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Commercial elliptical trainer (rear drive version) Row of elliptical trainers at a gym (right) ElliptiGO trainers are elliptical but not stationary. An elliptical trainer or cross-trainer is a stationary exercise machine used to stair climb, walk, or run without causing excessive pressure to the joints, hence decreasing the risk of impact injuries.
Data General microEclipse microprocessor. The Data General Eclipse line of computers by Data General were 16-bit minicomputers released in early 1974 and sold until 1988. The Eclipse was based on many of the same concepts as the Data General Nova, but included support for virtual memory and multitasking more suitable to the small office than the lab.
The Eclipse launch was marred by production problems and it was some time before it was a reliable replacement for the tens of thousands of Novas in the market. As the mini world moved from 16-bit to 32, DG introduced the Data General Eclipse MV/8000 , whose development was extensively documented in the popular book, The Soul of a New Machine .
The MV/8000 was succeeded by the MV/6000, MV/8000-II, MV/2000, MV/2500, MV/4000, MV/10000, MV15000, MV/20000, MV/30000 and MV/40000. Later models such as the MV/40000 were SMP systems with hot-swappable components. [1] The Eclipse MV was a 32-bit CISC architecture with a 4 GB address space.
The eclipse — when the moon passes between the sun and Earth, blocking the view of the sun — will start at 2:04 p.m. and last for about two and a half hours. The full eclipse will occur ...
This will be the longest total solar eclipse between 4000 BCE and at least CE 6000 (10,000 years), lasting a maximum of 7 minutes, 29.22 seconds. The factors that will make this such a long eclipse are: The Earth being very near aphelion (furthest away from the Sun in its elliptical orbit, making its angular diameter nearly as small as possible ...
Charlene Leibel, 75, started strength training after a body composition scan. Here's how she converted 50 percent of her body weight into muscle.
The eccentricity of an orbit is a measure of how elliptical (elongated) it is. All the planets of the Solar System except for Mercury have near-circular orbits (e<0.1). [8] Most exoplanets with orbital periods of 20 days or less have near-circular orbits, i.e. very low eccentricity.
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