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RST.11-12.7Common CoreELALiteracy in Science and Technical SubjectsGrades 11-12

RST.11-12.7: Integrating and Evaluating Science Sources in Diverse Formats and Media

In plain English: RST.11-12.7 is the Common Core ELA standard that asks students in grades 11-12 to integrate and evaluate multiple sources of information in diverse formats and media, such as quantitative data, video and multimedia, to address a question or solve a problem. Students combine data, text and visuals into one answer and judge how far each source can be trusted.

Integrate and evaluate multiple sources of information presented in diverse formats and media (e.g., quantitative data, video, multimedia) in order to address a question or solve a problem.

Common Core State Standards for English Language Arts & Literacy · Domain: Reading Standards for Literacy in Science and Technical Subjects 6-12 · Cluster: Integration of Knowledge and Ideas · Official standard

01

Lesson Plan

60-65 min

Overview

Real scientific questions are answered from many sources at once: a report, its data tables, a graph, a video explanation and a reference value. RST.11-12.7 asks students to integrate and evaluate multiple sources of information presented in diverse formats and media, such as quantitative data, video and multimedia, in order to address a question or solve a problem. This lesson poses one question, How fast does light travel, and how far can we trust Albert Michelson's 1880 answer?, and gives students seven sources in four formats: Michelson's own report (published in 1880), his table of 100 readings drawn as a histogram, his grouped results, a table of modern reference values, a transcript of an online video written for this page, and, for the homework, Robert S. Ball's The Story of the Heavens (1900 edition) and a modern fact card.

Students put numbers from different sources on one scale, check each claim against the source best placed to settle it, and judge which source to trust for which part of the answer. They test how close Michelson's result came to today's value, whether it fell inside the error limit he stated, and whether the video reports that point correctly. The video and the activity scenarios are invented for teaching.

Learning Objectives

By the end of this lesson, students will be able to:

  • Integrate information from text, data tables, graphs and video into one answer to a scientific question, citing each source
  • Put quantities from different sources on a common scale, with the same units and conditions, before comparing them
  • Evaluate each source for accuracy, completeness and design, checking its claims against the source best placed to settle them
  • Use the integrated and evaluated sources to solve a quantitative problem and explain which source they trust for each number

Prior Knowledge Required

Students should already be comfortable with:

  • Translating technical information between words, tables, charts and equations RST.9-10.7
  • Comparing findings in a text with those from other sources RST.9-10.9
  • Reading histograms and computing a mean and a percent difference
  • Speed as distance divided by time, and unit conversion

Lesson Procedure

60-65 minutes of class time across 5 phases.

  1. Warm-Up5 minutes

    Project three statements about one question, "How long does the school's late bus take to get home?": a bus company brochure ("about 20 minutes"), a student's phone timer log for five rides (24, 31, 22, 27 and 26 minutes), and a parent's short video of the bus stuck behind a train.

    Warm-Up Prompt

    Using all three sources, what would you tell a new student, and which source did you trust most for the number? Write two sentences.

    Take answers. Strong ones use the log for the number (a mean of 26 minutes, from 22 to 31), use the video to explain the slow days, and treat the brochure's 20 minutes as a best case the log does not support. Tell students that this is today's skill. RST.11-12.7 asks them to integrate and evaluate multiple sources of information presented in diverse formats and media, such as quantitative data, video and multimedia, in order to address a question or solve a problem. Integrating means combining the sources into one answer; evaluating means judging what each source is good for and where it is wrong.

  2. Direct Instruction15-20 minutes

    Part 1: The question and the sources. Today's question is How fast does light travel, and how far can we trust the answer Albert Michelson published in 1880? Michelson, then a young instructor at the U.S. Naval Academy in Annapolis, timed light over a baseline of about 2,000 feet with a rapidly turning mirror. Students will integrate seven sources in four formats: Michelson's own text (Sources 1 and 3), his data tables (Source 2: Diagram 1 and the table below), an online video (Source 4), a table of modern reference values (Source 5), and, in the homework, a 1900 astronomy book and a modern fact card (Sources 6 and 7). Post the four moves:

    1. State the question, and what each source can contribute to it.
    2. Put the numbers on one scale: same units, same conditions (in air or in a vacuum, before or after corrections).
    3. Check each claim against the source best placed to settle it.
    4. Weigh the sources: say which you trust for which part of the answer, and why.

    These experiments, made with very crude apparatus and under great difficulties, gave the following table of results for the velocity of light in miles per second:

    186730
    188820
    186330
    185330
    187900
    184500
    186770
    185000
    185800
    187940
    ------
    Mean 186500 ± 300 miles per second,
    or 300140 kilometers per second.

    In the following July the sum of $2,000 was placed at my disposal by a private gentleman for carrying out these experiments on a large scale. Before ordering any of the instruments, however, it was necessary to find whether or not it was practicable to use a large distance. With a distance (between the revolving and the fixed mirror) of 500 feet, in the preliminary experiments, the field of light in the eye-piece was somewhat limited, and there was considerable indistinctness in the image, due to atmospheric disturbances.

