1 00:00:00,790 --> 00:00:08,320 [Music] 2 00:00:14,509 --> 00:00:11,990 hey everyone your favorite astronomy 3 00:00:17,269 --> 00:00:14,519 education guys back and for those you 4 00:00:18,710 --> 00:00:17,279 who those who are new and we're not did 5 00:00:21,920 --> 00:00:18,720 not see me last year don't worry I'll be 6 00:00:24,230 --> 00:00:21,930 your favorite very soon so I'm Dani 7 00:00:25,790 --> 00:00:24,240 behringer I'm a graduate student at Penn 8 00:00:28,460 --> 00:00:25,800 State in the department of curriculum 9 00:00:30,050 --> 00:00:28,470 and instruction now had a bit of a weird 10 00:00:32,089 --> 00:00:30,060 path through grad school you can totally 11 00:00:33,139 --> 00:00:32,099 talk to me about that later I'm going to 12 00:00:34,790 --> 00:00:33,149 be telling you about some of the work 13 00:00:36,830 --> 00:00:34,800 I've been doing I started doing it with 14 00:00:39,170 --> 00:00:36,840 Chris Palma but this past semester Rick 15 00:00:42,410 --> 00:00:39,180 do Shiell has gotten involved as well 16 00:00:44,330 --> 00:00:42,420 with the the really in-depth part of the 17 00:00:46,190 --> 00:00:44,340 development of this coherent content 18 00:00:48,770 --> 00:00:46,200 storyline on exoplanets I'm going to 19 00:00:50,869 --> 00:00:48,780 tell you about the first may give you a 20 00:00:52,670 --> 00:00:50,879 bit of a summary of what I talked about 21 00:00:56,180 --> 00:00:52,680 last year because this is all relevant 22 00:01:00,110 --> 00:00:56,190 so I'm developing a course for Penn 23 00:01:02,900 --> 00:01:00,120 State called Astro 850 which is a course 24 00:01:05,509 --> 00:01:02,910 that is designed for pre-service high 25 00:01:06,950 --> 00:01:05,519 school teachers on exoplanets that is 26 00:01:09,890 --> 00:01:06,960 going to be an elective course they can 27 00:01:14,539 --> 00:01:09,900 take as part of the immediate earth 28 00:01:16,760 --> 00:01:14,549 science program online and asteroid 50 29 00:01:18,710 --> 00:01:16,770 is designed to use activities designed 30 00:01:20,270 --> 00:01:18,720 around this claims evidence reasoning 31 00:01:23,330 --> 00:01:20,280 framework that sunny very briefly 32 00:01:26,060 --> 00:01:23,340 outlined for you and to engage students 33 00:01:27,469 --> 00:01:26,070 in authentic science practices I'll tell 34 00:01:29,630 --> 00:01:27,479 you a bit more about that later because 35 00:01:32,420 --> 00:01:29,640 it comes particularly relevant when we 36 00:01:36,140 --> 00:01:32,430 start talking about NGSS next generation 37 00:01:37,819 --> 00:01:36,150 science standards so for this talk I'm 38 00:01:40,490 --> 00:01:37,829 going to start by telling you what is a 39 00:01:44,749 --> 00:01:40,500 current content storyline in more detail 40 00:01:46,399 --> 00:01:44,759 and why does it matter then move on to 41 00:01:48,230 --> 00:01:46,409 the next generation Stein standards 42 00:01:51,770 --> 00:01:48,240 because this is a course that is being 43 00:01:53,719 --> 00:01:51,780 built for high school teachers it's 44 00:01:56,510 --> 00:01:53,729 incredibly important that we're 45 00:01:59,389 --> 00:01:56,520 including and taking into account the 46 00:02:02,300 --> 00:01:59,399 standards that high school students are 47 00:02:05,179 --> 00:02:02,310 going to be held to and then I'll talk a 48 00:02:08,180 --> 00:02:05,189 little bit about running these activity 49 00:02:10,400 --> 00:02:08,190 based courses in an online setting I had 50 00:02:12,740 --> 