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Cassiopeia Constellations Astronomy Information

Cassiopeia is one of the rare constellations which its name is inspired by the name of someone, and in this case, it is the queen Cassiopeia in Greek mythology. She was arrogant and thought her beauty was unrivalled in the ancient myths. This constellation was also listed in the 48 constellations of Ptolemy, and still makes the list among the 88 modern constellations.

The image credits go to IAU.

Alpha Cassiopeiae (Schedar, derived from the Arabic word Al Sadr which means breast) is the brightest star of Cassiopeia (of magnitude 2.2), but there are occasions during which it is outshone by the variable Gamma Cassiopeiae (of magnitude 1.6). Alpha Cassiopeiae is a multiple stellar system and is composed of four stars. Beta Cassiopeiae (commonly called Caph that means hand) is a white-hued star fairly close to Earth (55 light-years away). Although perhaps not that famous, Cassiopeia contains some of the brightest stars discovered or some generally interesting cases. Among the bright stars, we mention the yellow hypergiants Rho Cassiopeiae and V509 Cassiopeiae and the white hypergiant 6 Cassiopeiae. The famous Tycho Brahe’s supernova which flared in 1572 is also located in Cassiopeia constellation. This is a remarkable supernova because it was among the eight supernovae visible to naked eye historically. A supernova is the energetic explosion of a star which its afterglow can be seen for days (depending on how energetic it would be).

The variable stars of Cassiopeia are: 50 Cassiopeiae,  Zeta Cassiopeiae,  Theta Cassiopeiae,  Iota Cassiopeiae (a triple star system),  Omicron Cassiopeiae (another triple star), Eta Cassiopeiae (which is a spectroscopic binary). The last one is also an RS Canum Venaticorum variable which means the binary components own active chromospheres leading to the emergence of stellar spots.  Kappa Cassiopeiae is another particular star of Cassiopeia which is a runaway star, and a blue supergiant. Due to its strong magnetic field and wind of particles, it is surrounded by a visible bow shock colliding with the interstellar gas and dust (see figure below). This bow shock is relatively huge in dimension, it covers an area of 12 light-years long and 1.8 light-years wide.

 Kappa Cassiopeiae imaged by Spitzer infrared image (NASA/JPL-Caltech).

Cassiopeia A which is the brightest extrasolar radio source in the sky is also located in this constellation and is a supernova remnant. There are fourteen stellar systems that host exoplanets in Cassiopeia constellation. Since a rich section of Milky Way flows through Cassiopeia constellation, it contains several open clusters:  M52 (NGC 7654), NGC 457NGC 457NGC 663, and M103 (NGC 581).

There are also binary stars belonging to Cassiopeia constellation: Sigma Cassiopeiae and AO Cassiopeiae.  Psi Cassiopeiae is a triple star belonging to this constellation, located 193 light-years from Earth. There are also yellow hypergiants which are among the most luminous stars of our galaxy: Rho Cassiopeiae and  V509 Cassiopeiae.  PZ Cassiopeiae which is one of the largest stars known to date also resides in Cassiopeia constellation.

PZ Cassiopeiae (upper right) imaged by WISE infrared.

The irregular galaxy IC 10 is also located in the Cassiopeia constellation, and is a starburst galaxy which means it is a star factory at a high rate.

IC 10, the Local Group dwarf galaxy (PI: Philip Massey, Lowell Observatory).

Heart Nebula and Soul Nebula are neighboring nebulae in Cassiopeia constellation.

Soul Nebula. The image credits go to NASA.
Heart Nebula photographed by ASI2600mc-pro.

Leo Star Constellations Astronomy Information

Leo means lion in Latin and is among the twelve zodiac signs. In Greek mythology, this was the lion killed by the hero Heracles. Leo is one of those rare constellations that hold a zodiac sign under its name and also has many bright stars.  Alpha Leonis is a very bright star in the night sky (1.35 in magnitude) and is a double star divisible even in binoculars. Beta Leonis (Denebola, the lion’s tail in Arabic) is another bright star (2.2 in magnitude) of the constellation. Gamma Leonis is a binary star accompanied by a third optical component. Note that the structure of this star is different from Zeta Leonis which is an optical triple star. Iota Leonis is another binary star in the constellation which is divisible in an amateur telescope. Tau Leonis is a dimmer double star.  R Leonis is a red giant, Mira variable star, and  Wolf 359 (CN Leonis) is a flare star that periodically brightens up in the night sky. CW Leo (IRC +10216) is a carbon star that is the brightest star observed at the infrared N-band (10 μm wavelength).

The image credits go to IAU.

Leo is also home to many bright galaxies:  Messier 65 and Messier 66 make up for the Leo Triplet along with NGC 3628Messier 95Messier 96, and Messier 105. Leo also owns some of the most massive structures in the universe, large quasar groups called Clowes–Campusano LQGU1.11U1.54, and the Huge-LQG.