    Accordingly, the same lens (39 feet focus) was employed, being placed, together with the other pieces of apparatus, along the north sea-wall of the Academy grounds, the distance being about 2,000 feet. The image of the slit, at noon, was so confused as not to be recognizable, but toward sunset it became clear and steady, and measurements were made of its position, which agreed within one one-hundredth of a millimeter. It was thus demonstrated that with this distance and a deflection of 100 millimeters this measurement could be made within the ten-thousandth part.

    In order to obtain this deflection, it was sufficient to make the mirror revolve 250 times per second and to use a "radius" of about 30 feet. In order to use this large radius (distance from slit to revolving mirror), it was necessary that the mirror should be large and optically true; also, that the lens should be large and of great focal length. Accordingly the mirror was made 1¼ inches in diameter, and a new lens, 8 inches in diameter, with a focal length of 150 feet was procured.

    [...]

    The first observation with the new lens was made January 30, 1879. The deflection was 70 millimeters. The image was sufficiently bright to be observed without the slightest effort. The first observation with the new micrometer eye-piece was made April 2, the deflection being 115 millimeters.

    The first of the final series of observations was made on June 5. All the observations previous to this, thirty sets in all, were rejected. After this time, no set of observations nor any single observation was omitted.

    Albert A. Michelson, Experimental Determination of the Velocity of Light, from the Introduction (Source 1; excerpt, cuts marked [...]) (1880). Public domain (published 1880). Source text.
    Source 2, part B: Michelson's table of results for groups of observations, velocity of light in air in km/s, as printed in 1880 (number of sets in parentheses). Part A is Diagram 1, drawn from his table of all 100 readings.
    Group of observationsResult
    Electric light (1 set)299850
    Set micrometer counting oscillations (2)299840
    Readings taken by Lieutenant Nazro (3)299830
    Readings taken by Mr. Clason (5)299860
    Mirror inverted (8)299840
    Speed of rotation, 192 (7)299990
    Speed of rotation, 128 (1)299800
    Speed of rotation, 96 (1)299810
    Speed of rotation, 64 (1)299870
    Radius, 28.5 feet (54)299870
    Radius, 33.3 feet (46)299830
    Highest temperature, 90° Fahr. (5)299910
    Mean of lowest temperatures, 60° Fahr. (7)299800
    Image, good (46)299860
    Image, fair (39)299860
    Image, poor (15)299810
    Frame, inclined (5)299960
    Greatest value300070
    Least value299650
    Mean value299852
    Average difference from mean60
    Value found for π3.26
    Probable error± 5
    Source 5: Modern reference values used in this lesson
    QuantityValue
    Speed of light in a vacuum (exact, since the definition of the meter adopted in 1983)299,792.458 km/s, about 186,282 miles per second
    One mile1.609344 km (exact)
    One foot0.3048 m (exact)
    Index of refraction of air near sea level and room temperatureabout 1.0003, so light in air is about 90 km/s slower than in a vacuum
    • Integrating a text with the data inside it (Source 1, paragraphs 1-2)

      Michelson prints ten results from 1878 and says they came from "very crude apparatus." Check his mean and his conversion, and say what the ten numbers add to his words.

      Result: The ten values add to 1,865,120, so the mean is 186,512 miles per second, which he rounds to 186,500. Converting with Source 5: 186,500 × 1.609344 ≈ 300,143 km/s, matching his 300,140. The numbers show what "crude" means: single trials run from 184,500 to 188,820, a spread of 4,320 miles per second, more than 2 percent of the mean. The words tell a reader the method was rough; the data tell how rough, and paragraphs 3-5 then explain the changes (a longer baseline of about 2,000 feet and a larger deflection) that were meant to fix it.

    • Putting three sources on one scale (Diagram 1, Source 3, Source 5)

      Diagram 1 shows the 100 readings as Michelson recorded them. Where does today's speed of light belong on that scale, and what does its position tell you about the kind of error in the 1879 result?

      Result: The readings are speeds in air before corrections. Source 3 adds +12 km/s for temperature and +80 km/s to go from air to a vacuum, 92 km/s in all. To compare like with like, subtract the same 92 from today's vacuum value: 299,792.458 - 92 ≈ 299,700 km/s. Only 2 of the 100 readings (299,620 and 299,650) lie below that line. If the method had only random error, the readings would scatter on both sides of the true value; instead almost the whole set sits high. That is a systematic error, and averaging more readings could not have removed it. No single source shows this: it takes the data, Michelson's corrections and the modern value together.

    Close the model: the integrated answer is not a list of what each source says. It is one claim ("Michelson's readings were precise but sat about 150 km/s high") that no single source makes, supported by all three.

