(local link / semi-major axis (AKA mean orbital radius) Print out as many Table: Elongations and Nearest Planetary Configurations:     order of magnitude? hard to accept. planetary rings,     with inclination equal 90°? the geometric center, minutes = "0" + minutes Ptolemaic system.     your instructor Power Laws and Logarithmic Plots can you show the empty focus, Kepler's 3 Laws of Planetary Motion Illustrated can you see or hear equal areas being swept out in equal times qualitatively? Task 13: The Planetary Orbit Simulator and a Logarithmic Plot: Also outside the circle of the FOV area, append it to the     Then you switch to the smaller eyepiece. If the astronomical objects are NOT named planet EVERYONE in the group must do the task for themselves. and 45--47°     Yes / No / Maybe Read the above subsections     Y / N Select y axis     Y / N End of Task the Ptolemaic system---from End of Task Sub Tasks: chooses and draw diagrams of those he/she chooses with Moon. Since you are an RMI student, one just observes the light curve of Mercury, A quadrature is: (local link / (local link / and orbit names out to Select x axis EVERYONE in the group must do this task for themselves. measure absolute distances beyond the print out the white background sky map.     More signal noise should make the field of view (FOV) diagrams planetary rings, Task 18: Exoplanet Mean Orbital Radius and Orbital Period: south, Push all the buttons on order of magnitude? HINT: Push all the buttons. Read over End of Task practitioners. Epicycle, Ptolemaic Read over     Y / N general link: copernican_system.html) which has the formula inner Solar System mass),     ___________________________ Have you read it?     general link: naap_radial_velocity_simulator.html). Launch TheSky     was worked out in great detail by Ptolemy, Ptolemaic system End of Task Task 20: Planet Observations Push all the buttons on See Table: C8 Telescope Specifications for Available Eyepieces. How does changing the planet Universal Time (UT) to your If there is only one sky map per group, east, EVERYONE in the group must do this task for themselves.     Y / N The Discovery of Exoplanets by Doppler Spectroscopy) (or your observing night) Set the date to today's date & time: and log scale. Push all the buttons of Did you succeed in getting a printout of the Power Laws and Logarithmic Plots, which has the formula     Y / N measure absolute distances beyond the measured The set of points on the favorite report form.     Y / N Y / N shown in the figure below Have you read it? planetary rings,     Y / N the planetary orbit simulator     Y / N you can wait a few days at least for a night with good enough Print out as many     Y / N including their embedded figures. and log scale. With parameters set for eclipsing it. Task 16: The Exoplanet Transit Simulator: Newtonian features tab, can you make the velocity and linear scale (i.e., non-log scale). line? (local link / //--> NAAP: Exoplanet Radial Velocity Simulator As Time Goes By (1931), _______________________________________________________________________________________ Outside the circle of the FOV area, End of Task affect Your truly suggests using the standard 40-mm eyepiece shown in the figure below naked eye. Doppler effect videos). circle was then called an epicycle,and the second a deferent. More signal noise should make the Using the Kepler's 3rd law tab, inferior planet? Can you make simulator show the motion of an So how could Copernicus     Y / N can you make all the planets with inclination equal 90°? line? they are sufficiently bright, Using the Kepler's 2nd law tab, Start the animation. You'll need to know that the linear scale plot, The focus is on and Mars, but NOT FOV area. they are above the horizon Push all the buttons on was revealed to Copernicus: celestial sphere) directions: First, read the subsection For the sketches of the FOV, R is the mean orbital radius nearest to today's eclipsing it. predict the mean orbital radii was the main argument for heliocentrism. Answer: The Discovery of Exoplanets by Doppler Spectroscopy) for one diagram and a 18-mm Why does it have this effect? general link: naap_planetary_orbit_simulator.html). Ptolemaic system. a little explication is needed to understand it for our purposes. Have you watched them? Answer: // End of Task approximately with the most interesting to look at---which if they are in the sky instructor directs. Start the animation. Print out the sky map figure below the structure of the Solar System     Answer: For example, 10**(-1) to 10**2 AU. which has the formula (local link /     Y / N affect You will see what an astronomer did - not at all what a modern one does - and     Y / N requires and append them to the instructor get the correct order and correct relative orbital radii of Push all the buttons of observed planet for fun.     Y / N Answer: Sub Tasks:     Y / N HINT: The short answer is expected. P=[2π/(GM)**(1/2)]*R**(3/2) , for your observing day and If you don't want to print after seeing the Preview, go north, telescope magnification, planets Y / N     symmetry of its parts.     Y / N Task 12: The Planetary Orbit Simulator: sky map? curve on the plot? range for known exoplanets to in the applet figure above What kind of plot is shown:     Y / N mass (assumed much larger than the So you can approximately figure out observations worse?     Y / N which is from Copernicus' of the Earth's orbit) perpendicular to the through the line perpendicular to its symmetry plane. and provide you with the theoretical toolkit possessed by a practitioner of Using the Kepler's 2nd law tab, observing time. eyepiece for the second diagram. are elucidated in the figure below (local link / The Discovery of Exoplanets by Doppler Spectroscopy) Can you start the animation, can you see or hear equal areas being swept out in equal times qualitatively? Push all the buttons to see what they do.     Yes / No / Maybe local link / Take a cell phone image of the and linear scale (i.e., non-log scale). a star. the size. Sub Tasks: Also outside the circle of the FOV area, through the line perpendicular to its symmetry plane. What happens to the radial velocity transits. (local link / and log scale. and put the elongation values which has the formula Read the above subsections (IPI only):     ______________________________ observed planet for fun. of the planets in their shown in the figure below     Y / N     Y / N Using the Kepler's 2nd law tab, Tychonic system east, is the zero point of the epicycle theory the most interesting to look at---which if they are in the sky What happens as you change the // $("#date_creamer_24h_html").load("/~jeffery/astro/date/date_creamer_24h.html" ); // Works. the NAAP: Exoplanet Radial Velocity Simulator He did not concern himself with the nature of general link: naap_ptolemaic_system_simulator.html.html) _______________________________________________________________________________________ general link: copernican_system.html) since they go beyond the basic and in particular look for the Do most discovered exoplanets What happens to the radial velocity illustrating End of Task universe or R is the mean orbital radius Earth-Sun line What planets can we see for sure tonight click off Answer: epicycle system---many roughly equally good No one could until the 17th century FOV diagram. requires and append them to the Take a cell phone image of the     . they are sufficiently bright, Can you change the signal noise?     Y / N Sky Maps by Ordinal Date     shown in the applet figure below The cord can be rotated by clicking and dragging the weight on the end. The fact that most points on and 45--47° orbital period to see what they do. The Doppler Effect). Power Laws and Logarithmic Plots,

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