meteor rates are notoriously hard to predict, and the Draconids were quite impressive in 1933, 1946, and 2011. Featured, Comet 21P gracefully posed between the Rosette (upper left) and Cone (lower right) nebulas two weeks ago before heading back out to near the orbit of Jupiter, to return again in about six and a half years.",
      "hdurl":"https://apod.nasa.gov/apod/image/1810/Comet21P_Hemmerich_1440.jpg",
      "image_thumbnail":[
         "image/?image=https://apod.nasa.gov/apod/image/1810/Comet21P_Hemmerich_960.jpg&width=480",
         "image/?image=https://apod.nasa.gov/apod/image/1810/Comet21P_Hemmerich_960.jpg&width=240"
      ],
      "media_type":"image",
      "title":"Comet 21P Between Rosette and Cone Nebulas",
      "url":"https://apod.nasa.gov/apod/image/1810/Comet21P_Hemmerich_960.jpg"
   },
   {
      "apod_site":"https://apod.nasa.gov/apod/ap181007.html",
      "copyright":"Cary & Michael Huang",
      "date":"2018-10-07",
      "description":"What does the universe look like on small scales? On large scales? Humanity is discovering that the universe is a very different place on every proportion that has been explored. For example, so far as we know, every tiny proton is exactly the same, but every huge galaxy is different. On more familiar scales, a small glass table top to a human is a vast plane of strange smoothness to a dust mite -- possibly speckled with cell boulders. Not all scale lengths are well explored -- what happens to the smallest mist droplets you sneeze, for example, is a topic of active research -- and possibly useful to know to help stop the spread of disease. The featured interactive flash animation, a modern version of the classic video Powers of Ten, is a new window to many of the known scales of our universe. By moving the scroll bar across the bottom, you can explore a diversity of sizes, while clicking on different items will bring up descriptive information.",
      "media_type":"other",
      "title":"The Scale of the Universe - Interactive"
   },
   {
      "apod_site":"https://apod.nasa.gov/apod/ap181006.html",
      "copyright":"Mia Stalnacke",
      "date":"2018-10-06",
      "description":"What does an aurora look like to a frog? \"Awesome!\" is the likely answer, suggested by this imaginative snapshot taken on October 3rd from Kiruna, Sweden. Frequented by apparitions of the northern lights, Kiruna is located in Lapland north of the Arctic Circle, and often under the auroral oval surrounding planet Earth's geomagnetic north pole. To create a tantalizing view from a frog's perspective the photographer turned on the flashlight on her phone and placed it on the ground facing down, resting her camera's lens on top. The \"diamonds\" in the foreground are icy pebbles right in front of the lens, lit up by the flashlight. Reflecting the shimmering northern lights, the \"lake\" is a frozen puddle on the ground. Of course, in the distance is the Bengt Hultqvist Observatory.",
      "hdurl":"https://apod.nasa.gov/apod/image/1810/AuroraFrogStalnacke3072.jpg",
      "image_thumbnail":[
         "image/?image=https://apod.nasa.gov/apod/image/1810/AuroraFrogStalnacke1024.jpg&width=480",
         "image/?image=https://apod.nasa.gov/apod/image/1810/AuroraFrogStalnacke1024.jpg&width=240"
      ],
      "media_type":"image",
      "title":"Aurora: The Frog's View",
      "url":"https://apod.nasa.gov/apod/image/1810/AuroraFrogStalnacke1024.jpg"
   },
   {
      "apod_site":"https://apod.nasa.gov/apod/ap181005.html",
      "copyright":"Radu-Mihai Anghel",
      "date":"2018-10-05",
      "description":"That's not a young crescent Moon poised above the hills along the western horizon at sunset. It's Venus in a crescent phase. About 54 million kilometers away and less than 20 percent illuminated, it was captured by telescope and camera on September 30 near Bacau, Romania. The bright celestial beacon is now languishing in the evening twilight, its days as the Evening Star in 2018 coming to a close. But it also grows larger in apparent size and becomes an ever thinner crescent in telescopic views. Heading toward an inferior conjunction (non-judgmental), the inner planet will be positioned between Earth and Sun on October 26 and lost from view in the solar glare. At month's end a crescent Venus will reappear in the east though, rising just before the Sun as the brilliant Morning Star.",
      "hdurl":"https://apod.nasa.gov/apod/image/1810/Venus_Radu-Mihai_MG_3429.jpg",
      "image_thumbnail":[
         "image/?image=https://apod.nasa.gov/apod/image/1810/Venus_Radu-Mihai_MG_3429_1067px.jpg&width=480",
         "image/?image=https://apod.nasa.gov/apod/image/1810/Venus_Radu-Mihai_MG_3429_1067px.jpg&width=240"
      ],
      "media_type":"image",
      "title":"The Last Days of Venus as the Evening Star",
      "url":"https://apod.nasa.gov/apod/image/1810/Venus_Radu-Mihai_MG_3429_1067px.jpg"
   }
]

