AD ES Soldeu Monterdit de Baix Puente de Montanana Col de Nargo Soldeu 343 km
Monterdit de Baix
From Soldeu we will visit another National Park in Spain.
After crossing the border of Spain we head towards Monterdit de Baix and then towards Puente de Montanana.
We pass a number of lakes and rivers on this trip.
I would like to mention two of them: Panta d 'Escales with its truly beautiful blue green color and Panta de Sant Antoni which is really bordered by beautiful mountains and is also special in color.
The nature that we cross today is called La Pobla de Segur and is beautiful with its occasional sun masses of red mountain massifs and the previously mentioned Panta de Sant Antoni.
Eventually we enter Andorra again and cross the country again on our way to Soldeu. It is a must to stroll around Andorra in the capital of Andorra la Vella. Special buildings and a small stream that cools and traverses the city.
Puente de Montanana
Col de Nargo
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About this region
NGC 2985 is a spiral galaxy located in the constellation Ursa Major. It is located at a distance of circa 70 million light years from Earth, which, given its apparent dimensions, means that NGC 2985 is about 95,000 light years across. It was discovered by William Herschel on April 3, 1785.The galaxy is seen with an inclination of 37 degrees. The galaxy has a bright nucleus from which emanate multiple tightly wound spiral fragments. Numerous blue knots are visible at the galactic disk. At the outer part of the galaxy lies a massive spiral arm that forms a pseudoring that encircles the galaxy. The inner part of the galaxy, where active star formation has been observed, has been found to be unstable, contrary to the outer stable one. It has been suggested that the presence of molecular clouds accounts for the instability of the region.The nucleus of NGC 2985 is active, and based on its spectrum has been categorised as a LINER. The most accepted theory for the activity source is the presence of an accretion disk around a supermassive black hole. The mass of the supermassive black hole at the centre of NGC 2985 is estimated to be 160 million (108.2) M☉, based on stellar velocity dispersion. The velocity dispersion is anisotropic, and changes with the azimuth. The rotational speed of the galaxy at its effective radius is 222.9 ± 31.2 km/s.NGC 2985 is the brightest member of a galaxy group known as the NGC 2985 group. Other members of the group include NGC 3027, 25 arcminutes away. Other nearby galaxies include NGC 3252, and NGC 3403.
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