| Observation data Epoch J2000.0 |
|
|---|---|
| Constellation (pronunciation) |
Ophiuchus |
| Right ascension | 16h 32m 51. The Henry Draper Catalogue ( HD) is an Astronomical Star catalogue published between 1918 and 1924 giving Spectroscopic classifications In Astronomy, an epoch is a moment in time used as a reference for the Orbital elements of a Celestial body. In Astronomy, an epoch is a moment in time used as a reference for the Orbital elements of a Celestial body. In common usage a constellation is a group of celestial bodies that are connected together in some arrangement typically stars to form a visible figure or picture Each culture has its own Constellations usually based on Mythology. Ophiuchus (Ὀφιοῦχος ˌɒfiːˈuːkəs is one of the 88 Constellations and was also one of the 48 listed by Ptolemy. Right ascension (abbrev RA; symbol α) is the Astronomical term for one of the two Coordinates of a point on the Celestial sphere 0498s |
| Declination | +02º 05' 05. In Astronomy, declination (abbrev dec or δ) is one of the two coordinates of the Equatorial coordinate system, the other being either 3954″ |
| Apparent magnitude (V) | 7. The apparent magnitude ( m) of a celestial body is a measure of its Brightness as seen by an observer on Earth, normalized to the value 90 |
| Absolute magnitude (V) | 3. In Astronomy, absolute magnitude (also known as absolute visual magnitude) is the Apparent magnitude an object would have if it were at a standard 89 |
| Distance | 207 ly (63. The cosmic distance ladder (also known as the Extragalactic Distance Scale) is the succession of methods by which astronomers determine the Distances to celestial A light-year or light year (symbol ly) is a unit of Length, equal to just under ten trillion Kilometres As defined by 5 pc) |
| Spectral type | G0 |
| Other designations | |
HD 149143 is a star located in Ophiuchus constellation that has spectral type of G0 located at a distance of 207 ly from us. History The first direct measurements of an object at interstellar distances were undertaken by German Astronomer Friedrich Wilhelm Bessel in 1838 In Astronomy, stellar classification is a classification of Stars based initially on photospheric temperature and its associated Spectral characteristics A star catalogue, or star catalog, is an Astronomical catalogue that lists Stars In Astronomy, many stars are referred to simply by catalogue In Astronomy, Durchmusterung or Bonner Durchmusterung ( BD) is the usual name for three comprehensive astrometric Star catalogues The Hipparcos and Tycho Catalogues (Tycho-1 are the primary products of the European Space Agency 's astrometric mission Hipparcos. The Smithsonian Astrophysical Observatory Star Catalog is an astrometric Star catalogue. A star is a massive luminous ball of plasma. The nearest star to Earth is the Sun, which is the source of most of the Energy on Earth Ophiuchus (Ὀφιοῦχος ˌɒfiːˈuːkəs is one of the 88 Constellations and was also one of the 48 listed by Ptolemy. In Astronomy, stellar classification is a classification of Stars based initially on photospheric temperature and its associated Spectral characteristics The cosmic distance ladder (also known as the Extragalactic Distance Scale) is the succession of methods by which astronomers determine the Distances to celestial Its apparent magnitude of the star is 7. The apparent magnitude ( m) of a celestial body is a measure of its Brightness as seen by an observer on Earth, normalized to the value 9 (binocular object) and the absolute magnitude is 3. In Astronomy, absolute magnitude (also known as absolute visual magnitude) is the Apparent magnitude an object would have if it were at a standard 9 (naked-eye object).
