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Pi1 Ursae Majoris ( Pi1 UMa, π¹ Ursae Majoris, π¹ UMa) is a yellow G-type main sequence dwarf with a mean apparent magnitude of +5.63. It is approximately 46.8 light years from Earth, [1] and is a relatively young star with an age of about 200 million years. [11]
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Surface of the red giant star π1 Gruis. [1] π1 Gruis ( Pi1 Gruis) is a semiregular variable star in the constellation Grus around 530 light-years from Earth. It forms a close naked-eye double with π 2 Gru four arc-minutes away. π 1 Gruis is an asymptotic giant branch (AGB) star of spectral type S5. It is one of the brightest members of a ...
Pi Aquarii, Latinized from π Aquarii, is the Bayer designation for a binary star in the equatorial constellation of Aquarius. This system has an apparent visual magnitude of a mean apparent magnitude of +4.57. [4] Based upon parallax measurements, it is located at a distance of roughly 780 light-years (240 parsecs) from Earth. [1]
The corresponding antibonding, or π* ("pi-star") molecular orbital, is defined by the presence of an additional nodal plane between these two bonded atoms. Multiple bonds [ edit ] A typical double bond consists of one sigma bond and one pi bond; for example, the C=C double bond in ethylene (H 2 C=CH 2 ).
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Pi Orionis (π Ori, π Orionis) is a group of fairly widely scattered stars in the constellation Orion that constitute the asterism Orion's Shield or Orion's Bow. [1] They form an exception to the general rule that stars that share the same Bayer designation are close together: π 1 is nearly 9° north of π 6 ( Tau Eridani is an even more ...
Pi1 Cygni ( π1 Cygni, abbreviated Pi1 Cyg, π1 Cyg) is a binary star [5] in the northern constellation of Cygnus. It is visible to the naked eye, having a combined apparent visual magnitude of 4.66. [2] The distance to this system can be roughly gauged by its annual parallax shift of 1.89 mas, [1] which yields a separation of around 1,700 ...