apod api
1.0.0
Un microservicio escrito en Python con el micro framework Flask.
El código se reorganizó para que funcione más fácilmente en el servicio Elastic Beanstalk de AWS.
Los cambios con respecto a la versión anterior fueron:
Puede encontrar una versión congelada del código anterior en la rama llamada "prevCodeOrganization".
Una gran cantidad de personas utilizan la instancia de esta API que la NASA ha creado. Si necesita una versión extremadamente confiable de esta API, probablemente desee crear su propia versión de la API. ¡Puedes hacerlo con este código! Toda la información que devuelve esta API en realidad se obtiene del sitio web de Fotografía astronómica del día (APOD).
Nadie que vea este repositorio tiene nada que ver con el sitio web de Foto astronómica del día, por lo que no podemos ocuparnos de problemas directamente relacionados con su contenido. Por favor contáctelos directamente.
virtualenvcondagit clone https://github.com/nasa/apod-apicd en el nuevo directorio cd apod-apilib del proyecto. pip install -r requirements.txt -t liblib a su PYTHONPATH y ejecute el servidor PYTHONPATH=./lib python application.pyvirtualenvgit clone https://github.com/nasa/apod-apicd en el nuevo directorio cd apod-apienv en el directorio python -m venv venv. v env S cripts A ctivatepip install -r requirements.txtpython application.pycondagit clone https://github.com/nasa/apod-apicd en el nuevo directorio cd apod-apienv en el directorio conda create --prefix ./envconda activate ./envpip install -r requirements.txtpython application.pygit clone https://github.com/nasa/apod-api.gitcd en el nuevo directorio cd apod-apidocker build . -t apod-apidocker run -p 5000:5000 apod-api/<version>/apodSolo hay un punto final en este servicio que toma 2 campos opcionales como parámetros para una solicitud http GET. Se devuelve nominalmente un diccionario JSON.
api_key | demostración: DEMO_KEY | https://api.nasa.gov/#signUpdate Una cadena en formato AAAA-MM-DD que indica la fecha de la imagen APOD (ejemplo: 2014-11-03). El valor predeterminado es la fecha de hoy. Debe ser posterior al 16 de junio de 1995, el primer día en que se publicó una foto APOD. No hay imágenes para mañana disponibles a través de esta API.concept_tags Un valor booleano True|False que indica si las etiquetas conceptuales deben devolverse con el resto de la respuesta. Las etiquetas de concepto no necesariamente se incluyen en la explicación, sino que se derivan de etiquetas de búsqueda comunes que están asociadas con el texto de descripción. (Mejor que una simple búsqueda de texto). El valor predeterminado es Falso.hd Un parámetro booleano True|False que indica si se deben devolver o no imágenes de alta resolución. Esto está presente para fines heredados, el servicio siempre lo ignora y de todos modos se devuelven URL de alta resolución.count Un número entero positivo, no mayor que 100. Si se especifica esto, count las imágenes elegidas al azar se devolverán en una matriz JSON. No se puede utilizar junto con date o start_date y end_date .start_date Una cadena en formato AAAA-MM-DD que indica el inicio de un rango de fechas. Todas las imágenes en el rango desde start_date hasta end_date se devolverán en una matriz JSON. No se puede utilizar con date .end_date Una cadena en formato AAAA-MM-DD que indica el final de un rango de fechas. Si se especifica start_date sin end_date , entonces end_date por defecto es la fecha actual.thumbs Un parámetro booleano True|False que indica si la API debe devolver una URL de imagen en miniatura para archivos de vídeo. Si se establece en True , la API devuelve la URL de la miniatura del vídeo. Si un APOD no es un vídeo, este parámetro se ignora.Campos devueltos
resource Un diccionario que describe el image_set o planet que ilustra la respuesta, completamente determinado por el punto final estructurado.concept_tags Un reflejo booleano de la opción proporcionada. Incluido en la respuesta debido a los valores predeterminados.title El título de la imagen.date Fecha de la imagen. Incluido en la respuesta debido a los valores predeterminados.url La URL de la imagen o vídeo APOD del día.hdurl La URL de cualquier imagen de alta resolución de ese día. Se devuelve independientemente de la configuración del parámetro 'hd', pero se omitirá en la respuesta SI no existe originalmente en APOD.media_type El tipo de medio (datos) devuelto. Puede ser "imagen" o "video" según el contenido.explanation La explicación en texto proporcionada de la imagen.concepts Los conceptos más relevantes dentro de la explicación del texto. Solo se proporciona si concept_tags está establecido en True.thumbnail_url La URL de la miniatura del vídeo.copyright El nombre del titular de los derechos de autor.service_version La versión del servicio utilizada.Ejemplo
