Xi Scorpius 

Penny Fisher
Star: Xi Scorpius  
Date & Time: 6/30/98, 21:30 ET  
Seeing: 6 <1-10 Seeing Scale (10 best)>  
Location of site:  Englishtown NJ, 40.25  N  74.333 W  
Site classification: Suburban  
Sky darkness: -- <Limiting magnitude>  
Telescope: 8 inch Dob  
Magnification: 47X , 94X  
  
 
Spotted this by star hopping from Graffias. This was a very pretty close double which was split with 47X.  It appeared of equal magnitude and similar color, a light pale yellow. With the higher magification, component 2 appeared about a half of a magnitude dimmer, and also it had a rather orange tinge to it. 
 
 
 
Luis Argüelles
Star: Xi Scorpius  
Date & Time: July,15,1998 - 21:30 UT   
Seeing: 6.5  <1-10 Seeing Scale (10 best)>  
Location of site: Santander - Spain   
Site classification:   
Sky darkness: 4.5 - (2.5 near horizont)  <Limiting magnitude>  
Telescope: Vixen 102 mm f/9.8 Achromatic refractor   
Magnification: 25x, 50x, 100x, 200x 
 
Using the setting circles, I navigate from Antares towards this very nice pair of double stars. The first observation is made at 25x and interestingly I observe them as something more than pinpoint stars. Anyway, I don't seem confident at all to say that I observe an elongation at 25x. 

Nevertheless, at 50x, both Xi Scorpius and Struve 1999 are an easy split with my 4" refractor. Xi Scorpius is located North from Struve 1999 and is a brighter pair, but the pair from Struve 1999 is easier to split than Xi Sco. At this magnification I can not observe difference in coloration in Struve 1999 and both components show more or less the same magnitude. 

On the other hand, I easily observe a nice difference in magnitude from both components of Xi Sco. What is very interesting is to note that these two double stars offer almost the same beauty as the typical "doble-doble", Epsilon Lyra. 

Using 100x, I observe a clear difference in magnitude in Struve 1999: The western component is a bit brighter than the another one. Also, I can't observe difference in coloration between them, and both components are rendered as white with a very slight yellowish tint. Maybe the low altitude of the star over the horizon makes it a little yellow. 

Again at 100x, the main component of Chi Sco appears white-light yellow, while the secondary does have a very soft blueish coloration. 

After removing the star diagonal, the main star of Chi Sco appears as orangeish. The secondary is white or white-blue (??). I also confirm the white coloration of both components of Struve 1999. 
 

 
 
Pino Bandini
Star: Xi Scorpius  
Location of site: Ravenna, Italy 
Date of observations (UT): 19 June 2000 – 21.39 UTC 
Site classification: Urban 
Sky conditions
Seeing: 7 (10 best) 
Temperature: 20C 
Limiting visual magnitude: -- 
Telescope: Celestron C8 
Magnification: 81x (eyepiece 25 mm Plossl) + diagonal 
 
 
 
 
 
 
Mary Flanagan
Star: Xi Scorpius 
Date & Time: 06 Jul 2000 04:46 UT; 05 Jul 11:46 PM CDT 
Seeing: 6 <1-10 Seeing Scale (10 best)>  
Transparency: 6 <1 - 10> 
Location of site: Apple Valley MN, USA 
93d 14m 25s W; 44d 45m 17s N 
Site classification: Suburban 
Sky darkness: 4 <limiting magnitude> 
Telescope: 8" f/6 Dobsonian  
Magnification: 80x
This one and STF 1999 are a pretty pair of doubles in the same field, both cleanly split @ 80x, (except for the Xi B component.) The Xi primary appeared pale blue; C looked pale orange-yellow. I must say this was a surprise, as my NSOG shows the exact opposite, and I can only guess that the atmospheric haze was playing havoc with my color perception. Magnitude difference obvious. 
 
 

 

 
 
William L. Schart
Star: Xi Scorpius 
Date & Time: 7/17/00 11:51 pm CDT 
Seeing: 6 <1-10 Seeing Scale (10 best)> 
Location of site: Killeen, TX (Lat 31 N, Elev 600 ft) 
Site classification: Suburban 
Sky darkness: 3.35 <Limiting magnitude> 
Telescope: Orion 6" Dob. 
Magnification: 32x, 48x, 72x, 120x, 98x 144x, 240x
Took a while to find this. Eventually I just resorted to looking at every star in the general area that was bright enough to be visible in my finder. Not split at 32x, barely at 48x. Primary was a bright yellow, the secondary possibly a faint blue. Separation 8”, PA 50 (published 7.8, 47). 
 
 
 
 
Eddy O'Connor
Star: Xi Scorpius
Date & Time: July 18th 2000, 6.45 -7.30 p.m local; UT +10
Seeing: 7 dropping to 3 <1-10 Seeing Scale (10 best)> 
Transparency: 9/10
Temperature: 7oC. Dew
Location of Site: Terara, New South Wales, Australia, Long.150.38 degrees; 
South 34.52. 
Site Classification: Suburban 
Sky darkness:  <Limiting magnitude> 
Instrument: 8" F9 Dobsonian
Magnification: --
 
I expected this star to be easier to find since it 
boasts a Greek letter. I was wrong. This is located in a fairly
vacant area of sky with few bright pit stops. However, I eventually 
tracked down this light yellow star and noticed its wide mag. 7 
companion but failed to unglue its bosum companion. 
 
 
 
Richard Harshaw
Star: Xi Scorpius 
Location of site: Northern Kansas City, 
Missouri (USA). 
94d 30m west longitude, 39d 15m north latitude 980 ft above Mean Sea Level 
Date of observations (UT): July 22, 2000; 0230 hours 
Site classification: suburban 
Sky conditions
seeing--  8 out of 10 
transparency--  8 out of 10 
limiting visual magnitude--  4.5 mag 
Telescope: Celestron C-8 
Eyepiece: 7.4mm, 280x 
 
 
Colors noted: yW, dO, bW, and W. 
This system is more complex than what was listed on our Results page. The fourth star (actually "E" in the WDS) was not shown on the Results page list. To confirm the 0.8" pair, I had to go to 697x with my Barlow. 

It was discovered in 1782 by William Herschel. 
The AB orbit takes 45.69 years (Baize, 1942). The primary is 1.45 times the sun's mass and the companion 1.34 times. They are at least 18 AU apart (the size of the orbit of Uranus). 

Star A is also a spectroscopic binary. 
The AC orbit probably takes over 1,000 years. 
STF 1999 is 40' S and is actually a part of this system, being at least 7,000 AU from Xi. 

First measures: AB = 1.1" @ 356.. AC = 6.7" @ 79 (1825). In 1903, Jouffray got 7.3" @ 63 for AC. 
 
Sep/PA's: 0.8"/51, 8"/50, 281"/169 
Year of measurement: 1991 
Distance (light years): 91 
Luminosity (in suns): 22.7 

 

 
 
John M. Ryan
Star: Xi Scorpius 
Date of Observation: 3/08/00 21UT  
Location of Observation: Barraras, Salamanca, Spain 
40º N, 6º W, Elev. 800 Meters. 
Seeing: 6 to 7 (1 - 10, 10 best) 
Transparency: 8 
Limiting Mag. (naked eye): 4.5  
Site classification: Rural  
Instrument: Televue 101 Apo Refractor  
Magnification: 90X (6mm Radian) 
 
Separation (Clear or Touching):Clear 
Magnitude Comment: Bright primary and dim secondary in accordance with the data. 
 
Color comment: Pale yellowish white primary and white secondary. 
General Comment: Nice easy split with Struve 1999 in the same field of view.