Coordinates: 50°48′14″N 1°58′41″W / 50.804°N 1.978°W / 50.804; -1.978
Wimborne Minster (often referred to as Wimborne, /ˈwɪmbɔːrn/) is a market town in East Dorset in South West England, and the name of the Church of England church in that town. The town has a population of 6,790 (according to the 2011 Census) and is situated at the confluence of the River Stour and River Allen, 5 miles (8 km) north of Poole, on the Dorset Heaths. The town is also recognised as part of the South East Dorset conurbation.
The Mayor of Wimborne is currently Andy Hampton. The town and its administrative area is served by eleven councillors and one from the nearby ward of Cranfield. The electoral ward of Wimborne Minster is slightly bigger than the parish. The population of this ward at the 2011 census is 7,014. Wimborne is twinned with Valognes, France and Ochsenfurt, Germany. Wimborne Minster is part of the Mid-Dorset and North Poole Parliamentary Constituency.
MLO may refer to:
Gliese 667 (142 G. Scorpii) is a triple-star system in the constellation of Scorpius lying at a distance of about 6.8 pc (23.6 ly) from Earth. All three of the stars have masses smaller than the Sun. There is a 12th magnitude star close to the other three, but it is not gravitationally bound to the system. To the naked eye, the system appears to be a single faint star of magnitude 5.89.
The system has a relatively high proper motion, exceeding 1 second of arc per year.
The two brightest stars in this system, GJ 667 A and GJ 667 B, are orbiting each other at an average angular separation of 1.81 arcseconds with a high eccentricity of 0.58. At the estimated distance of this system, this is equivalent to a physical separation of about 12.6 AU, or nearly 13 times the separation of the Earth from the Sun. Their eccentric orbit brings the pair as close as about 5 AU to each other, or as distant as 20 AU, corresponding to an eccentricity of 0.6. This orbit takes approximately 42.15 years to complete and the orbital plane is inclined at an angle of 128° to the line of sight from the Earth. The third star, GJ 667 C, orbits the GJ 667 AB pair at an angular separation of about 30", which equates to a minimum separation of 230 AU.