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Orbital decay is a gradual decrease of the distance between two orbiting bodies at their closest approach (the periapsis) over many orbital periods. These orbiting bodies can be a planet and its satellite , a star and any object orbiting it, or components of any binary system .
In the preface to Relativity: The Special and the General Theory, Einstein said "The present book is intended, as far as possible, to give an exact insight into the theory of Relativity to those readers who, from a general scientific and philosophical point of view, are interested in the theory, but who are not conversant with the mathematical ...
Cities on the Edge (PDF) Deep Beyond; Fifth Wave; High Frontier; In The Well; Martial Arts 2100 (PDF) Orbital Decay; Personnel Files 1; Personnel Files 2: The Meme Team (PDF) Personnel Files 3: Wild Justice (PDF) Personnel Files 4: Martingale Security (PDF) Personnel Files 5: School Days 2100 (PDF) Polyhymnia (PDF) Shell-Tech (PDF) Singapore ...
Steele began publishing short stories in 1988. His early novels formed a future history beginning with Orbital Decay and continuing through Labyrinth of Night. Some of his early novels such as Orbital Decay and Lunar Descent were about blue-collar workers working on future construction projects in space. Since 1992, he has tended to focus on ...
Steele said "V-S Day" first began as a novelette, "Operation Blue Horizon", which was published in 1988. The idea for the story came while researching his first book, Orbital Decay (1989) when he stumbled onto references to Sänger's space bomber. Steele stated that he "wasn't completely satisfied" with "Operation Blue Horizon" and rewrote it.
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NEW YORK (AP) — In a string of visits, dinners, calls, monetary pledges and social media overtures, big tech chiefs — including Apple's Tim Cook, OpenAI’s Sam Altman, Meta’s Mark ...
Simulated collision of two neutron stars. A stellar collision is the coming together of two stars [1] caused by stellar dynamics within a star cluster, or by the orbital decay of a binary star due to stellar mass loss or gravitational radiation, or by other mechanisms not yet well understood.