By Nancy Paulu, Margery Martin
A realistic advisor for exciting a kid's curiosity in technology. offers secure and easy actions appropriate for kids from preschool throughout the early straightforward grades. indicates actions with bubbles, insects, vegetation, crystals, and tv. so much actions rate little or not anything and require no designated apparatus. Explores possibilities for studying technology in such areas as zoos, museums, planetariums, aquariums, and farms. offers definitions and outlines of technology and gives feedback for assisting kids comprehend and research medical principles. Appendices provide functional tips encouraging faculties to improve reliable technology courses, descriptions of 9 clinical ideas, and a listing of prompt technology books and magazines. initially on hand from the U.S. division of schooling.
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Additional resources for Helping Your Child Learn Science (American Chemical Society Publication)
Example text
1 The energy level diagram of hydrogen. The principal quantum number, n, increases upwards (for clarity only the lower ones are labeled). The orbital angular momentum number, , increases rightwards and only the first few are shown. They are labeled s, p, d, f. The arrows indicate some allowed transitions. (a) The Lyman through transitions are indicated. (b) The transitions between the lowest levels are indicated. Note that the 2s level is metastable. (n = 3), Brackett (n = 4), Pfund (n = 5), and Humphreys (n = 6).
Kennicutt, 2001, in Tetons 4: Galactic Structure, Stars and the Interstellar Medium, ed. C. E. Woodward, M. D. Bicay, and J. M. Shull (San Francisco: ASP), p. 2 2 Gas cooling In this chapter, we will examine the various line cooling processes of interstellar gas. Together with the heating processes, which are discussed in the next chapter, this will allow us to solve the energy balance for the gas in a wide variety of environments. 3). 1). 3). A two-level system analysis is a powerful tool for understanding the details of gas emission processes and we will encounter this many times in subsequent chapters.
Thus, the energy levels of H2 divide out into two separate ladders with even or odd J , which are not connected by radiative transitions. , parallel nuclear spins). Then, owing to nuclear spin statistics (gS = 2S + 1), the ortho levels have three times the statistical weight of the para levels. Symmetric top molecules For a non-linear molecule, the rotational energy will depend on the axis of rotation. Two of the moments of inertia are equal – usually by symmetry – in a symmetric top molecule. For a prolate symmetric top, IA < IB = IC (a cigar shape) and for an oblate symmetric top, IA = IB < IC (a disk shape) with Ii the respective moments of inertia.