localhost:5000/v1/apod ? api_key=DEMO_KEY & date=2014-10-01 & concept_tags=True{
resource : {
image_set : "apod"
},
concept_tags : "True" ,
date : "2013-10-01" ,
title : "Filaments of the Vela Supernova Remnant" ,
url : "http://apod.nasa.gov/apod/image/1310/velafilaments_jadescope_960.jpg" ,
explanation : "The explosion is over but the consequences continue. About eleven
thousand years ago a star in the constellation of Vela could be seen to explode,
creating a strange point of light briefly visible to humans living near the
beginning of recorded history. The outer layers of the star crashed into the
interstellar medium, driving a shock wave that is still visible today. A roughly
spherical, expanding shock wave is visible in X-rays. The above image captures some
of that filamentary and gigantic shock in visible light. As gas flies away from the
detonated star, it decays and reacts with the interstellar medium, producing light
in many different colors and energy bands. Remaining at the center of the Vela
Supernova Remnant is a pulsar, a star as dense as nuclear matter that rotates
completely around more than ten times in a single second." ,
concepts : {
0 : "Astronomy" ,
1 : "Star" ,
2 : "Sun" ,
3 : "Milky Way" ,
4 : "Hubble Space Telescope" ,
5 : "Earth" ,
6 : "Nebula" ,
7 : "Interstellar medium"
}
}https://api.nasa.gov/planetary/apod ? api_key=DEMO_KEY & count=5[
{
"copyright" : "Panther Observatory" ,
"date" : "2006-04-15" ,
"explanation" : "In this stunning cosmic vista, galaxy M81 is on the left surrounded by blue spiral arms. On the right marked by massive gas and dust clouds, is M82. These two mammoth galaxies have been locked in gravitational combat for the past billion years. The gravity from each galaxy dramatically affects the other during each hundred million-year pass. Last go-round, M82's gravity likely raised density waves rippling around M81, resulting in the richness of M81's spiral arms. But M81 left M82 with violent star forming regions and colliding gas clouds so energetic the galaxy glows in X-rays. In a few billion years only one galaxy will remain." ,
"hdurl" : "https://apod.nasa.gov/apod/image/0604/M81_M82_schedler_c80.jpg" ,
"media_type" : "image" ,
"service_version" : "v1" ,
"title" : "Galaxy Wars: M81 versus M82" ,
"url" : "https://apod.nasa.gov/apod/image/0604/M81_M82_schedler_c25.jpg"
},
{
"date" : "2013-07-22" ,
"explanation" : "You are here. Everyone you've ever known is here. Every human who has ever lived -- is here. Pictured above is the Earth-Moon system as captured by the Cassini mission orbiting Saturn in the outer Solar System. Earth is the brighter and bluer of the two spots near the center, while the Moon is visible to its lower right. Images of Earth from Saturn were taken on Friday. Quickly released unprocessed images were released Saturday showing several streaks that are not stars but rather cosmic rays that struck the digital camera while it was taking the image. The above processed image was released earlier today. At nearly the same time, many humans on Earth were snapping their own pictures of Saturn. Note: Today's APOD has been updated." ,
"hdurl" : "https://apod.nasa.gov/apod/image/1307/earthmoon2_cassini_946.jpg" ,
"media_type" : "image" ,
"service_version" : "v1" ,
"title" : "Earth and Moon from Saturn" ,
"url" : "https://apod.nasa.gov/apod/image/1307/earthmoon2_cassini_960.jpg"
},
{
"copyright" : "Joe Orman" ,
"date" : "2000-04-06" ,
"explanation": "Rising before the Sun on February 2nd, astrophotographer Joe Orman anticipated this apparition of the bright morning star Venus near a lovely crescent Moon above a neighbor's house in suburban Phoenix, Arizona, USA. Fortunately, the alignment of bright planets and the Moon is one of the most inspiring sights in the night sky and one that is often easy to enjoy and share without any special equipment. Take tonight, for example. Those blessed with clear skies can simply step outside near sunset and view a young crescent Moon very near three bright planets in the west Jupiter, Mars, and Saturn. Jupiter will be the unmistakable brightest star near the Moon with a reddish Mars just to Jupiter's north and pale yellow Saturn directly above. Of course, these sky shows create an evocative picture but the planets and Moon just appear to be near each other -- they are actually only approximately lined up and lie in widely separated orbits. Unfortunately, next month's highly publicized alignment of planets on May 5th will be lost from view in the Sun's glare but such planetary alignments occur repeatedly and pose no danger to planet Earth.",
"hdurl" : "https://apod.nasa.gov/apod/image/0004/vm_orman_big.jpg" ,
"media_type" : "image" ,
"service_version" : "v1" ,
"title" : "Venus, Moon, and Neighbors" ,
"url" : "https://apod.nasa.gov/apod/image/0004/vm_orman.jpg"
},
{
"date" : "2014-07-12" ,
"explanation": "A new star, likely the brightest supernova in recorded human history, lit up planet Earth's sky in the year 1006 AD. The expanding debris cloud from the stellar explosion, found in the southerly constellation of Lupus, still puts on a cosmic light show across the electromagnetic spectrum. In fact, this composite view includes X-ray data in blue from the Chandra Observatory, optical data in yellowish hues, and radio image data in red. Now known as the SN 1006 supernova remnant, the debris cloud appears to be about 60 light-years across and is understood to represent the remains of a white dwarf star. Part of a binary star system, the compact white dwarf gradually captured material from its companion star. The buildup in mass finally triggered a thermonuclear explosion that destroyed the dwarf star. Because the distance to the supernova remnant is about 7,000 light-years, that explosion actually happened 7,000 years before the light reached Earth in 1006. Shockwaves in the remnant accelerate particles to extreme energies and are thought to be a source of the mysterious cosmic rays.",
"hdurl" : "https://apod.nasa.gov/apod/image/1407/sn1006c.jpg" ,
"media_type" : "image" ,
"service_version" : "v1" ,
"title" : "SN 1006 Supernova Remnant" ,
"url" : "https://apod.nasa.gov/apod/image/1407/sn1006c_c800.jpg"
},
{
"date" : "1997-01-21" ,
"explanation": "In Jules Verne's science fiction classic A Journey to the Center of the Earth, Professor Hardwigg and his fellow explorers encounter many strange and exciting wonders. What wonders lie at the center of our Galaxy? Astronomers now know of some of the bizarre objects which exist there, like vast dust clouds,r bright young stars, swirling rings of gas, and possibly even a large black hole. Much of the Galactic center region is shielded from our view in visible light by the intervening dust and gas. But it can be explored using other forms of electromagnetic radiation, like radio, infrared, X-rays, and gamma rays. This beautiful high resolution image of the Galactic center region in infrared light was made by the SPIRIT III telescope onboard the Midcourse Space Experiment. The center itself appears as a bright spot near the middle of the roughly 1x3 degree field of view, the plane of the Galaxy is vertical, and the north galactic pole is towards the right. The picture is in false color - starlight appears blue while dust is greenish grey, tending to red in the cooler areas.",
"hdurl" : "https://apod.nasa.gov/apod/image/9701/galcen_msx_big.gif" ,
"media_type" : "image" ,
"service_version" : "v1" ,
"title" : "Journey to the Center of the Galaxy rn Credit:" ,
"url" : "https://apod.nasa.gov/apod/image/9701/galcen_msx.jpg"
}
]https://api.nasa.gov/planetary/apod ? api_key=DEMO_KEY & start_date=2017-07-08 & end_date=2017-07-10[
{
"copyright" : "T. Rector" ,
"date" : "2017-07-08" ,
"explanation" : "Similar in size to large, bright spiral galaxies in our neighborhood, IC 342 is a mere 10 million light-years distant in the long-necked, northern constellation Camelopardalis. A sprawling island universe, IC 342 would otherwise be a prominent galaxy in our night sky, but it is hidden from clear view and only glimpsed through the veil of stars, gas and dust clouds along the plane of our own Milky Way galaxy. Even though IC 342's light is dimmed by intervening cosmic clouds, this sharp telescopic image traces the galaxy's own obscuring dust, blue star clusters, and glowing pink star forming regions along spiral arms that wind far from the galaxy's core. IC 342 may have undergone a recent burst of star formation activity and is close enough to have gravitationally influenced the evolution of the local group of galaxies and the Milky Way." ,
"hdurl" : "https://apod.nasa.gov/apod/image/1707/ic342_rector2048.jpg" ,
"media_type" : "image" ,