  3. Guided Practice15 minutes

    Pairs read the video transcript (Source 4), written for this page, and mark each statement C (can be checked in Sources 1-3 and 5), O (needs an outside source) or F (framing or opinion). Then work the two examples as a class.

    [Transcript of the segment "Racing a Beam of Light," episode 2 of an online science series, 4 minutes 10 seconds long. The series, its narrator and its graphics are invented for teaching. What appears on screen is described in brackets.]

    [On screen: a mirror spinning in slow motion.] NARRATOR: In the summer of 1879, a 26-year-old Navy instructor named Albert Michelson set out to time the fastest thing in the universe. His trick was a small mirror spinning about 257 times every second.

    [On screen: an animated map of the Naval Academy sea wall, with a line labeled "Light's round trip: 3,972 feet."] NARRATOR: A beam of light bounced off the spinning mirror, raced to a fixed mirror far down the sea wall and came back. The round trip took about four millionths of a second. In that time the spinning mirror turned only about a thousandth of a turn, so the returning beam came back a little off course, shifted by about 11 to 13 centimeters. Measure that shift, and you can work out the speed of light.

    [On screen: a stack of handwritten pages.] NARRATOR: Michelson repeated the measurement a hundred times, and he never threw away a single result.

    [On screen: a bar chart titled "Michelson Nailed It." Two bars are labeled "Michelson, 1879: 299,944 km/s" and "Today: 299,792 km/s." The vertical axis runs from 299,700 to 300,000.] NARRATOR: His answer, 186,380 miles per second, matches today's value almost exactly, and it was well inside his own margin of error. Other scientists soon agreed: the French physicist Alfred Cornu had found 300,400 kilometers per second with a spinning toothed wheel.

    [On screen: the words "c = 299,792.458 km/s. Exactly."] NARRATOR: Today the speed of light is fixed by definition at exactly 299,792.458 kilometers per second, so there is nothing left to measure.

    Written for this page (the video series, its narrator and its graphics are invented), Racing a Beam of Light: Transcript of an Online Science Video (Source 4). Original passage written for this page.
    • Checking a video's numbers against the primary source (Source 4, paragraph 3)

      The video says the round trip was 3,972 feet and "took about four millionths of a second," and that the mirror "turned only about a thousandth of a turn." Do Michelson's figures support all three?

      Result: Source 1, paragraph 4, gives a distance of "about 2,000 feet," so a round trip of about 4,000 feet fits the video's 3,972. In meters, 3,972 × 0.3048 ≈ 1,211 m, and at about 299,900 km/s the trip takes 1,211 ÷ 299,900,000 ≈ 0.00000404 s, about 4.0 millionths of a second. Source 3, paragraph 7, puts the usual speed at 256 turns per second, and 256 × 0.00000404 ≈ 0.0010 of a turn. All three claims check out, and they agree with each other.

    • Sorting statements by how they can be checked (Source 4, paragraph 2)

      Evaluate three statements: Michelson was "a 26-year-old Navy instructor," the mirror spun "about 257 times every second," and he set out "to time the fastest thing in the universe."

      Result: The age needs an outside source: none of these texts gives it. A biography gives his birth in December 1852, so he was 26 in the summer of 1879 and the claim is right, but a student must name that source. The spin rate can be checked: Source 3, paragraph 7, says the speed "was lowered from 256 turns," so 257 is a slightly different rounding of the same figure. "The fastest thing in the universe" is framing: true as physics, but it is not evidence about the experiment. A video mixes these kinds of statement, so each needs its own test.

    Debrief: Which of the video's statements could you not check yet? Students usually list the claims about "a hundred times," the bar chart, the margin of error and Cornu. Those need Michelson's own final section, which students read next.

  4. Independent Practice20 minutes

    Students read Source 3, from the end of Michelson's paper, on their own and answer quiz questions 1-20, using all the sources on this page. Before they read, explain three terms: "in vacuo" means in a vacuum; Michelson's "±51 kilometers" is his limit on the error, in the most unfavorable case; and Alfred Cornu was a French physicist who had timed light with a rapidly turning toothed wheel a few years earlier. Friedrich Helmert, a German geodesist, later recalculated Cornu's result.

    Summing up the various errors, we find, then, that the total constant error, in the most unfavorable case, where the errors are all in the same direction, would be .00015. Adding to this the probable error of the result, .00002, we have for the limiting value of the error of the final result ±.00017. This corresponds to an error of ±51 kilometers.

    The correction for the velocity of light in vacuo is found by multiplying the speed in air by the index of refraction of air, at the temperature of the experiments. The error due to neglecting the barometric height is exceedingly small. This correction, in kilometers, is +80.

    Final Result.

    The mean value of V from the tables is 299852
    Correction for temperature +12
    ------------
    Velocity of light in air 299864
    Correction for vacuo 80
    ------------
    Velocity of light in vacuo 299944±51

    The final value of the velocity of light from these experiments is then--299940 kilometers per second, or 186380 miles per second.

