How Does Light Intensity of a Star Change with Distance? Measure carbon abundances, using the medium-resolution spectroscopy (MRS) technique, for stars in the Milky Way's dwarf satellites Learn about how and why NASA false-colors x-ray images then follow the same procedure to create your own images and compare them to the NASA ones.Ī Computational Investigation of the Structures, Energies, and Formation Pathways of Interstellar Anions The Formation, Evolution and Death of Stars Measure true noon time using the sundial principleĬalculate the circumference of the Earth.Įxplore the deep space - stars and black holes Test the stellar parallax theory, a method used to determine the relative distance of stars, through a series of observations taken on a football field. What Are the Effects of Weather on Star Visibility?ĭiscover how many of the brightest infrared-emitting objects in an infrared sky patch are familiar objects such as stars. Use Internet-based software tools and databases to locate the center of the galaxy, based on the distribution of globular clusters.Īre the globular clusters in our galaxy just one color, and what might we guess from this about the ages and compositions of galaxies?įind whether cosmic rays are affected by magnets.ĭetermine if you can tell from a light curve if a variable star is a binary system.ĭo the Planets Revolve Around the Earth or the Sun?įind out if Saturn's moons cause the gaps in Saturn's rings. Measure the distance to some distant, small objects using motion parallax. Detecting solar system objects using blocked starlight: the case of Planet 9ĭetermining if Concrete Is a Liable Screen against Galactic Cosmic RadiationĬan an Amateur Astronomer Measure Double Stars Accurately?įinding the internal characteristics of variable stars by analyzing their light curves.Ī Photometric Comparison of the Variable Stars Beta Lyrae and Delta Cepheiįind out how old is a star (Monoceros R2) by using images from the Faulkes Telescope in Australia.
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