00:02:10,410 a little bit of practice doing this with 51 00:02:13,610 --> 00:02:12,750 the introductory lab class that I ran 52 00:02:16,250 --> 00:02:13,620 this past 53 00:02:18,740 --> 00:02:16,260 semester it was an in-person class in 54 00:02:20,809 --> 00:02:18,750 Italy but for some of the activities I 55 00:02:22,490 --> 00:02:20,819 admittedly use them as guinea pigs I 56 00:02:24,229 --> 00:02:22,500 mean what was worse that was going to 57 00:02:25,699 --> 00:02:24,239 happen so my last semester tieng are 58 00:02:28,160 --> 00:02:25,709 they going to like give me bad teach me 59 00:02:33,050 --> 00:02:28,170 reviews or something no this actually 60 00:02:35,170 --> 00:02:33,060 seem to enjoy them so why use a coherent 61 00:02:37,940 --> 00:02:35,180 content storyline and what really is it 62 00:02:40,640 --> 00:02:37,950 so the idea of a coherent content 63 00:02:44,569 --> 00:02:40,650 storyline goes back to a 2006 study 64 00:02:45,770 --> 00:02:44,579 which looked at a particular data set 65 00:02:49,250 --> 00:02:45,780 called the trends in international 66 00:02:53,740 --> 00:02:49,260 mathematics and science study TI MSS 67 00:02:57,199 --> 00:02:53,750 Tim's comparing the education or the 68 00:03:00,430 --> 00:02:57,209 instruction basically across a number of 69 00:03:03,949 --> 00:03:00,440 countries the video evidence showed that 70 00:03:06,559 --> 00:03:03,959 the United States compared to other 71 00:03:13,300 --> 00:03:06,569 high-performing countries while there 72 00:03:16,039 --> 00:03:13,310 were a lot of activity-based lessons the 73 00:03:18,890 --> 00:03:16,049 let the activities themselves lacked a 74 00:03:21,199 --> 00:03:18,900 strong connection to those lessons they 75 00:03:24,110 --> 00:03:21,209 were kind of a bunch of activities 76 00:03:27,080 --> 00:03:24,120 mashed together without some driving 77 00:03:29,629 --> 00:03:27,090 force behind them some larger 78 00:03:31,460 --> 00:03:29,639 organization this leads to another 79 00:03:34,339 --> 00:03:31,470 problem that was also observed with the 80 00:03:37,400 --> 00:03:34,349 United States where you get this mile 81 00:03:38,990 --> 00:03:37,410 wide inch deep problem of trying to 82 00:03:43,879 --> 00:03:39,000 cover a lot of material but only 83 00:03:45,680 --> 00:03:43,889 covering it at a very surface level so 84 00:03:48,229 --> 00:03:45,690 coherent content storyline is 85 00:03:50,780 --> 00:03:48,239 specifically a way to plan and organize 86 00:03:52,640 --> 00:03:50,790 a course yes for those you who are here 87 00:03:54,530 --> 00:03:52,650 last year I did use this slide already 88 00:03:58,280 --> 00:03:54,540 but it's a great one so I'm going to use 89 00:04:00,860 --> 00:03:58,290 it again um for coherent content 90 00:04:03,349 --> 00:04:00,870 storyline you want to start with what is 91 00:04:05,659 --> 00:04:03,359 the big idea that I'm trying to get 92 00:04:08,150 --> 00:04:05,669 across and this is going to be some kind 93 00:04:11,629 --> 00:04:08,160 of a phenomenon or causal model 94 00:04:14,360 --> 00:04:11,639 something like that once you know what 95 00:04:16,370 --> 00:04:14,370 you want to get across to them develop 96 00:04:18,949 --> 00:04:16,380 what's called the upper anchor statement 97 00:04:21,979 --> 00:04:18,959 this is the statement of the learning 98 00:04:24,409 --> 00:04:21,989 goals for this class basically what do I 99 00:04:26,750 --> 00:04:24,419 want the students to know coming out of 100 00:04:29,450 --> 00:04:26,760 my class 101 00:04:30,920 --> 00:04:29,460 there of course you can delve into okay 102 00:04:33,380 --> 00:04:30,930 to understand these why are the course 103 00:04:35,690 --> 00:04:33,390 topics going to be and then around those 104 00:04:37,850 --> 00:04:35,700 plan out the lessons activities this 105 00:04:40,100 --> 00:04:37,860 ensures that these lessons and 106 00:04:44,480 --> 00:04:40,110 activities are all going to be related 107 00:04:47,270 --> 00:04:44,490 back to this big idea more importantly 108 00:04:49,190 --> 00:04:47,280 perhaps is the way they build on one 109 00:04:51,590 --> 00:04:49,200 another this is the example of the 110 00:04:55,490 --> 00:04:51,600 storyline that I have been working on 111 00:04:58,160 --> 00:04:55,500 starting with the basic question of how 112 00:05:01,280 --> 00:04:58,170 do we know that exoplanets are common in 113 00:05:04,070 --> 00:05:01,290 the universe in our in our galaxy and so 114 00:05:06,530 --> 00:05:04,080 forth it all starts with our solar 115 00:05:10,670 --> 00:05:06,540 system of course we look at patterns in 116 00:05:12,620 --> 00:05:10,680 the solar system things like we have 117 00:05:15,370 --> 00:05:12,630 terrestrial plants that are close to the 118 00:05:19,450 --> 00:05:15,380 Sun gas and ice giants that are far away 119 00:05:21,530 --> 00:05:19,460 everything orbits in the same plane um 120 00:05:24,380 --> 00:05:21,540 everything is orbiting in pretty much 121 00:05:26,720 --> 00:05:24,390 the same direction and rotating in most 122 00:05:29,660 --> 00:05:26,730 of the same direction with like two odd 123 00:05:31,610 --> 00:05:29,670 cases there so it tells us that we 124 00:05:36,650 --> 00:05:31,620 formed out of you guessed it based on 125 00:05:39,200 --> 00:05:36,660 all the previous talks a disk and then 126 00:05:41,270 --> 00:05:39,210 what we won't need to look at is okay 127 00:05:42,620 --> 00:05:41,280 these we see these processes occurring 128 00:05:45,350 --> 00:05:42,630 in our solar system or we see the 129 00:05:47,870 --> 00:05:45,360 evidence for them now you look elsewhere 130 00:05:50,630 --> 00:05:47,880 and see okay it looks like these 131 00:05:54,590 --> 00:05:50,640 processes really are occurring in other 132 00:05:56,420 --> 00:05:54,600 star forming systems as well cool so we 133 00:05:57,500 --> 00:05:56,430 convicts we kind of expect exoplanets to 134 00:06:00,380 --> 00:05:57,510 be everywhere but we got to figure out 135 00:06:02,900 --> 00:06:00,390 how to find them once we figure out how 136 00:06:07,430 --> 00:06:02,910 to find them we find them and holy crud 137 00:06:09,350 --> 00:06:07,440 there are a lot of them so and there are 138 00:06:12,890 --> 00:06:09,360 a lot of very strange ones so we go into 139 00:06:14,710 --> 00:06:12,900 a bit beyond just plants are common how 140 00:06:18,140 --> 00:06:14,720 did the planets get to the way they are 141 00:06:20,540 --> 00:06:18,150 so we talk about the interactions that 142 00:06:22,010 --> 00:06:20,550 occur between the bodies and planetary 143 00:06:22,970 --> 00:06:22,020 systems because this leads some really 144 00:06:25,070 --> 00:06:22,980 cool stuff and it's actually very 145 00:06:28,970 --> 00:06:25,080 relevant for our solar system as well 146 00:06:30,260 --> 00:06:28,980 and of course we want to talk about the 147 00:06:32,510 --> 00:06:30,270 thing that everybody wants to know about 148 00:06:34,370 --> 00:06:32,520 exoplanets is there