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China’s Communication Satellite is Orbiting the Moon

China’s Relay Satellite, Queqiao-2, has successfully entered lunar orbit, marking a significant milestone in the Chinese Lunar Exploration Program. Launched on March 20th atop a Long March-8 Y3 carrier rocket, Queqiao-2 completed a perilune braking maneuver on March 24th, positioning itself 440 km from the lunar surface. This satellite will serve as a crucial communications relay for missions on the far side of the Moon, including Chang’e-4, Chang’e-6, Chang’e-7, and Chang’e-8.

The perilune braking maneuver is essential for establishing a lunar orbit, allowing the spacecraft to be captured by the Moon’s gravity. Along with Queqiao-2, two experimental satellites, Tiandu-1 and -2, also performed this maneuver successfully and entered lunar orbit. These satellites will conduct communication and navigation tests, including laser ranging with the Moon and microwave ranging between satellites.

Queqiao-2 will be positioned in a 24-hour elliptical orbit around the Moon, with its closest point at 200 km and its farthest point at 100,000 km. This orbit will provide direct communication with ground stations on Earth and the far side of the Moon. The satellite is equipped with advanced scientific instruments, including extreme ultraviolet cameras and lunar orbit Very Long Baseline Interferometry (VLBI) test subsystems.

According to CCTV, the CNSA selected Queqiao-2’s orbit for its strategic location in the Moon’s maria region, known as the Sea of Abundance. This area holds historical significance for China’s lunar exploration project, making it an ideal choice for the satellite’s operations. Queqiao-2 will support upcoming missions like Chang’e-6, as well as pave the way for future lunar exploration and resource scouting.

China’s Lunar Exploration Program aims to rival NASA’s Artemis Program, which is set to send astronauts on a circumlunar flight next year. NASA’s program includes plans for a sustained program of lunar exploration and development, with the deployment of the Lunar Gateway and Artemis Base Camp. In collaboration with international partners, these initiatives will pave the way for human exploration and research on the Moon.

As China’s Relay Satellite settles into lunar orbit, it heralds a new era of lunar exploration and cooperation among nations. With its advanced capabilities and strategic positioning, Queqiao-2 is poised to play a crucial role in China’s ambitious plans for the Moon, setting the stage for further discoveries and advancements in space exploration.

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Further Support for Gravitational Wave Background in the Universe

The discovery of the gravitational wave background in 2016 marked a significant milestone in our understanding of the Universe. This groundbreaking discovery was further validated by the release of a second data set from the European Pulsar Timing Array, along with the addition of data from the Indian Pulsar Timing Array. These complementary studies have provided more evidence for the existence of the gravitational wave background, shedding light on the cosmic phenomena that shape our universe.

Gravitational waves are ripples in spacetime that are generated by violent processes such as merging black holes and colliding neutron stars. Predicted by Einstein in 1916 as part of his General Theory of Relativity, these waves have the ability to travel through space, largely unimpeded by any obstacles in their path. The first detection of gravitational waves in 2015 by the Laser Interferometer Gravitational-Wave Observatory (LIGO) confirmed their existence, originating from a gravitational merger between two black holes located 1.3 billion light years away.

The Laser Interferometer Gravitational-Wave Observatory is made up of two detectors, this one in Livingston, La., and one near Hanford, Wash. The detectors use giant arms in the shape of an “L” to measure tiny ripples in the fabric of the universe. Credit: Caltech/MIT/LIGO Lab

The recent confirmation of the gravitational wave background by the European and Indian Pulsar Timing Arrays indicates that we are detecting a combined signal from the mergers of supermassive black holes. This random distribution of gravity waves that permeates the Universe offers a new avenue for studying the cosmos, akin to the Cosmic Background Radiation. The collaborative efforts of various observatories and research institutions have enabled us to delve deeper into the mysteries of the Universe.

The full-sky image of the temperature fluctuations (shown as color differences) in the cosmic microwave background, made from nine years of WMAP observations. These are the seeds of galaxies, from a time when the universe was under 400,000 years old. Credit: NASA/WMAP

Utilizing pulsar timing arrays as galaxy-sized detectors, researchers have been able to monitor and analyze the pulse arrival times of galactic pulsars on Earth. By detecting subtle patterns in these signals, they can uncover the presence of the gravitational wave background. The latest study led by J. Antoniadis from the Institute of Astrophysics in Greece delves into the implications of the low-frequency signals observed in the recent data releases from various pulsar timing array systems.

The accumulation of data from multiple sources has provided undeniable evidence for the existence of the gravitational wave background. With ongoing Pulsar Timing Array projects, the signals of the low-frequency gravity waves will become more distinct, offering a wealth of opportunities to explore the Universe in this novel way. The focus now shifts towards interpreting these signals to unlock the secrets of the cosmos.

Source : The second data release from the European Pulsar Timing Array: IV. Implications for massive black holes, dark matter and the early Universe

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