What a star's light shows: spectra and color
Grade 9 Science Worksheet - Challenge Me

Circle the best answer.
Hydrogen, 656.3, 486.1, 434.0, 410.2; helium, 587.6; sodium, 589.0, 589.6; calcium, 393.4, 396.8. A star shows dark lines at 656.3, 486.1, 434.0, 589.0 and 589.6 nm, and its light peaks near 480 nm. What can Esme conclude?
- Hydrogen and sodium; surface about 1,400 K
- Hydrogen and helium; surface about 6,000 K
- No hydrogen or sodium; surface about 6,000 K
- Hydrogen and sodium; surface about 6,000 K
A gas cloud's spectrum shows bright lines at 656.3 and 486.1 nm on a dark background. What is the cloud, by Jun's reading?
- Cool hydrogen gas sitting in front of a bright star
- A hot, dense solid
- Hot, thin hydrogen glowing on its own
- Gas that contains no hydrogen
Hydrogen, 656.3, 486.1, 434.0, 410.2; helium, 587.6; sodium, 589.0, 589.6; calcium, 393.4, 396.8. A star shows a dark line at 587.6 nm but none at 589.0 or 589.6 nm. Which element is it, by Kira's reading?
- Neither, since dark lines mean missing
- Sodium, since 587.6 is close to 589
- Both sodium and helium
- Helium, not sodium
Luz's friend says dark lines mean a star is missing those elements. Which response is best?
Drawing of light passing through gas, with dark lines in the spectrum. Drawing of light passing through gas, with dark lines in the spectrum. light gas spectrum dark lines - Agree: the elements are hidden in the core
- Disagree: elements in the outer gas absorb those wavelengths
- Disagree: dark lines are bright lines seen from far away
- Agree: dark means nothing is there
Milo's cousin says red stars are hottest, like a red-hot stove coil. Which response is best?
Row of glowing objects from red to white to blue, with temperatures rising. Row of glowing objects from red to white to blue, with temperatures rising. glowing objects red white blue temperatures rising - Agree: red is the hottest color
- Disagree: color tells nothing about temperature
- Disagree: red stars are coolest; hotter ones glow white, then blue
- Agree: red light peaks at the shortest wavelength
Peak = 2,898,000 nm·K ÷ temperature; stars at 4,000, 6,000 and 20,000 K. Which of these stars peaks in the ultraviolet: 4,000 K, 6,000 K or 20,000 K, by Ren's math?
- The 6,000 K star, like the Sun
- The 20,000 K star, peaking near 145 nm
- No star; their peaks stay in visible light
- The 4,000 K star
The Sun peaks near 502 nm. Another star peaks at 251 nm. How does its temperature compare, by Tala's math?
Two light curves: Sun peaking at 502 nm, star at 251 nm. Two light curves: Sun peaking at 502 nm, star at 251 nm. Sun star 502 nm 251 nm - About half the Sun's
- About twice the Sun's, near 11,500 K
- The same as the Sun's
- About 4 times the Sun's
Star P is blue with strong helium lines. Star Q is yellow with strong sodium and calcium lines. What can Zee say?
Two spectrum strips: P, blue, helium lines; Q, yellow, sodium and calcium lines. Two spectrum strips: P, blue, helium lines; Q, yellow, sodium and calcium lines. P Q blue yellow helium lines sodium calcium - Q is hotter, since it shows more lines
- P is hotter; each spectrum reveals elements in its outer gas
- P lacks sodium, since its strip shows no sodium lines
- Both are the same temperature
The Sun's dark calcium lines at 393.4 and 396.8 nm are very strong. What does this show, by Ari's reading?
Spectrum strip of the Sun with strong dark lines at 393.4 and 396.8 nm. Spectrum strip of the Sun with strong dark lines at 393.4 and 396.8 nm. Spectrum strip of the Sun with strong dark lines 393.4 nm 396.8 nm - The Sun has no calcium
- Calcium in the Sun's outer gas glows brightly at those wavelengths
- Calcium in the Sun's outer gas absorbs those wavelengths
- Those lines belong to hydrogen
The same dark-line pattern appears in a lab gas and in a distant star. What is the strongest conclusion, by Bo's reading?
Two spectrum strips with matching dark lines: lab gas and distant star. Two spectrum strips with matching dark lines: lab gas and distant star. lab gas distant star - The star lacks that element
- The star's gas glows with bright lines
- The star's outer gas contains that element
- The star is the same temperature as the lab