Dr. Nic Scott
Telescope Systems Scientist
The CHARA Array/NASA BAERI
GSU
-IScAI
-LESIA/Obs Paris
photography/film
UNCC
-physics
-psych
-astro
Applied Physics
-biomedical optics
-medical physics
-astro
NASA/BAERI
-exoplanets
-speckle
CHARA
-long baseline optical interferometry
Spotted magnetic stars
Interacting binaries
Expansion curve of Nova Del 2013.
Regulus -- Che et al. 2011, ApJ, 732, 68
Rasalhague -- Zhao et al. 2009, ApJ, 701, 209
Altair -- Monnier et al. 2007, Science, 317, 324
Alderamin -- Zhao et al. 2009, ApJ, 701, 209
Beta Cas -- Che et al. 2011, ApJ, 732, 68
All we can to measure is light from a distant star... so how can we find a planet that we can't see?
Unlike most illustrations of this kind, in this graphic, the Earth and the Moon are to scale. The Sun is off-screen to the left, about 400 times farther than the Earth-Moon distance and roughly twice as big as the Moon's orbit.
The only safe way to look directly at the uneclipsed or partially eclipsed sun is through special-purpose solar filters, such as “eclipse glasses” or hand-held solar viewers*. Homemade filters or ordinary sunglasses are not safe for looking at the sun
*verified to be compliant with the ISO 12312-2 international safety standard
The Sun's Corona
Bailey's Beads
"Diamond Ring"
Solar Prominence
ruby-red light of hydrogen gas heated to more than 20,000° Celsius (36,000° Fahrenheit)
Ippolito Caffi and the 1842 Solar Eclipse in Venice
Butler, 1918
Approach of the Moon's Shadow
Georg von Peurbach, Theoricæ nouæ planetarum, 1423-1461
Astronomy Explained, James Ferguson, 1757.
Etienne Trouvelot, Lithograph in colour, Total eclipse of sun; observed 29 July 1878
Roy Lichtenstein, Eclipse of the Sun I (left), II (right), Oil and Magna on Canvas, 1975
Zakariyya ibn Muhammad al-Qazwini, pages from “Aja’ib Al Makhluqat wa Ghara’eb Al Mawjodat” (The Wonders of Creation), 1203-1283
Image from On the Moon written by Konstantin Tsilkovsky in 1887
Phobos eclipse on Mars from Perserverence, 2019
A graph of April cloud amounts along the centre line derived from the same dataset as Figure 3. Stations are plotted according to their longitude, even though they often do not lie on the centreline. Source: NASA.
This graph shows the average October cloud cover (2000-2018) from satellite measurements at 10:30 am local time along the centerline of the October 14, 2023, annular eclipse track. Units are fractional sky cover, which can be interpreted as percent cloud cover. Courtesy Jay Anderson, Eclipsophile.com.
There's about 5077 stars visible by naked eye. Which works out to 404 stars per sterradian.
So if you hold an iphone out at arm's distance, there’re about 50 visible stars in that amount of sky
There’s estimated to be 200 billion galaxies. Which works out to about 15.9 billion per sterradian.
An iphone 12 screen pixel is ~0.3mm.
There’re about 1,400 galaxies in the area of that single pixel.
An estimate of the number of stars per galaxy is 100 billion.
So that puts around
140,000,000,000,000 stars in the area of that single pixel
Oxygen
Super-Earth or mini-Neptune?
(1548 – 1600)
Italian Friar
Oct 1995
Most stars aren' t single
~50% of the stars you see are binaries
~25% are triples
-on avg there's an exoplanet per star
~10% of Sun-like stars likely host rocky exoplanets, more for lower-mass stars
Telescope Systems Scientist (CHARA)
Instrumentalist (NASA)
Instrumentation development and maintenance program
-telescopes, adaptive optics systems, enclosures, and the beam relay systems.
-laboratory electro-optical systems
-design and development of new instruments
"dedicated generalist"