 NGC 3628, Sarah’s galaxy, or the Hamburger galaxy captured by ESO’s VLT.
M66 captured by ESO’s VLT.
M95 captured by Spitzer.
NGC 3368 captured by ESO’s VLT.
NGC2903 captured by ESA/NASA HST.

Hercules Star Constellations Astronomy Information

Hercules is named after the Roman mythological hero, and it is the fifth-largest constellation among the 88 modern constellations (covers 1225.1 square degrees and 2.970% of the night sky). Although the constellation has no particularly bright stars, it possesses some stars visible to naked eye (above magnitude 4). Alpha Herculis is one of these stars and is a triple star. Beta Herculis (Kornephoros, a yellow giant) is the brightest star in Hercules constellation. Delta Herculis is a double star (separable even in small amateur telescopes, same as Gamma Herculis and  Kappa Herculis). 30 Herculis (g Herculis) and  68 Herculis (u Herculis) are variable stars of Hercules. There are also fifteen stars that host planets in Hercules constellation: 14 Herculis (hosting two planets), HD 149026 (hosts a hot Jupiter), HD 154345 (hosts a long-period planet that takes more than 9 years to complete its orbit), HD 164922 (hosting a long period Saturn-like planet), HD 147506 (hosts a massive planet, of 8.6 Jupiter masses), HD 155358 (hosts two planets), GSC 03089-00929 (hosts one planet), Gliese 649 (owns a saturnian planet), HD 156668 (hosts one plent), HD 164595 (hosts one planet).

The image credits go to IAU.

Among the constellation’s deep-sky objects, we can name its globular clusters (M13, NGC 6229, and M92) and a number of beautiful planetary nebulae (Abell 39 and NGC 6210). As its name suggests, the largest structure in the visible universe, the Hercules–Corona Borealis Great Wall, lies in this constelaltion. By visible univeres we mean the space in which photons have had the time to travel so far from the beginning of time. This space that has been shed light on is observable today. There is also a world (containing many galaxies) located in Hercules cluster called  Hercules Cluster (Abell 2151).  

Abell 39 captured from the Mount Lemmon SkyCenter using the Schulman 32 inch Telescope.
NGC 6210 captured by ESA/NASA HST.

Apus Star Constellations Astronomy Information

A tiny constellation in the southern sky, Apus represents a bird-of-paradise. Its name literally means “without feet”. In the western world at the time of Bayer, who first identified this constellation, the only existing specimen of birds-of-paradise there had their wings and feet removed. French astronomer, Lacaille, gave this constellation’s brighter stars Bayer Designations for the first time in 1756 and also cut the tail of this bird-of-paradise. Alpha Apodis is an orange giant with a diameter 48 times larger than that of the Sun. Beta Apodis is another giant star in this constellation, with a radius 11 times larger than that of the Sun. Gamma Apodis is a yellow giant star of the constellation, and Delta Apodis is a binary stellar system, consisting of an orange giant and a red giant star. No Apodis is the beating heart of the constellation, it’s a variable pulsating star. Its magnitude changes between 5.71 and 5.95, with pulsation periods of 26.2 and 26.6 days respectively. With the help of Doppler spectroscopy, two exoplanets hosted by two stars of these constellations were discovered. This method is being used very frequently these days in astronomy for discovering exoplanets. We encourage the curious readers to visit this Wikipedia page to know more about this powerful method – it contains so many physical concepts involved. Milky Way covers most of this constellation, thus, no galaxies here. But there are two globular clusters, NGC 6101 and IC 4499 namely, in Apus.

Image credits go to universetoday.com.

Globular clusters are spherical crowds of stars orbiting a galactic core. They owe their spherical shape to their stars being too strongly bound to each other by gravity. This also gives them a dense core at the center (a beautiful, nice example of this is Messier 80 located in the Scorpius constellation). Globus is Latin means a small sphere. Globular clusters are found in the halo of galaxies. Open clusters, which contain coming stars (loosely gravitationally bound), are found in the disk of galaxies on the other hand.

Messier 80 located in the Scorpius constellation. Image credits go to Hubble space telescope.
Causes of Zika Virus Outbreak

Causes Of Zika Virus Outbreak

Zika is a mosquito-borne virus that in its urban cycle transmits between Aedes species mosquitoes and humans. Aedes can live in close contact with Humans. They preferentially feed on human blood. They can live in our house and leave to lay their eggs in standing water outside human residences. They are now understood to be other less common ways that Zika can be transmitted, vertically from mother to child during pregnancy, through sexual contact, and transfusion transmission. 

So Zika historically is an African virus that was first isolated in Uganda in 1947. And then it caused sporadic and poorly-described human disease starting, the first human disease was recognized in west Africa in the 1960s. So from the ’60s until about 10 years ago, Zika caused small and focal outbreaks in Africa and Asia. But as you know starting in 2014, Zika was introduced into the Americas.

