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YSM Issue 90.5

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FOCUS<br />

astronomy<br />

into many different wavelengths, or colors.<br />

Objects moving away from the Milky Way<br />

emit less intense light and subsequently undergo<br />

a shift in wavelength toward the red<br />

end of the color spectra where wavelengths<br />

are longer. Therefore, a galaxy with a larger<br />

redshift is moving further away. By gathering<br />

this information, the researchers were better<br />

able to understand the position of potential<br />

satellite galaxies, filling in the missing gap in<br />

knowledge about whether these galaxies are<br />

indeed satellites of a central galaxy.<br />

However, using this process to obtain redshifts<br />

comes with its own set of difficulties.<br />

For example, spectroscopy is expensive and<br />

time consuming. In addition, the slower<br />

that a galaxy moves, the fainter and harder<br />

it becomes to detect the redshifts. Though<br />

the research team was able to target over<br />

17,000 redshifts, the spectra obtained may<br />

be not only from galaxies themselves, but<br />

also from stars and other objects. Therefore,<br />

they needed to further filter out the<br />

redshifts corresponding to galaxies from<br />

those caused by other natural phenomena.<br />

To create a more efficient system for detecting<br />

redshifts of galaxies, the researchers<br />

observed the relative wavelengths of satellite<br />

galaxies and their redshift range. They<br />

found a range in which the redshifts were<br />

similar among satellites, indicating that<br />

redshifts in this range were the most likely<br />

to correspond to satellite galaxies. By going<br />

back over their collected sample of redshifts<br />

and selecting redshifts that fell within<br />

the “satellite galaxy” range, they were able<br />

to leave out redshift data from unwanted<br />

sources. Using this refined redshift information,<br />

researchers were able to locate 25<br />

satellites from analog galaxies, providing<br />

us a new perspective on the nature of many<br />

potential satellite galaxies in the universe.<br />

The SAGA continues<br />

IMAGE COURTESY OF NASA<br />

►The Milky Way Galaxy has long been studied,<br />

and houses numerous satellite galaxies.<br />

While the study has surprised the research<br />

team, there still remains much to<br />

uncover, and they are just getting started.<br />

The team is leading in this field—there<br />

is no other research team doing such an<br />

ambitious project. Once the SAGA is completed,<br />

scientists will better understand<br />

the Milky Way from a cosmological standpoint<br />

and how it compares to other analogs.<br />

“We’re really proud of the progress<br />

we made and we are well underway in answering<br />

the question of how atypical our<br />

galaxy may be,” Geha said.<br />

With a goal of analyzing 100 analog<br />

IMAGE COURTESY OF WIKIMEDIA COMMONS<br />

►Using optical telescopes, more than<br />

10,000 distant galaxies can be seen.<br />

galaxies similar to the Milky Way, the researchers<br />

are already analyzing the data<br />

of other analogs for their satellites. With<br />

more efficient methods for detecting redshifts,<br />

the team can more effectively locate<br />

even the faintest satellites. While Geha is<br />

not certain what the rest of their data will<br />

indicate once they finish analyzing all satellite<br />

galaxies, she believes it might take as<br />

few as two to four years to finish the survey<br />

and make more conclusions. “Once<br />

the SAGA Survey is complete, I think<br />

we will really understand our galaxy in a<br />

much broader context,” Geha said. Until<br />

then, the SAGA continues in uncovering<br />

the mystery of our galaxy.<br />

ABOUT THE AUTHOR<br />

JESSICA TRINH<br />

The Milky Way Galaxy—an outlier?<br />

The process of obtaining redshift information<br />

to determine satellite galaxies is<br />

a slow process, but it comes with a great<br />

payoff. The team’s analyses of these satellite<br />

galaxies have revealed an interesting finding:<br />

the analog galaxies contain mostly star<br />

forming satellite galaxies. Unlike the Milky<br />

Way, the results from the 8 analog galaxies<br />

indicated 26 of the 27 satellite galaxies are<br />

actively forming stars. “If more information<br />

supports this finding, we need to start<br />

reevaluating how we view our own satellite<br />

galaxies in the Milky Way,” Wechsler said.<br />

JESSICA TRINH is a sophomore Neuroscience major in Branford College.<br />

She is the Vice President of Synapse and is excited to teach middle schoolers<br />

about STEM. She also teaches health education in New Haven middle schools,<br />

nutrition counseling at HAVEN Free Clinic, and is currently leading a research<br />

project on nutrition.<br />

THE AUTHOR WOULD LIKE TO THANK Dr. Marla Geha and Dr. Risa<br />

Wechsler for their time and enthusiasm for sharing their research.<br />

FURTHER READING<br />

Geha, M., Wechsler, R.H., Mao, Y.Y., et al. 2017. “The SAGA Survey I: Satellite<br />

Galaxy Populations Around Eight Milky Way Analogs. The Astrophys. J. 847, 1-21.<br />

Geha, M., Wechsler, R.H., Bernstein, R., et al. 2017. The SAGA Survey.<br />

Retrieved from http://sagasurvey.org<br />

14 Yale Scientific Magazine December 2017 www.yalescientific.org

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