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  2. Numismatic Museum of Guatemala - Wikipedia

    en.wikipedia.org/wiki/Numismatic_Museum_of_Guatemala

    The Numismatic Museum of Guatemala (Spanish: Museo Numismático de Guatemala) is a museum in Guatemala City. The museum is dedicated to the history of banknotes and ...

  3. HE 2359-2844 - Wikipedia

    en.wikipedia.org/wiki/HE_2359-2844

    HE 2359-2844 is a subdwarf located approximately 800 light years away in the constellation Sculptor, with a surface temperature of approximately 38,000 °C (68,400 °F).). Along with stars HE 1256-2738 and LS IV-14 116, HE 2359-2844 forms a new group of star called heavy metal subdw

  4. Monasterio de Santo Domingo, Antigua Guatemala - Wikipedia

    en.wikipedia.org/wiki/Monasterio_de_Santo...

    "Arquitectos de Antigua Guatemala". antiguaguatemalaonline.com (in Spanish). Archived from the original on 15 May 2004. Cadena, Felipe (1774). Breve descripción de la noble ciudad de Santiago de los Caballeros de Guatemala y puntual noticia de su lamentable ruina ocasionada de un violento terremoto el día veintinueve de julio de 1773 (PDF ...

  5. Guillermo Arévalo - Wikipedia

    en.wikipedia.org/wiki/Guillermo_Arévalo

    Guillermo Arévalo Valera (born 1952) is a Shipibo vegetalista and businessperson from the Maynas Province of Peru. His Shipibo name is Kestenbetsa.. In 1982, Arévalo co-founded Aplicación de Medicina Tradicional (AMETRA), an organization that sought to improve the sustainability of health care for the Shipibo-Conibo people by integrating traditional plant medicines.

  6. Valley with Ploughman Seen from Above - Wikipedia

    en.wikipedia.org/wiki/Valley_with_Ploughman_Seen...

    Valley with Ploughman Seen from Above or Landscape with House and Ploughman (Dutch - Landschap met een huis en een ploeger in vogelvlucht gezien) is an 1889 [1] oil on canvas painting by Vincent van Gogh, produced during the autumn of his stay in Saint-Rémy.

  7. LB-1 - Wikipedia

    en.wikipedia.org/wiki/LB-1

    The optically observed star, LB-1 A, or LS V+22 25, is a B-type star [5] nine times the mass of the Sun and located at least 7,000 light-years (2,100 pc) from Earth. It was found to exhibit radial velocity variations by Chinese astronomers using the Large Sky Area Multi-Object Fiber Spectroscopic Telescope (LAMOST) and the radial-velocity method to search for such wobbly stars.