Michiana Astronomical Society Inc., October 2014

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Regular meeting of Michiana Astronomical Society Inc., with some events and related travel items since previous meeting. Upcoming events include partial solar eclipse, astronomy talk at ND, guest speaker at November MAS meeting, and Santa Parade at Eddy Street Commons.

Ciencias

Oct. 20, 2014
Regular Meeting
Agenda
•Treasurer’s report
•Events since last meeting
•Announcements
•Guest Speaker: Jim Hopkins
Constellations in Autumn &
Winter

October 28
The Notre Dame Club of St. Joseph Valley Hesburgh
Lecture is scheduled for Tuesday, October 28, at 7:00
p.m. in Room 101 of the Jordan Hall of Science. This
year’s guest speaker will be Dr. Peter Garnavich. His
presentation is entitled “The Expanding Universe and
Large Telescopes.” Dr. Garnavich was a member of the
research team that won the Nobel Prize in Physics for
their discovery of the accelerating expansion of the
universe. A reception will follow Dr. Garnavich’s
presentation. Weather permitting, there will be an
opportunity to go to the Observatory on Jordan Hall and
look through the telescopes.

November 17
Guest speaker at November MAS meeting will be Belinda
Cheeseboro, who did a summer internship at Kitt Peak where
she was studying active galactic nuclei using WISE data.

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Bollworms are among the most damaging pests in cotton cultivation, affecting the bolls where the cotton fibers are formed. There are several species of bollworms, each capable of causing significant yield loss and quality degradation if not effectively managed. Here’s a detailed look at the primary bollworm species affecting cotton: Cotton Bollworm (Helicoverpa armigera): Also known as the corn earworm or the Old World bollworm, this pest is found in many regions around the world. It is highly polyphagous (feeds on many different plants) and poses a threat not only to cotton but also to maize, tomatoes, and legumes. The larvae bore into the cotton bolls, feeding on the developing seeds and fibers, which can lead to boll rot. Pink Bollworm (Pectinophora gossypiella): A significant pest of cotton, the pink bollworm larvae infest the cotton bolls, feeding on the seeds and lint. This can severely damage or destroy the bolls. In regions where pink bollworms are prevalent, they have been a major driver for the adoption of genetically engineered Bt cotton, which expresses a bacterium gene toxic to certain insects. Tobacco Budworm (Heliothis virescens): Closely related to the cotton bollworm, the tobacco budworm primarily attacks tobacco but is also a common pest in cotton. It primarily damages the flowers and bolls of the cotton plant. Differentiating between the tobacco budworm and the cotton bollworm based on appearance can be challenging, but it is crucial for effective management. American Bollworm (Helicoverpa zea): Known in some regions as the corn earworm, it is similar in behavior to Helicoverpa armigera and poses a threat to a variety of crops, including cotton. The larvae attack the cotton bolls, leading to direct damage to the cotton lint and seeds. Management Strategies: Cultural Controls: Crop rotation, destruction of crop residues, and deep plowing can help break the pest’s life cycle. Timing of planting can also be adjusted to avoid peak pest infestation. Biological Controls: Natural enemies like Trichogramma wasps, which parasitize bollworm eggs, and predators such as lacewings and ladybugs can be encouraged. Bacillus thuringiensis (Bt) products can also be sprayed, which are particularly effective against young larvae. Chemical Controls: Insecticides may be required when infestation levels exceed economic thresholds. However, resistance management must be considered, alternating modes of action to avoid developing resistance. Genetic Approaches: Bt cotton, genetically modified to express Bacillus thuringiensis toxin, has been highly effective in controlling bollworms and has dramatically reduced the reliance on chemical insecticides. Monitoring and Scouting: Regular field scouting and using pheromone traps to monitor adult populations can help in timely and targeted application of control measures. The effective management of bollworms often requires an integrated approach

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Context. WASP-76 b has been a recurrent subject of study since the detection of a signature in high-resolution transit spectroscopy data indicating an asymmetry between the two limbs of the planet. The existence of this asymmetric signature has been confirmed by multiple studies, but its physical origin is still under debate. In addition, it contrasts with the absence of asymmetry reported in the infrared (IR) phase curve. Aims. We provide a more comprehensive dataset of WASP-76 b with the goal of drawing a complete view of the physical processes at work in this atmosphere. In particular, we attempt to reconcile visible high-resolution transit spectroscopy data and IR broadband phase curves. Methods. We gathered 3 phase curves, 20 occultations, and 6 transits for WASP-76 b in the visible with the CHEOPS space telescope. We also report the analysis of three unpublished sectors observed by the TESS space telescope (also in the visible), which represents 34 phase curves. Results. WASP-76 b displays an occultation of 260±11 and 152±10 ppm in TESS and CHEOPS bandpasses respectively. Depending on the composition assumed for the atmosphere and the data reduction used for the IR data, we derived geometric albedo estimates that range from 0.05 ± 0.023 to 0.146 ± 0.013 and from <0.13 to 0.189 ± 0.017 in the CHEOPS and TESS bandpasses, respectively. As expected from the IR phase curves, a low-order model of the phase curves does not yield any detectable asymmetry in the visible either. However, an empirical model allowing for sharper phase curve variations offers a hint of a flux excess before the occultation, with an amplitude of ∼40 ppm, an orbital offset of ∼−30◦ , and a width of ∼20◦ . We also constrained the orbital eccentricity of WASP-76 b to a value lower than 0.0067, with a 99.7% confidence level. This result contradicts earlier proposed scenarios aimed at explaining the asymmetry observed in high-resolution transit spectroscopy. Conclusions. In light of these findings, we hypothesise that WASP-76 b could have night-side clouds that extend predominantly towards its eastern limb. At this limb, the clouds would be associated with spherical droplets or spherically shaped aerosols of an unknown species, which would be responsible for a glory effect in the visible phase curves.

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Michiana Astronomical Society Inc., October 2014

1. Oct. 20, 2014 Regular Meeting Agenda •Treasurer’s report •Events since last meeting •Announcements •Guest Speaker: Jim Hopkins Constellations in Autumn & Winter

7. September 18

10.

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16.

17. October 7

18. Oct October 8

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22. Credit: Steve Accuosti

23. Credit: Candi Tyler

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26. October 16

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28. Credit: Candi Tyler

29. Credit: Candi Tyler

30. Upcoming Events…

31. October 23

32. October 23

33.

34. October 23

35. October 28 The Notre Dame Club of St. Joseph Valley Hesburgh Lecture is scheduled for Tuesday, October 28, at 7:00 p.m. in Room 101 of the Jordan Hall of Science. This year’s guest speaker will be Dr. Peter Garnavich. His presentation is entitled “The Expanding Universe and Large Telescopes.” Dr. Garnavich was a member of the research team that won the Nobel Prize in Physics for their discovery of the accelerating expansion of the universe. A reception will follow Dr. Garnavich’s presentation. Weather permitting, there will be an opportunity to go to the Observatory on Jordan Hall and look through the telescopes.

36. November 17 Guest speaker at November MAS meeting will be Belinda Cheeseboro, who did a summer internship at Kitt Peak where she was studying active galactic nuclei using WISE data.

37. D December 6

Michiana Astronomical Society Inc., October 2014

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