    [...]

    Change of Speed of Rotation.

    In the last four sets of observations the speed was lowered from 256 turns to 192, 128, 96, and 64 turns per second. The results with these speeds were the same as with the greater speed within the limits of errors of experiment.

    Bias.

    Finally, to test the question if there were any bias in taking these observations, eight sets of observations were taken, in which the readings were made by another, the results being written down without divulging them. Five of these sets are given in the "specimen," pages 133-134.

    It remains to notice the remarkable coincidence of the result of these experiments with that obtained by Cornu by the method of the "toothed wheel."

    Cornu's result was 300400 kilometers, or as interpreted by Helmert 299990 kilometers. That of these experiments is 299940 kilometers.

    Albert A. Michelson, Experimental Determination of the Velocity of Light, from the Discussion of Errors, Final Result and Objections Considered (Source 3; excerpt, cuts marked [...]) (1880). Public domain (published 1880). Source text.
  5. Closure5 minutes

    Exit ticket: "Answer today's question in three sentences. Use at least one number from Michelson's data, one from Source 5 and one judgment about the video, and name the source of each." Sort the tickets into "integrated," "listed source by source" and "one source only."

    Teacher note on the historical texts. Michelson's paper is printed as published in 1880; its "±51 kilometers" is a limit he computed from the known sources of error, not a statistical range in the modern sense. Two figures in his table of groups (Source 2, part B) do not match his table of all 100 readings: the least value there is 299,650, but the full table includes 299,620 (June 18), and the seven sets at about 192 turns per second average about 299,909 in the full table, not 299,990. Both are printed here as in the source; quiz question 7 uses the first. Michelson went on to make better measurements of the speed of light over the next fifty years, and in 1907 he received the Nobel Prize in Physics for his optical instruments and the measurements made with them. The texts have no dated or offensive language.

    Homework sources. The homework uses a passage from Robert S. Ball's astronomy book The Story of the Heavens (Source 6) and a modern fact card written for this page (Source 7). Ball writes "Roemer" for the Danish astronomer Ole Rømer; Rømer's result is usually dated 1676, the year he announced it, not Ball's 1675.

    [...] It was noticed that when the earth was near to Jupiter the eclipse generally occurred before the predicted time; while when the earth happened to be at the side of its orbit away from Jupiter, the eclipse occurred after the predicted time. Once this was proved, the great discovery was quickly made by Roemer, a Danish astronomer, in 1675. [...] We learned from it that light had a measurable velocity, which, according to recent researches, amounts to 186,300 miles per second.

    [...]

    It thus appears that we can tell the velocity of light either by the observations of Jupiter's satellites or by experimental enquiry. If we take the latter method, then we are entitled to deduce remarkable astronomical consequences. We can, in fact, employ this method for solving that great problem so often referred to--the distance from the earth to the sun--though it cannot compete in accuracy with some of the other methods.

    The dimensions of the solar system are so considerable that a sunbeam requires an appreciable interval of time to span the abyss which separates the earth from the sun. Eight minutes is approximately the duration of the journey, so that at any moment we see the sun as it appeared eight minutes earlier to an observer in its immediate neighbourhood. In fact, if the sun were to be suddenly blotted out it would still be seen shining brilliantly for eight minutes after it had really disappeared. We can determine this period from the eclipses of Jupiter's satellites.

    So long as the satellite is shining it radiates a stream of light across the vast space between Jupiter and the earth. When the eclipse has commenced, the little orb is no longer luminous, but there is, nevertheless, a long stream of light on its way, and until all this has poured into our telescopes we still see the satellite shining as before. If we could calculate the moment when the eclipse really took place, and if we could observe the moment at which the eclipse is seen, the difference between the two gives the time which the light occupies on the journey. This can be found with some accuracy; and, as we already know the velocity of light, we can ascertain the distance of Jupiter from the earth; and hence deduce the scale of the solar system. It must, however, be remarked that at both extremities of the process there are characteristic sources of uncertainty. The occurrence of the eclipse is not an instantaneous phenomenon. The satellite is large enough to require an appreciable time in crossing the boundary which defines the shadow, so that the observation of an eclipse cannot be sufficiently precise to form the basis of an important and accurate measurement. [...]

    Robert S. Ball, The Story of the Heavens, chapter on the planet Jupiter: the velocity of light and the distance of the sun (Source 6; excerpt, cuts marked [...]) (1886; this edition 1900). Public domain (published 1900). Source text.

    The average distance. The average distance from Earth to the Sun is called the astronomical unit (au). Since 2012, astronomers have fixed it at exactly 149,597,870.7 km, about 92.96 million miles. Light crosses it in about 499.0 seconds, or 8 minutes 19 seconds.

