Abstract
Abstract
The purpose of this paper is to show how we can obtain
spectra for different astronomical objects using low coat
equipment. Where a high-efficiency diffraction grating named “The
Star Analyzer” was used by the International Astronomical Center
(IAC) in Abu Dhabi, UAE to get the spectrum of different
astronomical objects. Balmer series was readily visible when
observing an “A” type star. TiO absorptions lines were
distinguished by observing an “M” type star. Methane absorption
lines were visible by observing Uranus and Neptune. Whereas HI and
HeI emission lines were detected by observing a blue hypergiant. In
addition, C2 Swan band absorption lines were identified by observing
a red giant carbon star. This type of observation is very
interesting for public outreach as well as university students,
because it shows astrophysical principles for public and students
practically and by using low cost equipment.
Subject
Mathematical Physics,Instrumentation