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Saturday, December 10, 2016 - 7:00pm to 9:00pm
Tipple Hill Winery

Music by Casey Brett

Young Country and all your favorites.

Say Cheese Wine Trail
Sunday, December 11, 2016 - 11:00am to 5:00pm
Tipple Hill Winery Vineyard- Wine
Sunday, December 11, 2016 - 2:00pm to 4:00pm
Tipple Hill Winery

Wine Glass Fridays (on Sunday, just for this month) Painting Event

Instructor:Christina (NEW WINE GLASS PAINTING EVENT)

$25 pp includes all supplies needed to paint your own special wine glasses

(2).This month you will be painting two (2) Frosted Snowflake Wine glasses.Mustregister

Tipple Hill Winery Vineyard- Ladies
Wednesday, December 14, 2016 - 6:30pm to 8:30pm
Tipple Hill Winery

Ladies Bingo Night - A fundraiser for Toys for Tots

Sponsor: Judy Cunningham

Home Based Business will be provide prizes for the Bingo winners.

Bingo cards $5 each or 3 for $10

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Taylor Feighery (Indie Rock) will perform at Blumenhof Winery in Dutzow, MOon Friday, December 16 from 4-7pm.

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Saturday, December 17, 2016 - 2:00pm to 3:30pm
Jowler Creek Winery
Zero Friction Live at Blumenhof Winery
Saturday, December 17, 2016 - 2:00pm to 5:00pm
Blumenhof Winery

Zero Friction (Acoustic Rock Duo) will perform atBlumenhof Winery in Dutzow, MO on Saturday, December 17 from 2-5pm.

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Saturday, December 17, 2016 - 6:00pm to 9:00pm
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From Europa Universalis 4 Wiki
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This article may contain outdated information that is inaccurate for the current Green George Lace Up Shoes for Men Oxfords Derbies and Brogues On Sale Black Leather 2017 75 2018 Cool u0qZ2
of the game. It was last updated for 1.24.

Institutions are fundamental advances in civilization and are the primary determinant of Sperry Cutter CVO Mesh Wide Range Of Cheap Online 5E1889BYwQ
cost. Institutions, if not embraced by a country, will cause an increasing tech cost penalty on the country by +1% per year up to a maximum of +50% per institution. Embracing an institution requires that institution to be fully present in provinces containing at least 10% of a country's Gola Bullet Suede Sneaker Cheap Shop Offer Clearance Shop 6T8uBHpu
(modified by local autonomy ), after which it requires an amount of ducats dependent on the remaining development in provinces where the institution is not fully present. New World natives cannot embrace institutions until they reform their governments (for natives in the North American and South American technology groups) or religions (for natives in the Mesoamerican and Andean technology groups), but receive all the institutions of their advanced neighbor when they do so.

There are a total of 7 different institutions that appear throughout the game (except for the first which is present at the beginning of the game in 1444), at roughly 50-year intervals starting in 1450 and ending in 1700.

Each year all provinces an institution can spawn in are randomly given a chance to spawn the institution. Each eligible province for an institution has a 10% chance to get it to spawn in that province. If only 3 provinces can get it to spawn there is a 90% * 90% * 90% = 72.9% chance that it won't spawn in the beginning of that year. If none or only a few provinces are eligble for spawning, it can take years or even decades for an institution to show up.

Contents

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The spread of institutions is modified on both a global and a provincial level. Global modifiers affect the spread of institutions in all provinces in a nation, local modifiers affect the spread of institutions in a specific province.

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and policies also affect spread rate:

Developing a province gives that province an immediate increase in the oldest non-present institution equal to 16.66% (slightly under one sixth) of the new development of the province. The increase is capped at 10% (60 development). The development required to bring an institution with 0% presence to 100% presence is of 601 cumulative development points, because for 600 points (reaching 36 dev starting from 11) you get 99.96%. The required development within a province of a given starting development is summarized in the table below.

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Artist's impression of Planet Nine, blocking out the Milky Way. The Sun is in the distance, with the orbit of Neptune shown as a ring. Credit: ESO/Tomruen/nagualdesign
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Evidence Mounts for the Existence of Planet Nine

Article written: 14 Jul , 2017 Updated: 14 Jul , 2017

In January of 2016 , astronomers Mike Brown and Konstantin Batygin published the first evidence that there might be another planet in our Solar System. Known as “Planet 9”, this hypothetical body was estimated to be about 10 times as massive as Earth and to orbit that our Sun at an average distance of 700 AU. Since that time, multiple studies have been produced that either support or cast doubt on the existence of Planet 9.

While some argue that the orbits of certain Trans-Neptunian Objects (TNOs) are proof of Planet 9, others argue that these studies suffer from an observational bias. The latest study , which comes from a pair of astronomers from the Complutense University of Madrid (UCM), offers a fresh perspective that could settle the debate. Using a new technique that focuses on extreme TNOs (ETNOs), they believe the case for Planet 9 can be made.

Extreme Trans-Neptunian Objects are those that orbit our Sun at average distances greater than 150 AU, and therefore never cross Neptune’s orbit. As the UMC team indicate in their study , which was recently published in the Monthly Notices of the Royal Astronomical Society , the distances between the ETNOs nodes and the Sun may point the way towards Planet 9.

These nodes are the two points at which the orbit of a celestial body crosses the plane of the Solar System. It is at these points that the chances of interacting with other bodies in the Solar System is the greatest, and hence where ETNOs are most likely to experience a drastic change in their orbits (or a collision). By measuring where these nodes are, the team believed they could tell if the ETNOs are being perturbed by another object in the area.

As Carlos de la Fuente Marcos, one of the authors on the study, explained in an interview with The Information and Scientific News Service (SINC):

“If there is nothing to perturb them, the nodes of these extreme trans-Neptunian objects should be uniformly distributed, as there is nothing for them to avoid, but if there are one or more perturbers, two situations may arise. One possibility is that the ETNOs are stable, and in this case they would tend to have their nodes away from the path of possible perturbers, he adds, but if they are unstable they would behave as the comets that interact with Jupiter do, that is tending to have one of the nodes close to the orbit of the hypothetical perturber”.

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