    Not a perfect circle. Earth's orbit is slightly oval. Early each January, Earth is closest to the Sun, about 147.1 million km away; early each July it is farthest, about 152.1 million km away. The seasons come from the tilt of Earth's axis, not from this change in distance.

    How we know. Modern distances in the solar system come from timing signals. Radar pulses bounced off the planets since the early 1960s, and radio signals sent to spacecraft, travel at the speed of light, so a distance is half the round-trip time of a signal multiplied by the speed of light. Before radar, astronomers found the distance of the Sun from careful angle measurements of Venus and Mars, and from the speed of light combined with its travel time.

    Written for this page (the values are real, rounded), Planetarium Fact Card: How Far Away Is the Sun? (Source 7). Original passage written for this page.

Differentiation Strategies

For Struggling Students

  • Give a source organizer with one row per source and three columns: what it says, in what format, and what it can settle
  • Provide the three conversions students need (miles to kilometers, feet to meters, the 92 km/s of corrections) on a card
  • For the quiz, allow students to work with a partner on the Source 4 items before answering alone

For Advanced Students

  • Recompute the mean of the seven sets at about 192 turns per second from Michelson's full table and explain the disagreement with his grouped table
  • Read Michelson's section on the speed of rotation and suggest which error source might explain a systematic error of about 150 km/s
  • Find a modern news video about a scientific measurement and evaluate its graphics and claims against the published paper

Assessment Guidance

What to Look For

Strong answers make one claim that no single source makes on its own, support it with numbers from several sources put on the same scale, and cite each source. Strong evaluations say what each source is good for and where it fails, with evidence, and they check a secondary source against the primary one. Watch for students who summarize the sources one at a time, who compare numbers under different conditions (in air against in a vacuum, raw against corrected), who trust the video because it is recent and confident, and who treat a stated error limit as proof of accuracy.

02

Classroom Activities

3 Activities

1

Which Bulb Should the School Buy?

15 minGroups of 3

The school must replace 200 hallway bulbs and wants the cheaper choice over the next five years. Each group gets four source cards in different formats (written for this page; the products and data are invented) and writes a one-paragraph recommendation that uses all four.

The 4 Source Cards

  1. Spec table from the supplier: Bulb X, 9 W, 800 lumens, rated life 25,000 hours, $4.50 each. Bulb Y, 10 W, 800 lumens, rated life 15,000 hours, $2.50 each.
  2. Independent lab chart, described: after 10,000 hours of use, Bulb X gave 92 percent of its light when new and Bulb Y gave 71 percent.
  3. Transcript of a product review video: "Bulb Y is every bit as bright as X, and at almost half the price it's a no-brainer."
  4. Facilities note: the hallway lights are on 12 hours a day for 180 school days a year, and electricity costs $0.15 per kilowatt-hour.

Teacher Key

  • Hours in five years: 12 × 180 × 5 = 10,800, less than either rated life, so each socket needs one bulb.
  • Bulb X: 9 W × 10,800 h = 97.2 kWh, costing $14.58, plus $4.50 = $19.08 per socket. Bulb Y: 108 kWh, costing $16.20, plus $2.50 = $18.70 per socket.
  • Y is cheaper by $0.38 per socket, $76 for 200 sockets, but by card 2 it gives only 71 percent of its light after 10,000 hours, near the end of the five years. The video's "every bit as bright" is true only when the bulbs are new.
  • A strong recommendation names the trade-off: Y saves a little money; X keeps the hallways brighter.

Discussion Questions

  • Which card could the school check for itself, and how?
  • Card 3 gives no numbers. What, if anything, does it add?
  • How would the answer change if the lights ran 24 hours a day?
2

Can the Class Wade at Site B?

15 minPairs

A biology class plans to wade in a creek on Friday, three days after a storm. Pairs integrate four sources (written for this page; the county, creek and data are invented) and decide whether Site B is open, then rate each source's credibility from 1 to 3.

The 4 Sources

  1. County lab table, E. coli per 100 mL of water. Site A: 180 on Monday, 90 on Wednesday. Site B: 1,400 on Monday, 520 on Wednesday. The county closes a site to wading while its latest sample is above 235.
  2. Rain gauge chart, described: 48 mm of rain fell on Sunday and none since; the forecast for Thursday is dry.
  3. Local news video transcript, Wednesday evening: "The creek is back to normal and the water looks clear again."
  4. County web page, updated Thursday morning: "Site A open. Site B closed pending Thursday sample."

Teacher Key

  • Site B's latest result, 520, is more than twice the limit of 235, and the county page still lists it as closed. Plan for Site A (90, open).
  • Site B is falling: 520 is 37 percent of Monday's 1,400. Dry weather makes a lower Thursday result likely, but only the Thursday sample can reopen it.
  • The video is the weakest source: clear water can still carry bacteria, and "back to normal" gives no measurement.
  • Credibility: the lab table and county page 3, the rain chart 2 (it explains the trend but measures no bacteria), the video 1.

