Events in time

<?php

// Demo token. (Replace it with your token).
$token = '93a1f6fc-3fa2-40ee-9fae-0ff301df50f0';

//if there is no such date in the calendar, then error 404
$year = 1975; // from -13000000000 to 100000000000000000000000000000000000000000000000000
$month = 3; // from 1 to 12
$day = 13; // from 1 to 31 

$url = 'https://wildtracks.pro/api/time/'.$token.'/'.$year.'/'.$month.'/'.$day.'/';
// We receive confirmation via the LINK
$jsonData = file_get_contents($url);
// Checking if the data was received successfully
if ($jsonData === false) {
    die('Error receiving data from the URL');
}
// Converting JSON to an associative array
$dataArray = json_decode($jsonData, true);
// Checking if it was possible to convert JSON to an array
if ($dataArray === null) {
    die('Error decoding JSON');
}
// Output an array
echo "<pre>";
print_r($dataArray);
echo "</pre>";

?>

{
  "year": "1975",
  "leap year": "no",
  "month": "3",
  "Name of the month": {
    "Chinese": "三月",
    "Spanish": "Marzo",
    "English": "March",
    "Hindi": "मार्च",
    "Arab": "مارس",
    "Bengal": "মার্চ",
    "Portuguese": "Março",
    "Russian": "Март",
    "Japanese": "三月",
    "Lahnda": "مارچ",
    "Marathi": "मार्च",
    "Telugu": "మార్చి",
    "Malay": "Mac",
    "Turkish": "Mart",
    "Korean": "3월",
    "French": "Mars",
    "German": "März",
    "Vietnamese": "Tháng Ba",
    "Tamil": "மார்ச்",
    "Urdu": "مارچ",
    "Javanese": "Maret",
    "Italian": "Marzo",
    "Persian": "مارس",
    "Gujaratis": "માર્ચ"
  },
  "day": "13",
  "day of the week": 4,
  "Day of the week": {
    "Chinese": "星期四",
    "Spanish": "Jueves",
    "English": "Thursday",
    "Hindi": "गुरुवार",
    "Arab": "الخميس",
    "Bengal": "বৃহস্পতিবার",
    "Portuguese": "Quinta-feira",
    "Russian": "Четверг",
    "Japanese": "木曜日",
    "Lahnda": " جمعرات",
    "Marathi": "गुरुवार",
    "Telugu": "గురువారం",
    "Malay": "Khamis",
    "Turkish": "Perşembe",
    "Korean": "목요일",
    "French": "Jeudi",
    "German": "Donnerstag",
    "Vietnamese": "Thứ năm",
    "Tamil": "வியாழக்கிழமை",
    "Urdu": " جمعرات",
    "Javanese": "Kemis",
    "Italian": "Giovedì",
    "Persian": "پنج‌شنبه",
    "Gujaratis": "ગુરુવાર"
  },
  "Property of time": {
    "year": 49,
    "month": 6,
    "day": 16,
    "property": "Past"
  },
  "Era": "AD",
  "Description": [
    "Vietnam War: South Vietnam President Nguyen van Thieu orders the Central Highlands evacuated.   This turns into a mass exodus involving troops and civilians (the Convoy of Tears)."
  ],
  "this year": [
    "Altair 8800 is released, sparking the microputer revolution.",
    "Volkswagen introduces the Golf, its new front-wheel-drive economy car, in the United States and Canada as the Volkswagen Rabbit.",
    "Watergate scandal: John N. Mitchell, H. R. Haldeman and John Ehrlichman are found guilty of the Watergate cover-up.",
    "Malawi changes its capital city from Zomba to Lilongwe.",
    "The United States Patent and Trademark Office is renamed U.S. Patent and Trademark Office.",
    "The Federal Rules of Evidence are approved by the United States Congress.",
    "Bangladesh freedom fighter Shiraj Shikder was killed by country's president Sheikh Mujibur Rahman"
  ],
  "Era in history": [
    {
      "era": "Modern Era",
      "period": "Cold War",
      "start": "1947",
      "end": "1991"
    }
  ],
  "Periud": {
    "Australian": [
      {
        "description": "Second Elizabethan era",
        "start": "1952",
        "end": "2022"
      }
    ],
    "European periods": [
      {
        "description": "Cold War",
        "start": "1945",
        "end": "1991"
      }
    ],
    "Iranian periods": [
      {
        "description": "Pahlavi Iran",
        "start": "1925",
        "end": "1979"
      }
    ],
    "Japanese periods": [
      {
        "description": "Shōwa period",
        "start": "1926",
        "end": "1989"
      }
    ],
    "Libyan periods": [
      {
        "description": "Libyan Arab Republic",
        "start": "1969",
        "end": "1977"
      }
    ],
    "Mexican periods": [
      {
        "description": "PRI One-Party State",
        "start": "1934",
        "end": "2000"
      }
    ],
    "United States historical periods": [
      {
        "description": "Fifth Party System",
        "start": "1932",
        "end": "1980"
      }
    ]
  },
  "Stratigraphic scale": [
    {
      "generalgroup": null,
      "eonothem": "Phanerozoic",