| Extrasolar planet | List of extrasolar planets | |
|---|---|---|
| Orbital elements | ||
| Semimajor axis | (a) | 0. An extrasolar planet, or exoplanet, is a Planet beyond the Solar System, orbiting around other Stars As of September 2008 312 The following are lists of stars with confirmed Extrasolar planets. The elements of an orbit are the parameters needed to specify that Orbit uniquely given a model of two point-masses obeying the Newtonian laws of motion and the In Geometry, the semi-major axis (also semimajor axis) is used to describe the dimensions of ellipses and hyperbolae 0531 AU |
| Eccentricity | (e) | 0 |
| Orbital period | (P) | 4. The astronomical unit ( AU or au or au or sometimes ua) is a unit of Length based on the distance from the Earth to the In Astrodynamics, under standard assumptions, any Orbit must be of Conic section shape The orbital period is the time taken for a given object to make one complete Orbit about another object 07±0. 70 d |
| Angular distance | (θ) | 0. A day (symbol d is a unit of Time equivalent to 24 Hours and the duration of a single Rotation of planet Earth with respect to the In Mathematics (in particular Geometry and Trigonometry) and all Natural sciences (including astronomy geophysics etc the angular distance 836 mas |
| Longitude of periastron |
(ω) | 0° |
| Time of periastron | (T0) | 2453483. A minute of arc, arcminute, or MOA is a unit of angular measurement, equal to one sixtieth (1/60 of one degree. In Astrodynamics, the longitude of the periapsis (symbolized \varpi of an orbiting body is the Longitude (measured from the point of the vernal equinox In Celestial mechanics, an apsis, plural apsides (ˈæpsɨdɪːz is the point of greatest or least distance of the Elliptical orbit of an object from In Celestial mechanics, an apsis, plural apsides (ˈæpsɨdɪːz is the point of greatest or least distance of the Elliptical orbit of an object from 9±1. 2 JD |
| Semi-amplitude | (K) | 149. The Julian date (JD is the interval of time in days and fractions of a day since 4713 B Amplitude is the magnitude of change in the oscillating variable with each Oscillation, within an oscillating system 6±3 m/s |
| Physical characteristics | ||
| Mass | (m) | >1. Mass is a fundamental concept in Physics, roughly corresponding to the Intuitive idea of how much Matter there is in an object 33 MJ |
| Discovery information | ||
| Discovery date | 2005 | |
| Discoverer(s) | Da Silva et al. Jupiter mass is the unit of Mass equal to one Jupiter (18986 × 1027 kg, 317 Year 2005 ( MMV) was a Common year starting on Saturday (link displays full calendar of the Gregorian calendar. | |
| Detection method | Doppler Spectroscopy | |
| Discovery status | Published | |
HD 149143 b is a 2005 exoplanet that has a minimum mass (unknown inclination) of 1. Any Planet is an extremely faint light source compared to its parent Star. Doppler spectroscopy, also known as Radial velocity measurement is a spectroscopic method for finding Extrasolar planets It involves the observation An extrasolar planet, or exoplanet, is a Planet beyond the Solar System, orbiting around other Stars As of September 2008 312 The term minimum mass refers to the detected objects with a lower-bound calculated Mass. Inclination in general is the Angle between a Reference plane and another plane or axis of direction 33 Jupiter mass. Jupiter mass is the unit of Mass equal to one Jupiter (18986 × 1027 kg, 317 Its orbital period is 0. The orbital period is the time taken for a given object to make one complete Orbit about another object 35 megaseconds and the semimajor axis would be 7. To help compare Orders of magnitude of different times this page lists times between 106 seconds and 107 seconds (approximately 11 In Geometry, the semi-major axis (also semimajor axis) is used to describe the dimensions of ellipses and hyperbolae 94 gigameters. The metre or meter is a unit of Length. It is the basic unit of Length in the Metric system and in the International As it is tyical for a lot of hot Jupiters, its orbital eccentricity value is practically zero and has high semi-amplitude of 150 meters per second. Hot Jupiters (also called roasters, epistellar jovians, pegasids or pegasean planets) are a class of Extrasolar planets whose In Astrodynamics, under standard assumptions, any Orbit must be of Conic section shape Amplitude is the magnitude of change in the oscillating variable with each Oscillation, within an oscillating system