life on these 149 00:06:38,180 --> 00:06:34,380 planets potentially and how would we 150 00:06:39,830 --> 00:06:38,190 look for that but first I'm going to 151 00:06:40,580 --> 00:06:39,840 give you a just brief overview about 152 00:06:42,140 --> 00:06:40,590 what 153 00:06:45,920 --> 00:06:42,150 the next generation science standards 154 00:06:48,290 --> 00:06:45,930 are all about traditionally science 155 00:06:50,810 --> 00:06:48,300 standards have just focused on these 156 00:06:52,400 --> 00:06:50,820 content areas the disciplinary core 157 00:06:55,060 --> 00:06:52,410 ideas this is the content knowledge 158 00:06:57,410 --> 00:06:55,070 stuff what you normally think of for our 159 00:07:00,400 --> 00:06:57,420 standards what do the students have to 160 00:07:02,570 --> 00:07:00,410 know more or less like factually and 161 00:07:04,100 --> 00:07:02,580 separate into three main areas life 162 00:07:05,860 --> 00:07:04,110 sciences does go science is earth 163 00:07:08,150 --> 00:07:05,870 sciences okay cool 164 00:07:11,030 --> 00:07:08,160 the next two the science and engineering 165 00:07:12,950 --> 00:07:11,040 practices and the cross-cutting concepts 166 00:07:16,880 --> 00:07:12,960 are the parts that are completely new 167 00:07:19,280 --> 00:07:16,890 for next generation science standards I 168 00:07:23,120 --> 00:07:19,290 want to get the students an idea of how 169 00:07:25,610 --> 00:07:23,130 science is done on and so some examples 170 00:07:26,630 --> 00:07:25,620 these there are actually eight science 171 00:07:28,460 --> 00:07:26,640 and engineering practices they're 172 00:07:31,420 --> 00:07:28,470 listing the full document but these just 173 00:07:36,890 --> 00:07:31,430 some examples and the cross-cutting 174 00:07:39,710 --> 00:07:36,900 concepts then are not disciplinary core 175 00:07:41,270 --> 00:07:39,720 ideas these are not your typical you 176 00:07:43,280 --> 00:07:41,280 know students to know that like the 177 00:07:46,280 --> 00:07:43,290 earth goes around the Sun these are kind 178 00:07:49,150 --> 00:07:46,290 of threads and recurring themes that 179 00:07:52,820 --> 00:07:49,160 connect your disciplinary core ideas 180 00:07:55,460 --> 00:07:52,830 across the various levels things like 181 00:07:57,980 --> 00:07:55,470 ideas about energy and matter and 182 00:08:00,830 --> 00:07:57,990 stability change in patterns and things 183 00:08:02,830 --> 00:08:00,840 like that so now you're all experts on 184 00:08:09,550 --> 00:08:02,840 the next generation science standards 185 00:08:13,780 --> 00:08:09,560 how do exoplanets fit into and GSS well 186 00:08:16,070 --> 00:08:13,790 unfortunately not strictly speaking 187 00:08:17,930 --> 00:08:16,080 because of course exoplanets are an 188 00:08:20,770 --> 00:08:17,940 incredibly new field that really haven't 189 00:08:22,940 --> 00:08:20,780 made their way into curricula below like 190 00:08:26,480 --> 00:08:22,950 introductory level astronomy at the 191 00:08:29,450 --> 00:08:26,490 college level so why should teachers 192 00:08:32,360 --> 00:08:29,460 care about that main thing to note is 193 00:08:35,120 --> 00:08:32,370 that standards are not necessarily a 194 00:08:39,340 --> 00:08:35,130 list of the ways in which you should 195 00:08:43,010 --> 00:08:39,350 teach your students something instead 196 00:08:44,900 --> 00:08:43,020 using exoplanets to talk about these in 197 00:08:47,960 --> 00:08:44,910 this case the disciplinary core ideas 198 00:08:50,360 --> 00:08:47,970 that I've listed here provides another 199 00:08:52,880 --> 00:08:50,370 context looking at them entirely and 200 00:08:53,930 --> 00:08:52,890 connects them in completely different 201 00:08:56,560 --> 00:08:53,940 ways than you 202 00:09:01,600 --> 00:08:56,570 would see just by following you know the 203 00:09:09,260 --> 00:09:05,530 secondly I'm referring to the 204 00:09:11,810 --> 00:09:09,270 cross-cutting concepts the two that I 205 00:09:14,060 --> 00:09:11,820 focused on the most in developing the 206 00:09:15,850 --> 00:09:14,070 curriculum for aster 850 were patterns 207 00:09:18,530 --> 00:09:15,860 and ideas of stability and change 208 00:09:21,320 --> 00:09:18,540 patterns are incredibly important to our 209 00:09:23,120 --> 00:09:21,330 detection of exoplanets because as you 210 00:09:25,790 --> 00:09:23,130 can see in like this sample light curve 211 00:09:27,950 --> 00:09:25,800 you're looking for a pattern a recurring 212 00:09:29,870 --> 00:09:27,960 decrease in the brightness of a star 213 00:09:31,910 --> 00:09:29,880 that indicates that there is they plant 214 00:09:33,170 --> 00:09:31,920 it transiting in front of it of course 215 00:09:34,580 --> 00:09:33,180 there's a little bit more work to figure 216 00:09:36,140 --> 00:09:34,590 out that's actually your planet and all 217 00:09:38,930 --> 00:09:36,150 but I'll leave that up to the people 218 00:09:43,250 --> 00:09:38,940 with the really fancy radial velocity 219 00:09:45,470 --> 00:09:43,260 instruments and stability and change so 220 00:09:47,750 --> 00:09:45,480 while our solar system now is very 221 00:09:50,210 --> 00:09:47,760 stable and everything is pretty much set 222 00:09:53,930 --> 00:09:50,220 in its orbit it wasn't always the case 223 00:09:58,640 --> 00:09:53,940 on the nice model which is illustrated 224 00:10:05,000 --> 00:09:58,650 here basically demonstrates that about 225 00:10:07,400 --> 00:10:05,010 what was it a few a few hundreds of 226 00:10:10,220 --> 00:10:07,410 millions of years into the formation of 227 00:10:13,610 --> 00:10:10,230 the solar system things went completely 228 00:10:15,050 --> 00:10:13,620 haywire um Uranus went from being the 229 00:10:17,900 --> 00:10:15,060 eighth planet orbiting the Sun to the 230 00:10:19,760 --> 00:10:17,910 seventh and kicked out a whole bunch of 231 00:10:23,210 --> 00:10:19,770 comets and things like that 232 00:10:24,560 --> 00:10:23,220 essentially planetary leftovers that 233 00:10:28,700 --> 00:10:24,570 eventually went on to form the Oort 234 00:10:31,420 --> 00:10:28,710 cloud and this also change where the 235 00:10:34,100 --> 00:10:31,430 orbits of the planets were it could have 236 00:10:35,870 --> 00:10:34,110 completely different consequences in 237 00:10:38,660 --> 00:10:35,880 terms of these shapes of the orbits but 238 00:10:42,320 --> 00:10:38,670 in our case most the orbits actually 239 00:10:44,210 --> 00:10:42,330 turned out to be fairly circular and the 240 00:10:46,130 --> 00:10:44,220 claims evidence reasoning framework the 241 00:10:48,790 --> 00:10:46,140 way that we are developing all the 242 00:10:50,660 --> 00:10:48,800 activities are really I am admittedly 243 00:10:54,220 --> 00:10:50,670 developing the activities for this 244 00:10:57,890 --> 00:10:54,230 course is a way that students can engage 245 00:11:00,230 --> 00:10:57,900 with actual like data or observations 246 00:11:02,720 --> 00:11:00,240 the example I'm showing here is this 247 00:11:05,570 --> 00:11:02,730 little web game called super planet 248 00:11:07,519 --> 00:11:05,580 crash if you haven't heard of it check 249 00:11:10,540 --> 00:11:07,529 it out it's addictively fun 250 00:11:14,960 --> 00:11:10,550 but what I have the students do here is 251 00:11:16,939 --> 00:11:14,970 you have planets orbiting this star you 252 00:11:18,949 --> 00:11:16,949 can adjust the mass of the inserted 253 00:11:20,929 --> 00:11:18,959 planet and you get a higher score when 254 00:11:23,920 --> 00:11:20,939 you use more massive objects but 255 00:11:27,610 --> 00:11:23,930 throwing a lot of massive objects into a 256 00:11:29,960 --> 00:11:27,620 you know to AU distance from a star 257 00:11:35,869 --> 00:11:29,970 obviously makes things go a little 258 00:11:38,360 --> 00:11:35,879 unstable so the goal here for this game 259 00:11:40,489 --> 00:11:38,370 is to try to create a stable system and 260 00:11:43,009 --> 00:11:40,499 what I have the students do is play 261 00:11:45,650 --> 00:11:43,019 around with this and look at what our 262 00:11:49,249 --> 00:11:45,660 the conditions that you're developing or 263 00:11:51,410 --> 00:11:49,259 your observing for stability in these 264 00:11:56,840 --> 00:11:51,420 systems and why is that going to be the 265 00:11:59,299 --> 00:11:56,850 case now on to the very last part the 266 00:12:01,480 --> 00:11:59,309 dealing with these kinds of activities 267 00:12:05,509 --> 00:12:01,490 in an online setting 268 00:12:08,119 --> 00:12:05,519 traditionally um students will write up 269 00:12:10,579 --> 00:12:08,129 claims evidence and reasoning and your 270 00:12:12,230 --> 00:12:10,589 group and present that to the class 271 00:12:14,389 --> 00:12:12,240 generally they'll write it on a 272 00:12:17,720 --> 00:12:14,399 whiteboard the term that's used in a lot 273 00:12:20,059 --> 00:12:17,730 of papers is the board meeting but the 274 00:12:22,429 --> 00:12:20,069 write up on a whiteboard and they talk 275 00:12:25,819 --> 00:12:22,439 about you know this is what we observe 276 00:12:28,610 --> 00:12:25,829 this is what we found and they get 277 00:12:32,019 --> 00:12:28,620 critique on it from other students this 278 00:12:35,720 --> 00:12:32,029 is scientific argumentation in practice 279 00:12:37,610 --> 00:12:35,730 moving the discussions online of course 280 00:12:40,549 --> 00:12:37,620 changes a lot of this because you don't 281 00:12:44,900 --> 00:12:40,559 have the face-to-face interactions and 282 00:12:48,769 --> 00:12:44,910 you have to switch to a more written 283 00:12:50,480 --> 00:12:48,779 style of critique argumentation then you 284 00:12:52,790 --> 00:12:50,490 would have in a normal face-to-face 285 00:12:54,590 --> 00:12:52,800 class which is usually where claims 286 00:12:58,160 --> 00:12:54,600 evidence reasoning type activities are 287 00:13:00,740 --> 00:12:58,170 used one interesting thing that this 288 00:13:04,249 --> 00:13:00,750 does though is as I noticed it gives you 289 00:13:06,679 --> 00:13:04,259 a window into the thinking of the 290 00:13:10,850 --> 00:13:06,689 students that are making the arguments 291 00:13:14,269 --> 00:13:10,860 both in terms of presenting what they 292 00:13:15,829 --> 00:13:14,279 determined and students who are maybe 293 00:13:19,220 --> 00:13:15,839 arguing against the way that they 294 00:13:20,770 --> 00:13:19,230 grouped you know the gas and ice giants 295 00:13:23,780 --> 00:13:20,780 separately 296 00:13:27,470 --> 00:13:23,790 