      "erathem": "Cenozoic",
      "series": "Quaternary",
      "epoch": null,
      "stage": "Holocene",
      "age": "Meghalayan",
      "start": "-2250",
      "end": "2024",
      "details": [
        "The end of Egypt's Old Kingdom (around 2200 BCE).",
        "The fall of the Akkadian Empire in Mesopotamia.",
        "The end of the Old Kingdom in Egypt and the beginning of the First Intermediate Period.\r\n",
        "The rise of civilizations such as the Harappan civilization in the Indus Valley.",
        "The development of the Maya and other Mesoamerican cultures.",
        "The emergence and rise of the Shang Dynasty in China.",
        "The spread of bronze metallurgy and the beginning of the Iron Age in various regions of the world.",
        "The rise of city-states in Greece and the emergence of Greek civilization.",
        "The rise and fall of great empires such as Assyria, Babylon, and Persia.",
        "The emergence and flourishing of the Roman Empire, including the Roman Renaissance in the 3rd-5th centuries CE.",
        "The beginning and end of the Middle Ages, including the early, high, and late Middle Ages.",
        "The spread of world religions such as Christianity and Islam.",
        "The revival of interest in ancient heritage, scientific and cultural achievements of the Renaissance.",
        "The Age of Discovery in the 15th-17th centuries.",
        "The Industrial Revolution and the rise of capitalism.",
        "The great revolutions of the 18th-19th centuries, the formation of modern states.",
        "The World Wars, the Cold War, and globalization in the 20th century.",
        "The Information Age, the beginning of the digital era."
      ]
    }
  ],
  "Space": [
    {
      "description": "Evolution of galaxies and the formation of large structures",
      "start": "-12800000000",
      "end": "20000000000000",
      "details": [
        "The Evolution of Galaxies and the Formation of Large Structures is a stage in the history of the Universe that began after the completion of the Epoch of Reionization and continues to the present day. This process covers the time from approximately 12.8 billion years ago to now and includes the development of galaxies, the formation of galaxy clusters, and larger cosmic structures.",
        "Formation of the first galaxies: After the Epoch of Reionization, the Universe was filled with primordial galaxies that began to form from gas clouds created in the early Universe. These first galaxies, consisting of gas and stars, started to merge under the influence of gravity, forming more complex and larger structures.",
        "Growth and merging of galaxies: Gravitational attraction between galaxies led to their approaching and merging. This process contributed to the formation of larger galaxies and galactic groups. Over time, large clusters of galaxies formed, which began to create superclusters — the largest structures in the observable Universe.",
        "Formation of large cosmic structures: Through multiple mergers and interactions, complex structures such as galaxy clusters and superclusters formed. These structures organized themselves along gigantic filaments and threads of dark matter, creating a cosmic web where galaxies and galaxy clusters are aligned along \"filaments\" of dark matter, separated by vast voids.",
        "Current state: Today, the Universe is still expanding, and galaxies and their clusters continue to interact and evolve. Observations show that the large-scale structure of the Universe looks like a network of filaments and voids, with galaxies and their clusters unevenly distributed.\r\n\r\n",
        "Impact on development: The evolution of galaxies and the formation of large structures have had a significant impact on the development of star systems, planetary systems, and, ultimately, the formation of complex systems like our solar system and exoplanetary systems in other galaxies."
      ]
    },
    {
      "description": "Lifetime of the solar system",
      "start": "-4600000000",
      "end": "5000000000",
      "details": [
        "The Lifetime of the Solar System can be considered in terms of its formation, current state, and projected future. Here is a detailed overview of the key stages and the lifetime of the Solar System:",
        "Formation of the Solar System (~4.6 billion years ago): The Solar System began forming approximately 4.6 billion years ago from a protoplanetary disk of gas and dust surrounding the young Sun. This process involved the formation of the Sun, planets, moons, and other celestial bodies.",
