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Chang'e 4 lander
|Mission type||Lander, Lunar rover|
|Mission duration||12 months|
|Launch mass||Orbiter: 425 kg|
Lander: 1,200 kg 
Rover: 140 kg
|Landing mass||Total: ~1,200 kg; rover: 140 kg|
|Dimensions||Length: 1.5 m, width: 1.0 m, height: 1.0 m |
|Start of mission|
|Launch date||Orbiter: 20 May 2018|
Lander & rover: UTC17:30-19:30 7 December 2018
|Rocket||Long March 3B |
|Launch site||Xichang Satellite Launch Center|
Chang'e 4 (Chinese: 嫦娥四号; pinyin: Cháng'é sìhào) is a planned Chinese lunar exploration mission, to be launched in December 2018, that will incorporate an orbiter, a robotic lander and rover. Chang'e 4 will be China's second lunar lander and rover. It was built as a backup to Chang'e 3, as Chang'e 2 was to Chang'e 1. Following the successful landing of the Chang'e 3 mission, the configuration of Chang'e 4 will be adjusted to meet new scientific objectives. Like its predecessors, the spacecraft is named after Chang'e, the Chinese Moon goddess.
The Chang'e 4 mission was first scheduled for launch in 2015 as part of the second phase of the Chinese Lunar Exploration Program. But the adjusted objectives and design of the mission imposed delays, and it is currently scheduled for launch in December 2018. This mission will attempt to determine the age and composition of an unexplored region of the Moon, as well as develop technologies required for the later stages of the program.
The Chinese Lunar Exploration Program has started to incorporate private investment from individuals and enterprises for the first time, a move aimed at accelerating aerospace innovation, cutting production costs, and promoting military-civilian relationships. After Chang'e 4, China will follow with a series of other robotic lunar missions that will build towards an attempted human landing in the early 2030s.
Since Chang'e 4 is planned to land on the far side of the Moon, CNSA first launched the Queqiao (Chinese: 鹊桥; pinyin: Quèqiáo) communication relay satellite to Earth–Moon L2 point on 20 May 2018 to relay commands and data between the lander/rover and the Earth station. The relay satellite has a mass of 425 kg, and it will use a 4.2-meter antenna to receive X band signals from the lander and rover, and relay them to Earth control on the S band.
The lander and rover are expected to be launched six months after the launch of the relay satellite, toward the end of 2018. It will be the first landing on the lunar far side, an unexplored region of the Moon called South Pole-Aitken Basin, a vast basin in the southern hemisphere of the far side which extends from the South Pole to Aitken crater.
The proposed landing site is the crater Von Kármán (180 km diameter) in the South Pole-Aitken Basin on the far side of the Moon. Regarding its composition, it contains about 10% by weight iron oxide (FeO) and 4-5 parts per million of thorium, which has been used as a replacement for uranium as nuclear fuel on several thorium reactors.Landing date in January 2019.
The science objectives include: 
The communications relay satellite, orbiting microsatellites, lander and rover will each carry scientific payloads. The relay satellite will perform radio astronomy, whereas the lander and rover will study the geophysics of the landing zone. These payloads are, in part, supplied by international partners in Sweden, Germany, the Netherlands and Saudi Arabia.
The primary function of the Queqiao relay satellite, which is being deployed in a halo orbit around the Earth-Moon L2 point, is to provide continuous communications between Earth and the lander on the far side of the Moon. Additionally, this satellite will host the Netherlands-China Low-Frequency Explorer (NCLE), an instrument which will perform astrophysical studies in the unexplored radio regime of 80 kHz to 80 MHz from translunar locations.
As part of the Chang'e 4 mission, two microsatellites (45 kg each) named Longjiang-1 and Longjiang-2 will be deployed into lunar orbit to observe the sky at very low frequencies (1 MHz-30 MHz), corresponding to wavelengths of 300m–10m, with the aim of studying energetic phenomena from celestial sources. Due to the Earth's ionosphere, no observations in this frequency range has been done in Earth orbit, offering potential breakthrough science.
The Lander is equipped with the following payloads: