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OREKIT (ORbits Extrapolation KIT) is a low level space dynamics library. It provides basic elements (orbits, dates, attitude, frames ...) and various algorithms to handle them (conversions, analytical and numerical propagation, pointing ...).

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/* Copyright 2002-2024 CS GROUP
 * Licensed to CS GROUP (CS) under one or more
 * contributor license agreements.  See the NOTICE file distributed with
 * this work for additional information regarding copyright ownership.
 * CS licenses this file to You under the Apache License, Version 2.0
 * (the "License"); you may not use this file except in compliance with
 * the License.  You may obtain a copy of the License at
 *
 *   http://www.apache.org/licenses/LICENSE-2.0
 *
 * Unless required by applicable law or agreed to in writing, software
 * distributed under the License is distributed on an "AS IS" BASIS,
 * WITHOUT WARRANTIES OR CONDITIONS OF ANY KIND, either express or implied.
 * See the License for the specific language governing permissions and
 * limitations under the License.
 */
/**
 *
 * This independent package provides classes to handle epochs, time scales,
 * and to compare instants together.
 *
 * 

* The principal class is {@link org.orekit.time.AbsoluteDate} * which represents a unique instant in time, with no ambiguity. For that * purpose, the ways to define this object are quite strict. *

* *

The easiest and most evident way is to define an instant with an offset from another * one. Orekit defines 9 reference epochs. The first 6 are commonly used in the space * community, the seventh one is commonly used in the computer science field and the * last two are convenient for initialization in min/max research loops: *

    *
  • {@link org.orekit.time.AbsoluteDate#JULIAN_EPOCH Julian Epoch}: -4712-01-01 at 12:00:00, TTScale
  • *
  • {@link org.orekit.time.AbsoluteDate#MODIFIED_JULIAN_EPOCH Modified Julian Epoch}: 1858-11-17 at 00:00:00, TTScale
  • *
  • {@link org.orekit.time.AbsoluteDate#FIFTIES_EPOCH Fifties Epoch}: 1950-01-01 at 00:00:00, TTScale
  • *
  • {@link org.orekit.time.AbsoluteDate#CCSDS_EPOCH CCSDS Epoch}: 1958-01-01 at 00:00:00, TAIScale
  • *
  • {@link org.orekit.time.AbsoluteDate#GPS_EPOCH GPS Epoch}: 1980-01-06 at 00:00:00, UTCScale
  • *
  • {@link org.orekit.time.AbsoluteDate#J2000_EPOCH J2000 Epoch}: 2000-01-01 at 12:00:00, TTScale
  • *
  • {@link org.orekit.time.AbsoluteDate#JAVA_EPOCH Java Epoch}: 1970-01-01 at 00:00:00, TTScale
  • *
  • {@link org.orekit.time.AbsoluteDate#PAST_INFINITY Past infinity}: at infinity in the past,
  • *
  • {@link org.orekit.time.AbsoluteDate#FUTURE_INFINITY Future infinity}: at infinity in the future.
  • *
* *

* The second definition, which could be the source of some confusion if not used with care, * is by giving a location (a date) in a specific time scale. It is of prime importance * to understand the various available time scales definitions to avoid mistakes. Orekit provides * 9 of the most important ones: *

    *
  • {@link org.orekit.time.TAIScale}: International Atomic Time,
  • *
  • {@link org.orekit.time.TTScale}: Terrestrial Time as defined by IAU(1991) * recommendation IV. * Coordinate time at the surface of the Earth. It is the successor of * Ephemeris Time TE. By convention, TT = TAI + 32.184 s,
  • *
  • {@link org.orekit.time.UTCScale}: Coordinated Universal Time. * UTC is related to TAI using step adjustments from time to time according * to IERS (International Earth Rotation Service) rules. These adjustments * require introduction of leap seconds. * Some leaps are already known and predefined in the library (at least * from 1972-01-01 to 2009-01-01) and other ones can be supported by * providing UTC-TAI.history files using the data loading mechanism * provided by {@link org.orekit.data.DataProvidersManager},
  • *
  • {@link org.orekit.time.UT1Scale}: Universal Time 1. * UT1 is a time scale directly linked to the actual rotation of the Earth. * It is an irregular scale, reflecting Earth irregular rotation rate. * The offset between UT1 and {@link org.orekit.time.UTCScale} is found in * the Earth Orientation Parameters published by IERS,
  • *
  • {@link org.orekit.time.TCGScale}: Geocentric Coordinate Time. * Coordinate time at the center of mass of the Earth. * This time scale depends linearly on TTScale,
  • *
  • {@link org.orekit.time.TDBScale}: Barycentric Dynamic Time. * Time used to compute ephemerides in the solar system. * This time is offset with respect to TT by small relativistic corrections * due to Earth motion,
  • *
  • {@link org.orekit.time.TCBScale}: Barycentric Coordinate Time. * Coordinate time used for computations in the solar system. * This time scale depends linearly on TDBScale,
  • *
  • {@link org.orekit.time.GPSScale}: Global Positioning System reference scale. * This scale was equal to UTC at start of the {@link * org.orekit.time.AbsoluteDate#GPS_EPOCH GPS Epoch} when it was 19 seconds * behind TAI, and remained parallel to TAI since then (i.e. UTC is now * offset from GPS due to leap seconds). TGPS = TAI - 19 s,
  • *
  • {@link org.orekit.time.GMSTScale}: Greenwich Mean Sidereal Time scale. * The Greenwich Mean Sidereal Time is the hour angle between the meridian * of Greenwich and mean equinox of date at 0h UT1.
  • *
* *

* Once it is built, an {@link org.orekit.time.AbsoluteDate} can be compared to * other ones, and expressed in other time scales. It is used to define states, * orbits, frames... Classes that include a date implement the {@link * org.orekit.time.TimeStamped} interface. * The {@link org.orekit.time.ChronologicalComparator} singleton can sort objects * implementing this interface chronologically. *

* * @author L. Maisonobe * */ package org.orekit.time;




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