        "Current Time (~4.6 billion years after formation): The Solar System is currently in a stable state where the Sun is on the main sequence of its stellar evolution. This stage, characterized by stable hydrogen fusion in the star's core, is expected to last for approximately another 5 billion years.",
        "Future of the Solar System:\r\nRed Giant Phase (~5 billion years from now): In about 5 billion years, the Sun will exhaust its hydrogen fuel and begin to expand, transforming into a red giant. This will lead to the expansion of its outer layers and possibly engulfing the inner planets, including Earth.",
        "Future of the Solar System:\r\nWhite Dwarf Period (~5.5 billion years from now): After the red giant phase, the Sun will shed its outer layers, leaving behind a hot core that will become a white dwarf. This white dwarf will gradually cool and fade over the subsequent billions of years.",
        "Future of the Solar System:\r\nCooling of the White Dwarf (over 10 billion years): The white dwarf will continue to cool and dim, eventually becoming a black dwarf. This process will take tens of billions of years.",
        "End of the Solar System's Life: At this point, predicting the exact moment when the entire Solar System will \"die\" or become inactive is challenging, as it depends on the long-term processes affecting the white dwarf and its remnants. However, it is likely that, in the timescale of the Universe, the Solar System will become a cold, dark object, existing in a state of near-total stasis."
      ]
    },
    {
      "description": "Life time planet earth",
      "start": "-4540000000",
      "end": "5000000000",
      "details": [
        "The lifetime of Planet Earth refers to the various stages and changes the planet will undergo from its formation to the point where it becomes uninhabitable. This timeline encompasses its early development, stable habitable phase, and eventual transition to an inhospitable state.",
        "Formation (~4.54 billion years ago): Earth formed approximately 4.54 billion years ago from the protoplanetary disk around the young Sun. This period involved the accretion of material, differentiation into core and mantle, and the early development of the planet’s surface.",
        "Early Life and Stabilization (~3.5 billion years ago): Life began to appear on Earth around 3.5 billion years ago. During this time, the planet experienced stabilization of its geological and atmospheric conditions, making it conducive for the development and evolution of life.",
        "Current Habitable Phase (~4.6 billion years ago to about 1 billion years from now): Earth has been in a stable, habitable phase for about 4.6 billion years. This period includes the development of complex life forms and ecosystems. The planet's climate and atmospheric conditions have supported life, including advanced organisms like plants, animals, and humans.",
        "Loss of Habitability (in about 1-1.5 billion years): As the Sun’s luminosity increases over the next 1-1.5 billion years, Earth’s temperature will rise, leading to the loss of liquid water and the breakdown of the planet’s ability to support life. This period will see the gradual transition of Earth into a less habitable state.",
        "Red Giant Phase (~5 billion years from now): In about 5 billion years, the Sun will enter the red giant phase, expanding and potentially engulfing Earth. This expansion will make the planet’s surface temperatures rise dramatically, making it impossible for life to survive.",
        "White Dwarf Phase (~5.5 billion years from now): After shedding its outer layers, the Sun will become a white dwarf. Earth will remain as a cold, lifeless rock orbiting this cooling remnant. Over billions of years, the white dwarf will gradually cool and dim.",
        "Final Stages (tens of billions of years from now): Eventually, the white dwarf will become a black dwarf, a cold, dark object. If Earth still exists by this point, it will be a frigid and lifeless world, reflecting the end of its habitable era.",
        "Cosmic Events and External Factors: Throughout its lifetime, Earth may also face additional challenges from cosmic events such as asteroid impacts or intense radiation, which could affect its habitability."
      ]
    }
  ]
}