the last thing of course is deadlines 297 00:13:30,290 --> 00:13:27,480 because this is not face to face you 298 00:13:35,150 --> 00:13:30,300 need to make sure that students have you 299 00:13:39,740 --> 00:13:35,160 know provide feedback on the your other 300 00:13:41,630 --> 00:13:39,750 students work by this time because then 301 00:13:46,850 --> 00:13:41,640 the students need to be able to respond 302 00:13:49,970 --> 00:13:46,860 to the critiques of their work so I'll 303 00:13:52,930 --> 00:13:49,980 leave my summary slide up here and I 304 00:14:03,080 --> 00:13:52,940 will take questions at this time thank 305 00:14:10,140 --> 00:14:06,300 so Danny you mentioned that exoplanets 306 00:14:13,410 --> 00:14:10,150 don't fit into the NGSS system strand Li 307 00:14:16,410 --> 00:14:13,420 speak strictly speaking and so are you 308 00:14:18,570 --> 00:14:16,420 envisioning that instructors will go out 309 00:14:20,040 --> 00:14:18,580 of their way to sort of convolute the 310 00:14:21,690 --> 00:14:20,050 system so that they can talk about 311 00:14:25,440 --> 00:14:21,700 exoplanets in particular or are you 312 00:14:27,720 --> 00:14:25,450 using it as sort of a where in the 313 00:14:30,090 --> 00:14:27,730 curriculum do you see exoplanets fitting 314 00:14:33,690 --> 00:14:30,100 I see it as a way to grab students 315 00:14:36,480 --> 00:14:33,700 attention frankly um let's face it 316 00:14:38,910 --> 00:14:36,490 exoplanets are really cool they're one 317 00:14:40,770 --> 00:14:38,920 of the most interesting fields right now 318 00:14:43,350 --> 00:14:40,780 because it's growing incredibly fast and 319 00:14:45,360 --> 00:14:43,360 planets unlike a whole lot of the other 320 00:14:47,790 --> 00:14:45,370 stuff in astronomy is something that we 321 00:14:51,110 --> 00:14:47,800 can relate to very directly being on a 322 00:14:53,730 --> 00:14:51,120 planet ourselves so thinking about that 323 00:14:56,400 --> 00:14:53,740 there are other planets out there what 324 00:14:58,680 --> 00:14:56,410 about other planets with life out there 325 00:15:01,950 --> 00:14:58,690 is just one of the most fundamental 326 00:15:06,030 --> 00:15:01,960 questions of our existence and you can 327 00:15:07,950 --> 00:15:06,040 bring that into a classroom context just 328 00:15:10,100 --> 00:15:07,960 on the fact that students can find it 329 00:15:13,100 --> 00:15:10,110 more interesting than maybe you know 330 00:15:15,900 --> 00:15:13,110 rehashing the same things about Earth 331 00:15:17,910 --> 00:15:15,910 but they give you opportunity to sound 332 00:15:20,750 --> 00:15:17,920 all of those same disciplinary core 333 00:15:23,820 --> 00:15:20,760 ideas you would be hitting otherwise um 334 00:15:31,990 --> 00:15:23,830 just doing it with a slightly different 335 00:15:43,760 --> 00:15:41,510 one in the back Bradley alright so 336 00:15:46,070 --> 00:15:43,770 piggybacking on that question so are you 337 00:15:48,020 --> 00:15:46,080 envisioning this as a semester kind of 338 00:15:49,990 --> 00:15:48,030 course or is it going to be something 339 00:15:53,660 --> 00:15:50,000 that you would you know plug in into 340 00:15:55,700 --> 00:15:53,670 certain classes like patterns you know 341 00:15:57,710 --> 00:15:55,710 you put it into a physics class and the 342 00:16:01,640 --> 00:15:57,720 chapter and you know you give a case 343 00:16:04,040 --> 00:16:01,650 study almost okay so a350 itself is on a 344 00:16:06,350 --> 00:16:04,050 course on its