Discussion Questions

  • Which source is most up to date, and does that make it the most reliable?
  • What would you need to know to trust the video's claim?
  • Write the sentence you would send to parents, citing two sources.

Variation: Missing Source

Remove card 4. Pairs decide with the other three sources alone, then compare their decision with the county page.

3

Will the Backup Battery Last the Night?

15 minGroups of 4

The school's server room runs on a backup battery during a planned power cut from 11 p.m. to 7 a.m. Groups combine a spec sheet, meter data, an equation and a video claim to decide whether the battery is enough (written for this page; the equipment and data are invented).

The Sources

  • Spec sheet: usable battery energy 5.0 kWh; the inverter delivers 94 percent of the battery's energy to the equipment.
  • Power meter, last week, 11 p.m. to 7 a.m.: average load 620 W, highest single hour 700 W.
  • Equation from the installer's manual: run time in hours = (usable energy in kWh × inverter share) ÷ (load in kW).
  • Technician's phone video: "Five kilowatt-hours? That'll easily run the room all night."

Teacher Key

  • Energy delivered: 5.0 × 0.94 = 4.7 kWh. At the average load, 4.7 ÷ 0.62 ≈ 7.6 hours, about 7 hours 35 minutes; the cut lasts 8 hours.
  • At 700 W all night the battery would last 4.7 ÷ 0.70 ≈ 6.7 hours.
  • The technician's claim fails by about 25 minutes even at the average load. Options: shut down non-essential machines, add capacity, or shorten the cut.

Discussion Questions

  • Why is the average load not enough information on its own?
  • Which source would you question first if the battery ran out at 5 a.m.?
  • How much would the load have to fall for the battery to last exactly 8 hours?

03

Diagrams & Visual Aids

2 diagrams

Diagram 1 (Source 2, part A): Michelson's 100 Readings as a Histogram, Drawn to Scale

Michelson's 100 readings, June 5 to July 2, 1879 (in air, before corrections) 0 5 10 15 20 25 30 1 1 6 12 27 28 10 11 3 1 299,600 299,700 299,800 299,900 300,000 300,100 Speed of light in air, km/s, as recorded (bins 50 km/s wide) Number of readings Mean of the tables: 299,852 (Source 3) Today, on this scale: 299,792 - 92 ≈ 299,700 Red line: today's speed minus Michelson's own corrections of +12 and +80 km/s (Source 3).
Each bar counts the readings in one 50 km/s bin, from Michelson's table of all 100 observations (June 5 to July 2, 1879), as recorded: speeds in air before his corrections. The counts from left to right are 1, 1, 6, 12, 27, 28, 10, 11, 3 and 1. The dashed line is the mean he reports in Source 3. The red line is today's speed of light with his two corrections (+12 and +80 km/s, Source 3) taken off, so that it sits on the same scale as the readings.

Diagram 2: Five Estimates of the Speed of Light on One Axis, Drawn to Scale

Estimates of the speed of light in a vacuum, km/s, on one scale 299,600 299,800 300,000 300,200 300,400 300,600 Today: 299,792.458 (Source 5) Michelson, 1878 trials (Source 1) 300,140 Michelson, 1879 final (Source 3) 299,944 Cornu, toothed wheel (Source 3) 300,400 Cornu, per Helmert (Source 3) 299,990 Bars: the range each author states (± 300 mi/s, about ± 483 km/s, for 1878; ± 51 km/s for 1879). Cornu's figures appear in Source 3 without a stated range.
All values are in km/s and are meant as the speed in a vacuum; Source 1 does not say whether the 1878 mean was corrected from air to a vacuum, but its range is far wider than that 80 km/s correction. The 1878 mean is Michelson's 300,140 with his stated ± 300 miles per second, converted with Source 5. The 1879 value is his final 299,944 ± 51. Cornu's result and Helmert's reading of it come from Source 3, paragraph 11, which gives no range for them. The red line is the modern exact value (Source 5).

04

Homework Assignment

~30 min

RST.11-12.7 Homework: How Far Away Is the Sun?

Directions: Use Robert S. Ball's passage (Source 6) and the fact card (Source 7), printed at the end of the Closure phase of the lesson plan (paragraphs are numbered), together with Michelson's final value in Source 3 and the reference values in Source 5. Your task is to solve one problem, finding the distance from Earth to the Sun from the speed of light, and to evaluate the sources you use. Show your arithmetic for Problems 1, 2 and 4, and cite a source for every number.

Part 1: Solving with the Sources (Problems 1-2)

  1. Use only Ball's figures in Source 6: the speed of light in paragraph 1 and the travel time in paragraph 3. (a) Find the distance from Earth to the Sun in miles. (b) Compare your answer with the average distance in Source 7, as a percent. (c) Which of Ball's two figures causes most of the difference? Explain.
  2. Now use Michelson's final value in Source 3 and the travel time in Source 7, paragraph 1. (a) Find the distance in kilometers. (b) Compare it with the fixed value in Source 7, as a percent. (c) Explain why this answer is so much closer than the one in Problem 1, naming the source of each improvement.