The virus has been introduced into 50+ new countries and territories in the Americas. So what happens when there is a Zika case that’s reported to CDPH, the Mosquito and Vector Control districts go out to the case’s residence, try to kill adult mosquitoes in the area and then remove the standing water containers to eliminate breeding sites.

Which mosquitoes are responsible for transmitting Zika? And this is epidemiologically-relevant because if you want to target vector control without a licensed vaccine, you have to know which species are transmitting the virus. After all, mosquitoes have different ecologies and different feeding behaviors and they also have different distributions.

One reason why it’s important to know whether North American Culex can transmit Zika is you’ll notice that their range extends much, especially for Culex pipiens much further north than the Aedes species. So when that press release came out, a lot of the Mosquito and Vector Control districts around the United States expressed a lot of concern in understanding whether there was a big host switch. So how do we know which mosquito species are competent vectors? As you know there are hundreds of different mosquito species around the world. And to the naked eye, they look very similar, but they are very different. And they’re not all capable of transmitting human and animal pathogens.

So there are four criteria that a mosquito species has to fulfill to be considered a competent vector. They have to be abundant, they have to survive long enough to transmit, they have to feed frequently on competent vertebrate hosts. So these are criteria that we can establish in field entomological surveys.

The fourth criterion is the one that researchers have been looking at which is that you can show in a laboratory setting that certain species are capable of transmitting the virus. This is a cross-section of a mosquito. Researchers ingest an infectious blood meal that goes into the mosquito stomach or the midgut. The virus has to infect the midgut epithelium and then disseminate onto the other side of the midgut into the open circulatory cavity of the mosquito and be in the liquid that bathes it, which is called the demolish. So that then it can infect the secondary target organs which in the case of a transition-competent mosquito would include the salivary glands. So that the virus will then be excreted into the saliva so that when the mosquito refeeds, she transmits it into a new host.

This period takes a certain amount of time in a mosquito. So the way we do this experimentally is we take viremic mice that have been inoculated with Zika, and then are at their peak of viremia. We anesthetize them and then we present them to cohorts of female mosquitoes of the different species that we’re interested in studying. 

Then after the period that the virus moves through the mosquito body, we tear off the legs and the wings of the still-living mosquito and we inject the proboscis into a tube filled with liquid which stimulates salivation. So we’re essentially milking the mosquitoes. If we detect the Zika virus or RNA in the expectorant, we know that that species is transmission-competent. 

There’s another interesting phenomenon that’s been observed which is that within a given mosquito species, there can be regional variations or geographic variations in the capacity for those mosquitoes to transmit.

So there’s also been an interest in understanding whether Aedes aegypti from one place is also as transmission-competent as Aedes aegypti from another place. This data synthesizes the field of vector transmission studies where you can see groups from various places have been collecting their local mosquitoes and then looking at the capacity of them to transmit.

Lab data confirms that Aedes aegypti from all over the world are capable of transmitting Zika as is Aedes albopictus from the one study in Germany. Looking at the Culex data, it is almost uniform that not a single mosquito was tested and unlike invertebrate studies, we have lots more mosquitoes, so our cohort sizes are often in 50 to 100. We can say out of the thousands of Culex that have been tested from around the world, they’re not transmission-competent, save for this one outlier study which I think could be potentially interesting.

So barring any methodological issues with the paper, this could be a case that there is something different about these Chinese Culex quinquefasciatus mosquitoes that enables them to transmit Zika. Alternately there could be something different about the Zika virus strain that was used in that Chinese study. It was an Asian lineage genotype virus, the same that’s circuiting in the Americas that was in a traveler returning to China. But overall, the burden of evidence shows that Zika has not shifted to use Culex mosquitoes as vectors.

Another question that scientists have been interested in, as you know there’s been a lot of curiosity as to what factors have promoted the emergence of Zika. On the mosquito side, one question is whether the spread of the Asian lineage virus has been promoted by enhanced transmissibility by the primary vector in most places, Aedes aegypti.

To address this question, Scientists took an ancestral virus in the Asian lineage from 1966 in Malaysia that was the low passage and compared that in the vector-competent experiment, side-by-side with the contemporary Puerto Rican strain.

They used an Uganda strain from 1947 and a Senegalese strain from 1997. Data shows 40% and 60% of the mosquitoes that fed on the mouse were capable of transmitting between seven and 14 days post-feed, but there was no significant strain-specific difference. This refutes the idea that the emerging Asian lineage Zika is more transmissible than its Asian lineage progenitor strain. So in fact the emerging viruses are doing worse in aegyptia than the African lineage strains.

So the reasons for having animal models of infectious diseases, We think are pretty obvious, but we feel that the placental and neurological development of nonhuman primates is closer to humans than that of mice. So even in the last year and a half, the Zika non-human primate field has rapidly advanced and globally know a lot already. Please find latest development from WHO on ZIKA virus here