own but the idea of the 345 00:16:09,440 --> 00:16:06,360 activities is that they can kind of slot 346 00:16:12,260 --> 00:16:09,450 into a course individually these are 347 00:16:14,090 --> 00:16:12,270 things that really we want teachers to 348 00:16:15,530 --> 00:16:14,100 be able to take into their own 349 00:16:18,200 --> 00:16:15,540 classrooms which is why it's so 350 00:16:20,840 --> 00:16:18,210 important that they're NGSS aligned in 351 00:16:23,240 --> 00:16:20,850 things like that ideally it would be 352 00:16:26,510 --> 00:16:23,250 kind of a curriculum unit that you do 353 00:16:28,820 --> 00:16:26,520 all together you know in sequence so 354 00:16:31,160 --> 00:16:28,830 you're not breaking up this you know 355 00:16:34,310 --> 00:16:31,170 coherent content storyline that I've put 356 00:16:36,440 --> 00:16:34,320 together but really if you just want to 357 00:16:39,620 --> 00:16:36,450 you know take out a particular part of 358 00:16:49,760 --> 00:16:39,630 this and use it by all means that's 359 00:16:52,370 --> 00:16:49,770 totally fine with me so this can 360 00:16:54,860 --> 00:16:52,380 coherent content storyline can this be 361 00:16:57,560 --> 00:16:54,870 scaled down to a single lecture for 362 00:17:00,200 --> 00:16:57,570 someone who's like a TA for a larger 363 00:17:02,120 --> 00:17:00,210 course who needs to stay on a stricter 364 00:17:04,640 --> 00:17:02,130 schedule could they incorporate some of 365 00:17:08,870 --> 00:17:04,650 these ideas to you know enhance their 366 00:17:14,420 --> 00:17:08,880 own lectures I'm not going to say no to 367 00:17:16,340 --> 00:17:14,430 that so the main thing to take away from 368 00:17:19,850 --> 00:17:16,350 that if you're scaling it down to you 369 00:17:24,500 --> 00:17:19,860 know a single classes worth of material 370 00:17:26,050 --> 00:17:24,510 is to come up with what do you want 371 00:17:29,600 --> 00:17:26,060 students to get out of this particular 372 00:17:31,340 --> 00:17:29,610 you know lecture activity or lecture 373 00:17:33,770 --> 00:17:31,350 plus activity whatever it happens to be 374 00:17:35,930 --> 00:17:33,780 and make sure you're playing around that 375 00:17:36,620 --> 00:17:35,940 with that in mind throughout the entire 376 00:17:40,360 --> 00:17:36,630 process 377 00:17:43,640 --> 00:17:40,370 um spell out what those connections are 378 00:17:44,630 --> 00:17:43,650 it's not like the your learning goal is 379 00:17:47,050 --> 00:17:44,640 some 380 00:17:49,310 --> 00:17:47,060 thing that the students never get to see 381 00:17:50,870 --> 00:17:49,320 ideally they should know exactly what 382 00:17:53,870 --> 00:17:50,880 they're working towards the entire time 383 00:17:57,260 --> 00:17:53,880 that's what you start with actually day 384 00:17:59,570 --> 00:17:57,270 one of a class for a straight fifty 385 00:18:02,480 --> 00:17:59,580 students will be introduced to like the 386 00:18:04,940 --> 00:18:02,490 Keppler or e because it shows a lot of 387 00:18:06,920 --> 00:18:04,950 planets and the diversity of the systems 388 00:18:08,540 --> 00:18:06,930 that Kepler is found of course it's not 389 00:18:11,300 --> 00:18:08,550 complete because we found planets other 390 00:18:15,580 --> 00:18:11,310 ways but they'll get all of these as 391 00:18:18,410 --> 00:18:15,590 caveats as well um but scaling it down 392 00:18:20,450 --> 00:18:18,420 I'd say works on that level just make 393 00:18:29,950 --> 00:18:20,460 sure that things are consistent and