Part 2: Evaluating the Sources (Problems 3-4)

  1. Ball says the light method "cannot compete in accuracy with some of the other methods" (Source 6, paragraph 2). Using Source 6, paragraph 4, explain the reason he gives. Then use Source 7, paragraph 3, to say whether his judgment still holds today, and why.
  2. Source 7, paragraph 2, gives Earth's nearest and farthest distances from the Sun. (a) Find the light travel time for each. (b) Explain whether Ball's "eight minutes" is accurate enough for his purpose in paragraph 3 and for fixing the scale of the solar system, and why the answers differ.

Part 3: Integrating Across the Lesson (Problems 5-6)

  1. Ball gives the speed of light as 186,300 miles per second "according to recent researches" (Source 6, paragraph 1), and Michelson gives 186,380 (Source 3). (a) Which is closer to the modern value in Source 5, and by how much is each off? (b) Describe where Ball's value would go if you added it to Diagram 2. (c) Does being closer make Ball's figure the better source? Explain.
  2. Write one paragraph that answers "How far away is the Sun, and how do we know?" for a reader of a school science magazine. Integrate at least three sources from this lesson, cite each one, and say which source you trust most for each number you use.

Rubric

CriterionFull Credit (2 pts)Partial Credit (1 pt)No Credit (0 pts)
Solving the ProblemDistances, percents and travel times are correct, with units and arithmetic shownOne arithmetic or unit errorAnswers are missing or unsupported
IntegrationNumbers from different sources are put on one scale and combined into one answerSources are used side by side but not combinedOnly one source is used
EvaluationEach judgment of a source names what it is good for, its limits and the evidenceJudgments are stated without evidenceNo evaluation, or a judgment the sources contradict
Citation and WritingEvery number and claim is cited by source and paragraph, and the paragraph reads as one argumentSome citations are missing, or the paragraph lists sources one by oneNo citations

05

Quiz: 20 Questions

Interactive, with answers

Instructions

All questions use the sources in the lesson plan: Source 1 in Direct Instruction, Source 2 (Diagram 1 and the table of groups), Source 5 (the reference table), Source 4 (the video transcript) in Guided Practice, and Source 3 in Independent Practice (paragraphs are numbered). For each question, decide which sources settle it before you answer, and cite sources and paragraphs in your short answers. Your score updates as you answer, and Reset quiz clears everything so you or your students can try again.

Multiple choice: pick an option to check it. Short answer: write your answer, then reveal the model answer.

0 of 20 answered · 0 correct

  1. Question 1 of 20 · Multiple Choice

    Which statement correctly fits Diagram 1 together with Source 3?

  2. Question 2 of 20 · Multiple Choice

    The video says Michelson "never threw away a single result" (Source 4, paragraph 4). Which evaluation is best supported by Michelson's own text?

  3. Question 3 of 20 · Multiple Choice

    The video's bar chart (Source 4, paragraph 5) starts its axis at 299,700. Which evaluation of the chart is accurate?

  4. Question 4 of 20 · Multiple Choice

    By what percent does Michelson's final 299,944 km/s (Source 3) differ from the modern value in Source 5?

  5. Question 5 of 20 · Multiple Choice

    The video says Michelson's answer "was well inside his own margin of error" (Source 4, paragraph 5). Which evaluation is correct?

  6. Question 6 of 20 · Multiple Choice

    Which group in Source 2, part B, together with which paragraph of Source 3, best tests whether Michelson's expectations could have influenced his readings?

  7. Question 7 of 20 · Multiple Choice

    Source 2, part B, lists the "Least value" as 299,650, but Diagram 1 shows one reading in the bin from 299,600 to 299,649. What is the best conclusion?

  8. Question 8 of 20 · Multiple Choice

    Michelson calls his agreement with Cornu a "remarkable coincidence" (Source 3, paragraph 10). Which evaluation fits paragraph 11?

  9. Question 9 of 20 · Multiple Choice

    Single 1878 trials in Source 1, paragraph 2, run from 184,500 to 188,820 miles per second. Using the greatest and least values in Source 2, part B, for the 1879 readings, by about what factor did the spread of single trials shrink?

  10. Question 10 of 20 · Multiple Choice

    The video says the returning beam "came back a little off course, shifted by about 11 to 13 centimeters" (Source 4, paragraph 3). How does this compare with Source 1?

  11. Question 11 of 20 · Multiple Choice

    The video ends: "Today the speed of light is fixed by definition ... so there is nothing left to measure" (Source 4, paragraph 6). Which evaluation is best?

  12. Question 12 of 20 · Multiple Choice

    A student needs the size of the correction from air to a vacuum. Which source should she use, and why?