Example url: /search/?search_query=planetary%20nebula&number=5&page=2

This query will return 2nd page of 5 APODs that match the query planetary nebula:

[
   {
      "apod_site":"https://apod.nasa.gov/apod/ap180417.html",
      "copyright":"NASA, ESA, Hubble Legacy Archive; Composition: Giuseppe Donatiello",
      "date":"2018-04-17",
      "description":"Except for the rings of Saturn, the Ring Nebula (M57) is probably the most famous celestial band. Its classic appearance is understood to be due to our own perspective, though. The recent mapping of the expanding nebula's 3-D structure, based in part on this clear Hubble image,indicates that the nebula is a relatively dense, donut-like ring wrapped around the middle of a (American) football-shaped cloud of glowing gas. The view from planet Earth looks down the long axis of the football, face-on to the ring. Of course, in this well-studied example of a planetary nebula, the glowing material does not come from planets. Instead, the gaseous shroud represents outer layers expelled from the dying, once sun-like star, now a tiny pinprick of light seen at the nebula's center. Intense ultraviolet light from the hot central star ionizes atoms in the gas. The Ring Nebula is about one light-year across and 2,000 light-years away.",
      "hdurl":"https://apod.nasa.gov/apod/image/1804/Ring_HubbleDonatiello_3251.jpg",
      "media_type":"image",
      "title":"M57: The Ring Nebula",
      "url":"https://apod.nasa.gov/apod/image/1804/Ring_HubbleDonatiello_960.jpg"
   },
   {
      "apod_site":"https://apod.nasa.gov/apod/ap180109.html",
      "copyright":"Hubble, NASA, ESA; Processing & License: Judy Schmidt",
      "date":"2018-01-09",
      "description":"It is one of the brightest planetary nebulae on the sky -- what should it be named? First discovered in 1878, nebula NGC 7027 can be seen toward the constellation of the Swan (Cygnus) with a standard backyard telescope. Partly because it appears there as only an indistinct spot, it is rarely referred to with a moniker. When imaged with the Earth-orbiting Hubble Space Telescope, however, great details are revealed. Studying Hubble images of NGC 7027 have led to the understanding that it is a planetary nebula that began expanding about 600 years ago, and that the cloud of gas and dust is unusually massive as it appears to contain about three times the mass of our Sun. Pictured here in assigned colors, the resolved, layered, and dust-laced features of NGC 7027 might remind sky enthusiasts of a familiar icon that could be the basis for an informal name. A leading previous suggestion was the Pillow Nebula, but please feel free to make new suggestions -- for example, in an online APOD discussion forum.",
      "hdurl":"https://apod.nasa.gov/apod/image/1801/NGC7027_HubbleSchmidt_960.jpg",
      "media_type":"image",
      "title":"Bright Planetary Nebula NGC 7027 from Hubble",
      "url":"https://apod.nasa.gov/apod/image/1801/NGC7027_HubbleSchmidt_960.jpg"
   },
   {
      "apod_site":"https://apod.nasa.gov/apod/ap180103.html",
      "copyright":"CFHT, Coelum, MegaCam, J.-C. Cuillandre (CFHT) & G. A. Anselmi (Coelum)",
      "date":"2018-01-03",
      "description":"Will our Sun look like this one day? The Helix Nebula is one of brightest and closest examples of a planetary nebula, a gas cloud created at the end of the life of a Sun-like star. The outer gasses of the star expelled into space appear from our vantage point as if we are looking down a helix. The remnant central stellar core, destined to become a white dwarf star, glows in light so energetic it causes the previously expelled gas to fluoresce. The Helix Nebula, given a technical designation of NGC 7293, lies about 700 light-years away towards the constellation of the Water Bearer (Aquarius) and spans about 2.5 light-years. The featured picture was taken with the Canada-France-Hawaii Telescope (CFHT) located atop a dormant volcano in Hawaii, USA. A close-up of the inner edge of the Helix Nebula shows complex gas knots of unknown origin.",
