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A single upgrade is usually the difference between first and third place, and it's the upgrades where GT Racing 2's free-to-play elements emerge.Įach upgrade takes time, but it also requires that you hire a mechanic for the job. You have to work your way up through the ranks, earning a hefty number of stars in races before you can add the next car to your garage.Įarning stars often feels like it's more a matter of upgrading your vehicle than actual racing skill, which can be frustrating. Of course, seeing it all takes time, and lots of it.

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> Download 'Oceanhorn' from the App Store

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Oceanhorn may not be as clever as Nintendo's series in its dungeon designs, and few games are, but the sense of exploration and discovery makes it easy to recommend on its own merits. It's also a huge world, with an adventure that could easily last a dozen or more hours of island hopping and dungeon spelunking.

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Even with sometimes shallow puzzles and control quirks, the world of Oceanhorn is just a joy to explore, full of hidden secrets and side-quests to discover. It really can't be stressed enough just how gorgeous Oceanhorn is though. There are also occasional control frustrations due to the reliance on a single context-sensitive action button that might accidentally pick up a nearby pot instead of swinging your sword when enemies are around. Hipparchus made his discovery around 130 BCE, based on comparisons of astronomical observations more than a century apart.Dungeon puzzles usually just revolve around pushing blocks, standing on switches and lighting torches instead of finding creative ways to use the equipment you find like bombs and a bow and arrow. Greek astronomer Hipparchus of Nicea is historically credited as the man who first proposed that Earths axis gradually shifts, though very slowly. It outlines the shape of a pair of cones or two spinning tops connected at the tips, which would be at the center of Earth. A complete wobble of Earth's axis takes around 26,000 years. Acts Like Two Spinning TopsĪxial precession can be described as a slow gyration of Earth's axis about another line intersecting it. It is caused by the gravitational force from the Sun, the Moon, and other planets. This wobble motion is called axial precession, also known as precession of the equinoxes. The reason for this changing obliquity angle is that Earth's axis also wobbles around itself. The Arctic and Antarctic circles today are 1,2 m (4 ft) closer to the poles, and the Tropic of Cancer and Tropic of Capricorn are equally closer to the equator than 30 days ago.Įarth: The living planet The Tilt ChangesĮarth's axial tilt actually oscillates between 22.1 and 24.5 degrees. at noon, Earth's axial tilt, or mean obliquity was 23,43633° or 23☂6'10.8'.Įarth's mean obliquity today is about 0,00001°, or 0.04', less than 30 days ago. We say 'at the moment' because the obliquity changes over time, although very, very slowly. This slant is the axial tilt, also called obliquity.Įarth's obliquity angle is measured from the imaginary line that runs perpendicular to another imaginary line Earth's ecliptic plane or orbital plane (see illustration).Īt the moment, Earth's obliquity is about 23.4 degrees and decreasing. The impact around 4.5 billion years ago is described in the Giant Impact Hypothesis, which is the current prevailing theory on how the Moon was formed and how Earth got its tilt.Įver since this impact, Earth has been orbiting the Sun at a slant. In our illustrations, Earth's axis is drawn as a straight red line.

In astronomy, an axis refers to the imaginary line that an object, usually a planet, rotates around.Įarth's rotational axis is an imaginary straight line that runs through the North and South Pole. Business Date to Date (exclude holidays).