  13. Question 13 of 20 · Multiple Choice

    Which set of sources is needed, and enough, to answer "Was Michelson's result correct within the error limit he stated?"

  14. Question 14 of 20 · Multiple Choice

    Source 3, paragraph 1, gives the limit of error as "±.00017" of the result. Which statement is correct?

  15. Question 15 of 20 · Short Answer

    Answer the lesson's question in one paragraph: How fast does light travel, and how far can we trust Michelson's 1880 answer? Integrate at least three sources, cite each, and include at least two numbers.

  16. Question 16 of 20 · Short Answer

    Evaluate the video (Source 4) as a source. Name two of its statements that are accurate and two that are misleading or false, other than those checked in Examples 3 and 4, and support each with a specific source. Then say what the video is and is not useful for.

  17. Question 17 of 20 · Short Answer

    Describe the shape and spread of Diagram 1 in words. Then explain what the spread of single readings, the "Average difference from mean" of 60 in Source 2, part B, and the error limit of ±51 in Source 3 each tell a reader, and why the mean can be far more precise than a single reading and still be wrong.

  18. Question 18 of 20 · Short Answer

    Redesign the video's bar chart (Source 4, paragraph 5) so that it shows the comparison honestly. Describe the chart type, the axis and what it marks, and explain how Diagram 2 does or does not already solve the problem.

  19. Question 19 of 20 · Short Answer

    Plan one new visual that integrates Diagram 1, Source 3 and Source 5 to answer the question "Was the error in Michelson's 1879 result random or systematic?" Describe what it shows and what a reader would conclude from it.

  20. Question 20 of 20 · Short Answer

    Michelson says his limit of ±51 km/s covers the case "where the errors are all in the same direction" (Source 3, paragraph 1). What does the comparison with Source 5 suggest about that limit, and what general lesson does it teach about evaluating even a careful primary source?

0 of 20 answered · 0 correct

06

Frequently Asked Questions

10 Questions

What does RST.11-12.7 mean?

RST.11-12.7 asks students in grades 11-12 to integrate and evaluate information from several sources in different formats and media, such as data tables, graphs, video and text, to answer a question or solve a problem. Integrating means combining the sources into one answer; evaluating means judging what each source is good for and where it falls short.

How is RST.11-12.7 different from RST.9-10.7?

RST.9-10.7 asks students to translate one piece of technical information between forms, for example from words into a chart or from an equation into words. RST.11-12.7 asks them to combine several sources that may disagree, judge their reliability and use them together to address a question. Translation is a tool; integration and evaluation are the goal.

What counts as "diverse formats and media" in RST.11-12.7?

The standard names quantitative data, video and multimedia. In practice that includes data tables, graphs, diagrams, equations, printed reports, video or its transcript, animations and websites. The point is that the sources present information in different ways, so students must put them on a common footing before they can combine them.

Can RST.11-12.7 be taught without showing a video?

Yes. A transcript with descriptions of what appears on screen lets students evaluate a video's narration and its graphics, as this lesson does with Source 4. Where classroom time and technology allow, a real short video on the same topic works as well; the skills of checking claims and judging design are the same.

What does "evaluate" add to "integrate"?

Integrating combines what the sources say; evaluating decides how much weight each deserves. A student who averages Michelson's value with the video's claims has integrated without evaluating. A student who notices that the video's margin-of-error claim is contradicted by the primary source has done both.

How should students decide which source to trust when sources disagree?

Ask which source is closest to the evidence, which gives its methods and numbers, which has been checked independently, and what each source is designed to do. A primary report is usually best for methods, a modern reference for accepted values, and a video for a quick picture of how something works. Trust can differ by claim within one source.

Why use Michelson's 1879 speed of light experiment for this standard?

His paper gives text, a table of all 100 readings, grouped results and his own corrections, so students can integrate formats that come from one careful source. The modern exact value lets them evaluate it. The result is close to the truth but outside his stated limit, so students must weigh precision against accuracy.

How does RST.11-12.7 relate to SL.11-12.2 and RI.11-12.7?

All three ask students to integrate sources in different formats. SL.11-12.2 applies it to making decisions and solving problems from information presented orally and visually, and RI.11-12.7 to informational texts in general. RST.11-12.7 applies it to science and technical sources, where quantitative data and consistent units matter most.

What mistakes do students often make when integrating sources?

Three are frequent. They summarize each source in turn instead of combining them into one claim; they compare numbers measured under different conditions (in air and in a vacuum, before and after corrections); and they trust a polished video over a primary source because it is recent or confident. Asking "what does each source contribute to the question?" helps with all three.

How is RST.11-12.7 usually assessed?

Usually with a task that supplies several sources, such as a passage, a data table and a graph, and asks for a short written answer to a question that uses and cites them all. Stronger tasks include a source with a flaw to catch. This page's quiz and homework follow that pattern and lead into research writing under WHST.11-12.8.