      "hdurl":"https://apod.nasa.gov/apod/image/1801/Helix_CFHT_2000.jpg",
      "media_type":"image",
      "title":"The Helix Nebula from CFHT",
      "url":"https://apod.nasa.gov/apod/image/1801/Helix_CFHT_960.jpg"
   },
   {
      "apod_site":"https://apod.nasa.gov/apod/ap171028.html",
      "copyright":"Image  Hubble Heritage Team, NASA",
      "date":"2017-10-28",
      "description":"Wraithlike NGC 6369 is a faint apparition in night skies popularly known as the Little Ghost Nebula. It was discovered by 18th century astronomer Sir William Herschel as he used a telescope to explore the medicinal constellation Ophiucus. Herschel historically classified the round and planet-shaped nebula as a Planetary Nebula. But planetary nebulae in general are not at all related to planets. Instead they are gaseous shrouds created at the end of a sun-like star's life, the dying star's outer layers expanding into space while its core shrinks to become a white dwarf. The transformed white dwarf star, seen near the center, radiates strongly at ultraviolet wavelengths and powers the expanding nebula's glow. Surprisingly complex details and structures of NGC 6369 are revealed in this tantalizing image composed from Hubble Space Telescope data. The nebula's main round structure is about a light-year across and the glow from ionized oxygen, hydrogen, and nitrogen atoms are colored blue, green, and red respectively. Over 2,000 light-years away, the Little Ghost Nebula offers a glimpse of the fate of our Sun, which could produce its own planetary nebula about 5 billion years from now.",
      "hdurl":"https://apod.nasa.gov/apod/image/1710/NGC6369LittleGhostHST.jpg",
      "media_type":"image",
      "title":"NGC 6369: The Little Ghost Nebula",
      "url":"https://apod.nasa.gov/apod/image/1710/NGC6369LittleGhostHST1024c.jpg"
   },
   {
      "apod_site":"https://apod.nasa.gov/apod/ap170611.html",
      "copyright":"NASA, ESA, and the Hubble Heritage Team (STScI/AURA); Acknowledgement: R. Sahai (JPL) et al.",
      "date":"2017-06-11",
      "description":"What is creating the strange texture of IC 418? Dubbed the Spirograph Nebula for its resemblance to drawings from a cyclical drawing tool, planetary nebula IC 418 shows patterns that are not well understood. Perhaps they are related to chaotic winds from the variable central star, which changes brightness unpredictably in just a few hours. By contrast, evidence indicates that only a few million years ago, IC 418 was probably a well-understood star similar to our Sun. Only a few thousand years ago, IC 418 was probably a common red giant star. Since running out of nuclear fuel, though, the outer envelope has begun expanding outward leaving a hot remnant core destined to become a white-dwarf star, visible in the image center. The light from the central core excites surrounding atoms in the nebula causing them to glow. IC 418 lies about 2000 light-years away and spans 0.3 light-years across. This false-color image taken from the Hubble Space Telescope reveals the unusual details.",
      "hdurl":"https://apod.nasa.gov/apod/image/1706/Spirograph_Hubble_2119.jpg",
      "media_type":"image",
      "title":"IC 418: The Spirograph Nebula",
      "url":"https://apod.nasa.gov/apod/image/1706/Spirograph_Hubble_960.jpg"
   }
]

