Shop/product_info.php/language/en/info/p144 TS-Optics Super Plössl Eyepiece 20 mm (2017). Thickness of impact crater ejecta on the lunar surface. Journal of Physics: Conference Series, 901, 1–4. The pre-service teachers understanding about moon phase. Measuring the depth of an impact crater using an internal Scott, R., Shen, X., Mulley, I., & Pan, Z. Determining the volume of material excavated during a cratering event.
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How to make an impact with planetary science? Part II. How to make an impact with planetary science? Part I. Crater dimensions from Apollo data and supplemental sources. The thin border between light and shadow. Measuring the apparent size of the Moon with a digital camera. The crater diameter–depth relationship from Ranger VII photographs. Retrieved from /cameras/the-imaging-source-dfk-41au02-as-color-astro-camera/p,11775īaldwin, R. Astro camera: The Imaging Source DFK 41AU02.AS. Such experimental work enables students to gain specific natural science and mathematical competences that are also required for the study of other natural phenomena.Ī (2017). With some mathematical simplifications, however, the treatment of the topic can also be appropriate in primary school. Virtual Moon Atlas, used to locate the position of the flash on the moon. An analysis of the results of the students’ experimental work, as well as of curricula on various levels of education, led us to conclusion that this kind of experimental work is suitable for incorporation in secondary school physics education. 14 (355mm) f/8 Meade RCX400 on an equatorial wedge or a 10 f/4.7 Newtonian. The fieldwork with students of junior grade school education was performed within the framework of the optional subject Astronomy. We focus on the observation of craters on the Moon, determining their lateral size and depth on the basis of photographs and simple calculations. In this paper, we present an example of observation of the Moon, which is our nearest astronomic object and therefore does not require professional astronomic equipment for observation. The open star cluster M37 is shown below as captured with an 8″ telescope and video camera.Experimental work in the research of astronomical phenomena is often difficult or even impossible because of long-lasting processes or too distant objects and correspondingly too expensive equipment. Even if there isn’t much nebulosity visible, the Trapezium at the center of M42 can be seen as a quadruple star system. The open clusters are M35 in Gemini and M36, M37, and M38 in Auriga, and the nebula is M42 the Orion Nebula. Nebula and Star Clusters: There are a few open clusters of stars and one nebula that wouldn’t normally be too difficult to see, but they all will appear fairly close to the moon tonight, reducing their visibility. This article from Sky and Telescope magazine gives information on other interesting stars in the area. Some years ago it was difficult to “split” as a double, now it’s easier because their separation has increased. Castor can be seen as a double star in almost any telescope, and the orbital motion of its components is visible within a human lifetime.
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Free star-charting program for MS-Windows Virtual Moon Atlas Consolidated Lunar Atlas. It will be high overhead tonight, 73 degrees in altitude at 8pm. Khan Scope Centre KW Telescope (Kitchener) Meade Telescopes.
Deep-Sky Objects:ĭouble Stars: Castor is a bright binary star in Gemini. While appearing close together in the sky, Mars is 154 million miles away and Uranus is 1890 million. Mars will be observable with a telescope until 9pm, after which it will be too low in the sky, and nearby Uranus will reach the limit at 8:45. Image copyright (c) Virtual Moon Atlas /, with thanks to Christian Legrand & Patrick Chevalley.
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