"service_version" : "v1" ,
"title" : "Hidden Galaxy IC 342" ,
"url" : "https://apod.nasa.gov/apod/image/1707/ic342_rector1024s.jpg"
},
{
"date" : "2017-07-09" ,
"explanation" : "Can you find your favorite country or city? Surprisingly, on this world-wide nightscape, city lights make this task quite possible. Human-made lights highlight particularly developed or populated areas of the Earth's surface, including the seaboards of Europe, the eastern United States, and Japan. Many large cities are located near rivers or oceans so that they can exchange goods cheaply by boat. Particularly dark areas include the central parts of South America, Africa, Asia, and Australia. The featured composite was created from images that were collected during cloud-free periods in April and October 2012 by the Suomi-NPP satellite, from a polar orbit about 824 kilometers above the surface, using its Visible Infrared Imaging Radiometer Suite (VIIRS)." ,
"hdurl" : "https://apod.nasa.gov/apod/image/1707/EarthAtNight_SuomiNPP_3600.jpg" ,
"media_type" : "image" ,
"service_version" : "v1" ,
"title" : "Earth at Night" ,
"url" : "https://apod.nasa.gov/apod/image/1707/EarthAtNight_SuomiNPP_1080.jpg"
},
{
"date" : "2017-07-10" ,
"explanation" : "What's happening around the center of this spiral galaxy? Seen in total, NGC 1512 appears to be a barred spiral galaxy -- a type of spiral that has a straight bar of stars across its center. This bar crosses an outer ring, though, a ring not seen as it surrounds the pictured region. Featured in this Hubble Space Telescope image is an inner ring -- one that itself surrounds the nucleus of the spiral. The two rings are connected not only by a bar of bright stars but by dark lanes of dust. Inside of this inner ring, dust continues to spiral right into the very center -- possibly the location of a large black hole. The rings are bright with newly formed stars which may have been triggered by the collision of NGC 1512 with its galactic neighbor, NGC 1510." ,
"hdurl" : "https://apod.nasa.gov/apod/image/1707/NGC1512_Schmidt_1342.jpg" ,
"media_type" : "image" ,
"service_version" : "v1" ,
"title" : "Spiral Galaxy NGC 1512: The Nuclear Ring" ,
"url" : "https://apod.nasa.gov/apod/image/1707/NGC1512_Schmidt_960.jpg"
}
]Si está volviendo a mostrar imágenes, es posible que desee verificar la presencia de derechos de autor. Todo lo que no tenga un campo de devolución de derechos de autor es generalmente de la NASA y de dominio público. Consulte la sección "Acerca de los permisos de imágenes" en el sitio principal de Foto astronómica del día para obtener más información.
El APOD Parser no forma parte de la API en sí. Más bien está pensado para acceder rápidamente a la API de APOD con Python sin tener que escribir mucho código adicional. Se encuentra en la carpeta apod_parser.
Primero importe el archivo apod_object_parser.py .
Ahora use la función get_data y pase su clave API como único argumento. Puede obtener la clave API aquí
response = apod_object_parser . get_data ( < your_api_key > ) -> apod_object_parser.get_date(response)
-> apod_object_parser.get_explaination(response)
-> apod_object_parser.get_hdurl(response)
-> apod_object_parser.get_media_type(response)
-> apod_object_parser.get_service_version(response)
-> apod_object_parser.get_title(response)
-> apod_object_parser.get_url(response)
para obtener documentos completos y más funciones, visite el archivo Léame del analizador apod haciendo clic aquí
La versión implementada de esta API se basa en la rama eb . La versión que se implementó antes está en la rama eb_previous . La rama master se utiliza como desarrollo ya que es allí donde entrarán la mayoría de las solicitudes de extracción.
Esta API se implementa en AWS mediante elastic beanstalk debido a la gran cantidad de personas que utilizan el servicio. Sin embargo, si planea usarlo usted mismo, es lo suficientemente pequeño como para colocarlo en un solo micro EC2 o en cualquier otra máquina informática en la nube de tamaño pequeño.
Destaque este repositorio si lo encontró útil. Utilice el rastreador de problemas de github para enviar comentarios sobre este repositorio.
Aceptamos solicitudes de extracción del público. Tenga en cuenta que podemos tardar en responder. Por favor tenga paciencia.
Además, las personas con derechos sobre este repositorio no son personas que puedan depurar problemas con el sitio web de APOD en sí . Si desea contribuir, ahora mismo nos vendría bien prestar atención a las pruebas.