Example url: /api/?count=5

This query will return 5 random APODs:

[
   {
      "apod_site": "https://apod.nasa.gov/apod/ap091016.html",
      "copyright": "ESA, SPIRE & PACS Consortia",
      "date": "2009-10-16",
      "description": "With a 3.5 meter diameter mirror, larger than the Hubble Space Telescope, Herschel is ESA's new infrared observatory. The space-based telescope is named for German-born British astronomer Frederick William Herschel who discovered infrared light over 200 years ago. In initial tests, Herschel's cameras have combined to deliver this spectacular view along the plane of the Milky Way in the constellation of the Southern Cross. Spanning some 2 degrees the premier, false-color, far-infrared view captures our galaxy's cold dust clouds in extreme detail, showing a remarkable, connected maze of filaments and star-forming regions. These and planned future Herschel observations are intended to unravel mysteries of star formation by surveying broad areas of the galactic plane.",
      "hdurl": "https://apod.nasa.gov/apod/image/0910/FirstParallelMode_SPIRE_PACS.jpg",
      "media_type": "image",
      "title": "Herschel Views the Milky Way",
      "url": "https://apod.nasa.gov/apod/image/0910/FirstParallelMode_SPIRE_PACS_c900.jpg"
   },
   {
      "apod_site": "https://apod.nasa.gov/apod/ap091125.html",
      "copyright": "Axel Mellinger (Central Mich. U)",
      "date": "2009-11-25",
      "description": "If you could go far away from the Earth and look around the entire sky -- what would you see? Such was the goal of the All-Sky Milky Way Panorama 2.0 project of Axel Mellinger. Presented above is the result: a digital compilation of over 3,000 images comprising the highest resolution digital panorama of the entire night sky yet created. An interactive zoom version, featuring over 500 million pixels, can be found here. Every fixed astronomical object visible to the unaided eye has been imaged, including every constellation, every nebula, and every star cluster. Moreover, millions of individual stars are also visible, all in our Milky Way Galaxy, and many a thousand times fainter than a human can see. Dark filaments of dust lace the central band of our Milky Way Galaxy, visible across the image center. The satellite galaxies Large and Small Magellanic Clouds are visible on the lower right. This was not the first time Dr. Mellinger has embarked on such a project: the results of his first All-Sky Milky Way Panorama Project, taken using photographic film, are visible here.",
      "hdurl": "https://apod.nasa.gov/apod/image/0911/mwpan_mellinger_big.jpg",
      "media_type": "image",
      "title": "All-Sky Milky Way Panorama",
      "url": "https://apod.nasa.gov/apod/image/0911/mwpan_mellinger.jpg"
   },
   {
      "apod_site": "https://apod.nasa.gov/apod/ap971017.html",
      "copyright": "MGS Project, JPL, NASA",
      "date": "1997-10-17",
      "description": "An icy mist and late afternoon clouds cover much of this section of Valles Marineris on Mars. The Valles Marineris or Mariner Valley is a huge canyon system about 2,000 miles long and up to 5 miles deep. This test image was produced using data from Mars Global Surveyor's wide angle cameras viewing the canyon from a distance of 360-600 miles. Color was synthesized using images recorded through blue and red filters. Mission controllers have recently raised the spacecraft's aerobraking orbit to study the unexpected motion of one of the Surveyor's solar panels.",
      "hdurl": "https://apod.nasa.gov/apod/image/9710/marval1_mgs_big.jpg",
      "media_type": "image",
      "title": "Mars: A Mist In Mariner Valley",
      "url": "https://apod.nasa.gov/apod/image/9710/marval1_mgs.jpg"
   },
   {
      "apod_site": "https://apod.nasa.gov/apod/ap950928.html",
      "copyright": "NASA, JPL Magellan Project",
      "date": "1995-09-28",
      "description": "This computer generated view of a Venusian volcano was created using data from NASA's Magellan spacecraft. Magellan used its onboard radar to map the surface of Venus which is hidden from telescopic observations by a perpetual cloud cover. Using this radar data to provide three dimensional information, a computer was then able to produce this view of Maat Mons, a 5 mile high volcano, from a dramatic perspective. The colors used to render the surface are based on earlier color images transmitted by TV cameras on the Soviet Venera 13 and 14 Venus landers.",
      "hdurl": "https://apod.nasa.gov/apod/image/maat_mons.gif",
      "media_type": "image",
      "title": "A Venusian Landscape",
      "url": "https://apod.nasa.gov/apod/image/maat_mons.gif"
   },
   {
      "apod_site": "https://apod.nasa.gov/apod/ap131217.html",
      "copyright": "Juan Carlos Casado (TWAN, Earth and Stars)",
      "date": "2013-12-17",
      "description": "On some nights it rains meteors. Peaking two nights ago, asteroid dust streaked through the dark skies of Earth, showering down during the annual Geminids meteor shower. Astrophotographer Juan Carlos Casado captured the space weather event, as pictured above, in a series of exposures spanning about 2.3 hours using a wide angle lens. The snowcapped Teide volcano of the Canary Islands of Spain towers in the foreground, while the picturesque constellation of Orion highlights the background. The star appearing just near the top of the volcano is Rigel. Although the asteroid dust particles are traveling parallel to each other, the resulting meteor streaks appear to radiate from a single point on the sky, in this case in the constellation of Gemini, off the top of the image. Like train tracks appearing to converge in the distance, the meteor radiant effect is due to perspective. The astrophotographer has estimated that there are about 50 Geminids visible in the above composite image -- how many do you see?",
      "hdurl": "https://apod.nasa.gov/apod/image/1312/geminds2013_jcc_1500.jpg",
      "media_type": "image",
      "title": "Geminid Meteors over Teide Volcano",
      "url": "https://apod.nasa.gov/apod/image/1312/geminds2013_jcc_960.jpg"
   }
]

Dependencies

Node.js JavaScript runtime

Express web framework

Request library

Cheerio library

Sharp library

iconv-lite library

Made by Pawel Pleskaczynski