PERIOD DETERMINATION FOR NEA (162421) 2000 ET70

Eduardo Manuel Alvarez; Julian Oey; Xianming Han; Orry R. Heffner; Adam W. Kidd; Bradley J. Magnetta; Frederick W. Rastede

PERIOD DETERMINATION FOR NEA (162421) 2000 ET70

Eduardo Manuel Alvarez, Julian Oey, Xianming Han, Orry R. Heffner, Adam W. Kidd, Bradley J. Magnetta, Frederick W. Rastede

Research output: Contribution to journal › Article › peer-review

Abstract

Lightcurve analysis for (162421) 2000 ET70 was performed in collaboration with observers in Uruguay, Australia, and the United States from observations obtained during the asteroid’s favorable opposition in 2012. The synodic rotation period was found to be 8.947 ± 0.001 h and the lightcurve amplitude was 0.60 ± 0.07 mag.

Original language	American English
Journal	Scholarship and Professional Work - LAS
Volume	39
Issue number	3
State	Published - Jan 1 2012

Keywords

asteroids
minor planet

Disciplines

Astrophysics and Astronomy

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PERIOD DETERMINATION FOR NEA (162421) 2000 ET70Final published version, 643 KBLicense: Unspecified

Cite this

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title = "PERIOD DETERMINATION FOR NEA (162421) 2000 ET70",

abstract = " Lightcurve analysis for (162421) 2000 ET70 was performed in collaboration with observers in Uruguay, Australia, and the United States from observations obtained during the asteroid{\textquoteright}s favorable opposition in 2012. The synodic rotation period was found to be 8.947 ± 0.001 h and the lightcurve amplitude was 0.60 ± 0.07 mag.",

keywords = "asteroids, minor planet",

author = "Alvarez, \{Eduardo Manuel\} and Julian Oey and Xianming Han and Heffner, \{Orry R.\} and Kidd, \{Adam W.\} and Magnetta, \{Bradley J.\} and Rastede, \{Frederick W.\}",

year = "2012",

month = jan,

day = "1",

language = "American English",

volume = "39",

journal = "Scholarship and Professional Work - LAS",

number = "3",

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TY - JOUR

T1 - PERIOD DETERMINATION FOR NEA (162421) 2000 ET70

AU - Alvarez, Eduardo Manuel

AU - Oey, Julian

AU - Han, Xianming

AU - Heffner, Orry R.

AU - Kidd, Adam W.

AU - Magnetta, Bradley J.

AU - Rastede, Frederick W.

PY - 2012/1/1

Y1 - 2012/1/1

N2 - Lightcurve analysis for (162421) 2000 ET70 was performed in collaboration with observers in Uruguay, Australia, and the United States from observations obtained during the asteroid’s favorable opposition in 2012. The synodic rotation period was found to be 8.947 ± 0.001 h and the lightcurve amplitude was 0.60 ± 0.07 mag.

AB - Lightcurve analysis for (162421) 2000 ET70 was performed in collaboration with observers in Uruguay, Australia, and the United States from observations obtained during the asteroid’s favorable opposition in 2012. The synodic rotation period was found to be 8.947 ± 0.001 h and the lightcurve amplitude was 0.60 ± 0.07 mag.

KW - asteroids

KW - minor planet

UR - https://digitalcommons.butler.edu/facsch_papers/746

M3 - Article

VL - 39

JO - Scholarship and Professional Work - LAS

JF - Scholarship and Professional Work - LAS

IS - 3

ER -

PERIOD DETERMINATION FOR NEA (162421) 2000 ET70

Abstract

Keywords

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