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Featuring free WiFi, Hotel Europa & Casino offers pet-friendly accommodation in Kutaisi. The hotel has a barbecue and views of the mountain, and guests can enjoy a drink at the bar. Each room has a flat-screen TV with satellite channels. Some units have a seating area for your convenience. Certain units feature views of the garden or city.

The rooms include a private bathroom. For your comfort, you will find slippers and free toiletries.

There is a 24-hour front desk and shops at the property. Bike hire is available at this hotel and the area is popular for horse riding. Europa Hotel offers unique retro car hire service.

Regulatory Fitness and Performance Programme (REFIT) and the 10 Priorities of the Commission. Scoreboard summary (2017). Nov 13, 2018 - The 28th Alzheimer Europe Conference (#28AEC) “Making dementia a European priority” was held in Barcelona on 29-31 October 2018,.

Bagrati Cathedral is 5.5 km away while Gelati Monastery is 13 km from Hotel Europa&Casino. The nearest airport is Kutaisi International Airport, 12 km from the property.

Artist concept of the Europa Jupiter System Mission: Jupiter Europa Orbiter (top) and Jupiter Ganymede Orbiter (bottom) Mission type Multiple orbiters and lander Operator Proposed joint / The Europa Jupiter System Mission – Laplace ( EJSM/Laplace) was a proposed joint / slated to launch around 2020 for the in-depth exploration of 's moons with a focus on, and Jupiter's. The mission would have comprised at least two independent elements, NASA's (JEO) and ESA's (JGO), to perform coordinated studies of the Jovian system. The (JAXA) and the (Roscosmos) had expressed their interest in contributing to EJSM/Laplace, although no deals had been finalized. JEO was estimated to cost $4.7 billion, while ESA would spend $1.0 billion (€710 million) on JGO. In April 2011, ESA stated that it seemed unlikely that a joint US–European mission will happen in the early 2020s given NASA's budget, so ESA continued with its initiative, called the (JUICE) that will be based on the JGO design. Selection of JUICE for the L1 launch slot of ESA's science programme was announced on 2 May 2012.

Later, in June 2015, NASA approved the and it entered the formulation stage, with an expected launch between 2022-2025. Contents • • • • • Origins [ ] In February 2008, and began joint investigations into sending a probe to study the icy satellites of the outer Solar System under the title. Two primary candidate missions were considered under the study: EJSM and (TSSM), also known under the ESA designation TandEM. In February 2009 it was announced that NASA/ESA had given EJSM priority ahead of the TSSM.

The ESA contribution still faced funding competition from two other missions, the (LISA) and the (IXO), which is why NASA kept a contingency plan of sending its part of the mission as a stand-alone project. Mission architecture [ ]. A map showing all the nations which are either currently part of (red) or interested in becoming a part of (brown) the EJSM The most distinctive feature of the EJSM/Laplace-study, was the proposed collaboration with multiple orbiters and landers: •: (JEO), proposed to study. •: (JGO), proposed to study and •: (JMO), proposed to study 's magnetosphere.

•: (JTAX), proposed to study a. The baseline EJSM architecture consisted of JEO and JGO, which were proposed to be launched in 2020 and explore the Jupiter System before settling into orbit around Europa and Ganymede, respectively. The JEO and JGO were separate and independent spacecraft developed, launched and operated by their respective organizations to work together.

Their launch dates and interplanetary trajectories were not to be dependent on each other, but would have been synergistic. Goal [ ] The goal was to determine whether the Jupiter system harbors, while focusing on Europa and Ganymede. The main science objectives supporting this goal were: • Characterize sub-surface oceans • Characterize the ice shells and any subsurface water • Characterize the deep internal structure for Ganymede and the intrinsic magnetic field • Compare the, environments, and magnetospheric interactions. • Determine global surface compositions and chemistry • Understand the formation of surface features, including sites of recent or current activity, and identify and characterize candidate sites for future in situ exploration. References [ ]. • (page 365) • de Selding, Peter B. (4 February 2011).