<  
Home   /  
Astronomy   /  
Sun   /  
Venus Transit 2004
>  

Venus Transit 2004/6/8

6:53 EDT, an airplane happened to join the transit. 1/270 second, F6, EXP+0.3, f8.2mm, ISO 200, white balance cloudy. All images on this page are taken with Baader Astrosolar filter, Celestron star hopper 8"/f6 Dob, Scopetronix 18mm eyepiece/adapter, Nikon coolpix 995 digital camera. From Green Tree, Pittsburgh, PA, USA.

 Double Transit.  This photo appeared on the front page of 2004/6/9's Pittsburgh Post Gazette.
Double Transit. This photo appeared on the front page of 2004/6/9's Pittsburgh Post Gazette.


A faint ring of light (aureole) can be seen surronding the dark part of Venus, evidence that Venus has an atmosphere. Some interesting observations:
1. The ring of light is most visible when most of Venus is still within the disc of the Sun;
2. The lower half of the ring is brighter than the upper half.
The photos were intentionally over-exposed to bring out the ring of light.
Figure 1--4: The ring of light is most evident immediately after the third contact. And the lower half of the ring is more prominent.
Figure 1: 7:07 EDT. 1/15 second, F3.8, f19.1mm, ISO 200, white balance cloudy
Figure 2: 7:08 EDT. F3.8, f19.1mm, ISO 200.
Figure 3: 7:08 EDT. F3.3, f15.0mm, ISO 200.
Figure 4: 7:09 EDT. F3.3, f15.0mm, ISO 200.

 [Figure 1,2,3,4] The ring of light (aureole) shows Venus has an atmosphere
[Figure 1,2,3,4] The ring of light (aureole) shows Venus has an atmosphere
Figure 5--8: The ring of light gradually disappears as Venus moves further out of the Sun. Again the lower half is relatively more visible.
Figure 5: 7:10 EDT. 1/15 second, F3.3, f15.0mm, ISO 400
Figure 6: 7:10 EDT. 1/60 second, F3.8, f19.3mm, ISO 800
Figure 7: 7:11 EDT. 1/60 second, F3.8, f19.3mm, ISO 800
Figure 8: 7:12 EDT. 1/30 second, F3.8, f19.3mm, ISO 800

 [Figure 5,6,7,8] The ring of light gradually disappears as Venus moves out.
[Figure 5,6,7,8] The ring of light gradually disappears as Venus moves out.
Figure 9--12: The ring of light has all but disappeared after Venus is half way out.
Figure 9: 7:16 EDT. 1/30 second, F5.1, f31.0mm, ISO 800
Figure 10: 7:23 EDT. 1/30 second, F5.1, f31.0mm, ISO 400
Figure 11: 7:23 EDT. 1/30 second, F5.1, f31.0mm, ISO 800
Figure 12: 7:25 EDT. 1/15 second, F5.1, f31.0mm, ISO 800

 [Figure 9,10,11,12] The ring of light disappeared after Venus is half way out.
[Figure 9,10,11,12] The ring of light disappeared after Venus is half way out.


Third contact. No obvious 'black drop'. Composite of six photos. 7:04 -- 7:06 EDT. 1/125 second, F5.1, f31mm, ISO 200, white balance cloudy.

 Contact III
Contact III


Venus Transit 2004/6/8 6:27 EDT. 1/177 second, F3.7, f8.2mm, ISO 200, white balance cloudy.

 Venus Transit 2004/6/8 6:27 EDT.
Venus Transit 2004/6/8 6:27 EDT.


All images on this page are taken with the following settings: Baader Astrosolar filter, Celestron star hopper 8"/f6 Dob, Scopetronix 18mm eyepiece/adapter, Nikon coolpix 995 digital camera. From Green Tree, Pittsburgh, PA, USA. The exquisite black 'EXPRESS' bag at the rear end of the scope tastefully blocks ambient light, adding an elegant touch to the whole setup :-)

 Telescope Setting
Telescope Setting


Kavan Ratnatunga, an astronomy professor at Carnegie Mellon university, traveled to Egypt for the transit and has this interesting story .

<  
Home   /  
Astronomy   /  
Sun   /  
Venus Transit 2004
>  

Google
Tip: to search within my pages only, keep inurl:zhuxj in your query. For example, inurl:zhuxj venus transit.

All images by Jerry Xiaojin Zhu unless noted otherwise. Feel free to use them for your personal enjoyment. For other usage please contact the author at jerryzhu@gmail.com